Author: "Park, H. -S." / Database: OAIster - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"Park, H. -S."' showing total 242 results

Start Over Author "Park, H. -S." Database OAIster

242 results on '"Park, H. -S."'

1. Measurements of low energy nuclear recoil quenching factors for Na and I recoils in the NaI(Tl) scintillator

Author: Lee, S. H., Joo, H. W., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Ko, Y. J., Lee, H. S., Lee, J. Y., Park, H. S., Yoon, Y. S., Lee, S. H., Joo, H. W., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Ko, Y. J., Lee, H. S., Lee, J. Y., Park, H. S., and Yoon, Y. S.
Abstract: Elastic scattering off nuclei in target detectors, involving interactions with dark matter and coherent elastic neutrino nuclear recoil (CE$\nu$NS), results in the deposition of low energy within the nuclei, dissipating rapidly through a combination of heat and ionization. The primary energy loss mechanism for nuclear recoil is heat, leading to consistently smaller measurable scintillation signals compared to electron recoils of the same energy. The nuclear recoil quenching factor (QF), representing the ratio of scintillation light yield produced by nuclear recoil to that of electron recoil at the same energy, is a critical parameter for understanding dark matter and neutrino interactions with nuclei. The low energy QF of NaI(Tl) crystals, commonly employed in dark matter searches and CE$\nu$NS measurements, is of substantial importance. Previous low energy QF measurements were constrained by contamination from photomultiplier tube (PMT)-induced noise, resulting in an observed light yield of approximately 15 photoelectrons per keVee (kilo-electron-volt electron-equivalent energy) and nuclear recoil energy above 5 keVnr (kilo-electron-volt nuclear recoil energy). Through enhanced crystal encapsulation, an increased light yield of around 26 photoelectrons per keVee is achieved. This improvement enables the measurement of the nuclear recoil QF for sodium nuclei at an energy of 3.8 $\pm$ 0.6 keVnr with a QF of 11.2 $\pm$ 1.7%. Furthermore, a reevaluation of previously reported QF results is conducted, incorporating enhancements in low energy events based on waveform simulation. The outcomes are generally consistent with various recent QF measurements for sodium and iodine.
Published: 2024

2. Background study of the AMoRE-pilot experiment

Author: Agrawal, A., Alenkov, V. V., Aryal, P., Beyer, J., Bhandari, B., Boiko, R. S., Boonin, K., Buzanov, O., Byeon, C. R., Chanthima, N., Cheoun, M. K., Choe, J. S., Choi, Seonho, Choudhury, S., Chung, J. S., Danevich, F. A., Djamal, M., Drung, D., Enss, C., Fleischmann, A., Gangapshev, A. M., Gastaldo, L., Gavrilyuk, Yu. M., Gezhaev, A. M., Gileva, O., Grigorieva, V. D., Gurentsov, V. I., Ha, C., Ha, D. H., Ha, E. J., Hwang, D. H., Jeon, E. J., Jeon, J. A., Jo, H. S., Kaewkhao, J., Kang, C. S., Kang, W. G., Kazalov, V. V., Kempf, S., Khan, A., Khan, S., Kim, D. Y., Kim, G. W., Kim, H. B., Kim, Ho-Jong, Kim, H. J., Kim, H. L., Kim, H. S., Kim, M. B., Kim, S. C., Kim, S. K., Kim, S. R., Kim, W. T., Kim, Y. D., Kim, Y. H., Kirdsiri, K., Ko, Y. J., Kobychev, V. V., Kornoukhov, V., Kuzminov, V. V., Kwon, D. H., Lee, C. H., Lee, DongYeup, Lee, E. K., Lee, H. J., Lee, H. S., Lee, J., Lee, J. Y., Lee, K. B., Lee, M. H., Lee, M. K., Lee, S. W., Lee, Y. C., Leonard, D. S., Lim, H. S., Mailyan, B., Makarov, E. P., Nyanda, P., Oh, Y., Olsen, S. L., Panasenko, S. I., Park, H. K., Park, H. S., Park, K. S., Park, S. Y., Polischuk, O. G., Prihtiadi, H., Ra, S., Ratkevich, S. S., Rooh, G., Sari, M. B., Seo, J., Seo, K. M., Sharma, B., Shin, K. A., Shlegel, V. N., Siyeon, K., So, J., Sokur, N. V., Son, J. K., Song, J. W., Srisittipokakun, N., Tretyak, V. I., Wirawan, R., Woo, K. R., Yeon, H. J., Yoon, Y. S., Yue, Q., Agrawal, A., Alenkov, V. V., Aryal, P., Beyer, J., Bhandari, B., Boiko, R. S., Boonin, K., Buzanov, O., Byeon, C. R., Chanthima, N., Cheoun, M. K., Choe, J. S., Choi, Seonho, Choudhury, S., Chung, J. S., Danevich, F. A., Djamal, M., Drung, D., Enss, C., Fleischmann, A., Gangapshev, A. M., Gastaldo, L., Gavrilyuk, Yu. M., Gezhaev, A. M., Gileva, O., Grigorieva, V. D., Gurentsov, V. I., Ha, C., Ha, D. H., Ha, E. J., Hwang, D. H., Jeon, E. J., Jeon, J. A., Jo, H. S., Kaewkhao, J., Kang, C. S., Kang, W. G., Kazalov, V. V., Kempf, S., Khan, A., Khan, S., Kim, D. Y., Kim, G. W., Kim, H. B., Kim, Ho-Jong, Kim, H. J., Kim, H. L., Kim, H. S., Kim, M. B., Kim, S. C., Kim, S. K., Kim, S. R., Kim, W. T., Kim, Y. D., Kim, Y. H., Kirdsiri, K., Ko, Y. J., Kobychev, V. V., Kornoukhov, V., Kuzminov, V. V., Kwon, D. H., Lee, C. H., Lee, DongYeup, Lee, E. K., Lee, H. J., Lee, H. S., Lee, J., Lee, J. Y., Lee, K. B., Lee, M. H., Lee, M. K., Lee, S. W., Lee, Y. C., Leonard, D. S., Lim, H. S., Mailyan, B., Makarov, E. P., Nyanda, P., Oh, Y., Olsen, S. L., Panasenko, S. I., Park, H. K., Park, H. S., Park, K. S., Park, S. Y., Polischuk, O. G., Prihtiadi, H., Ra, S., Ratkevich, S. S., Rooh, G., Sari, M. B., Seo, J., Seo, K. M., Sharma, B., Shin, K. A., Shlegel, V. N., Siyeon, K., So, J., Sokur, N. V., Son, J. K., Song, J. W., Srisittipokakun, N., Tretyak, V. I., Wirawan, R., Woo, K. R., Yeon, H. J., Yoon, Y. S., and Yue, Q.
Abstract: We report a study on the background of the Advanced Molybdenum-Based Rare process Experiment (AMoRE), a search for neutrinoless double beta decay (\znbb) of $^{100}$Mo. The pilot stage of the experiment was conducted using $\sim$1.9 kg of \CAMOO~ crystals at the Yangyang Underground Laboratory, South Korea, from 2015 to 2018. We compared the measured $\beta/\gamma$ energy spectra in three experimental configurations with the results of Monte Carlo simulations and identified the background sources in each configuration. We replaced several detector components and enhanced the neutron shielding to lower the background level between configurations. A limit on the half-life of $0\nu\beta\beta$ decay of $^{100}$Mo was found at $T_{1/2}^{0\nu} \ge 3.0\times 10^{23}$ years at 90\% confidence level, based on the measured background and its modeling. Further reduction of the background rate in the AMoRE-I and AMoRE-II are discussed.
Published: 2024

3. Nonproportionality of NaI(Tl) Scintillation Detector for Dark Matter Search Experiments

Author: Lee, S. M., Adhikari, G., Carlin, N., Cho, J. Y., Choi, J. J., Choi, S., Ezeribe, A. C., a, L. E. Fran., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, S. W., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, J. C., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Son, M. K., Spooner, N. J. C., Truc, L. T., Yang, L., Yu, G. H., Lee, S. M., Adhikari, G., Carlin, N., Cho, J. Y., Choi, J. J., Choi, S., Ezeribe, A. C., a, L. E. Fran., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, S. W., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, J. C., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Son, M. K., Spooner, N. J. C., Truc, L. T., Yang, L., and Yu, G. H.
Abstract: We present a comprehensive study of the nonproportionality of NaI(Tl) scintillation detectors within the context of dark matter search experiments. Our investigation, which integrates COSINE-100 data with supplementary $\gamma$ spectroscopy, measures light yields across diverse energy levels from full-energy $\gamma$ peaks produced by the decays of various isotopes. These $\gamma$ peaks of interest were produced by decays supported by both long and short-lived isotopes. Analyzing peaks from decays supported only by short-lived isotopes presented a unique challenge due to their limited statistics and overlapping energies, which was overcome by long-term data collection and a time-dependent analysis. A key achievement is the direct measurement of the 0.87 keV light yield, resulting from the cascade following electron capture decay of $^{22}$Na from internal contamination. This measurement, previously accessible only indirectly, deepens our understanding of NaI(Tl) scintillator behavior in the region of interest for dark matter searches. This study holds substantial implications for background modeling and the interpretation of dark matter signals in NaI(Tl) experiments., Comment: 12 pages, 7 figures
Published: 2024
Full Text: View/download PDF

4. X-ray imaging and electron temperature evolution in laser-driven magnetic reconnection experiments at the National Ignition Facility

Author: Valenzuela-Villaseca, V., Molina, J. M., Schaeffer, D. B., Malko, S., Griff-McMahon, J., Lezhnin, K., Rosenberg, M. J., Hu, S. X., Kalantar, D., Trosseille, C., Park, H. -S., Remington, B. A., Fiksel, G., Uzdensky, D., Bhattacharjee, A., Fox, W., Valenzuela-Villaseca, V., Molina, J. M., Schaeffer, D. B., Malko, S., Griff-McMahon, J., Lezhnin, K., Rosenberg, M. J., Hu, S. X., Kalantar, D., Trosseille, C., Park, H. -S., Remington, B. A., Fiksel, G., Uzdensky, D., Bhattacharjee, A., and Fox, W.
Abstract: We present results from X-ray imaging of high-aspect-ratio magnetic reconnection experiments driven at the National Ignition Facility. Two parallel, self-magnetized, elongated laser-driven plumes are produced by tiling 40 laser beams. A magnetic reconnection layer is formed by the collision of the plumes. A gated X-ray framing pinhole camera with micro-channel plate (MCP) detector produces multiple images through various filters of the formation and evolution of both the plumes and current sheet. As the diagnostic integrates plasma self-emission along the line of sight, 2-dimensional electron temperature maps $\langle T_e \rangle_Y$ are constructed by taking the ratio of intensity of these images obtained with different filters. The plumes have a characteristic temperature $\langle T_e \rangle_Y = 240 \pm 20$ eV at 2 ns after the initial laser irradiation and exhibit a slow cooling up to 4 ns. The reconnection layer forms at 3 ns with a temperature $\langle T_e \rangle_Y = 280 \pm 50$ eV as the result of the collision of the plumes. The error bars of the plumes and current sheet temperatures separate at $4$ ns, showing the heating of the current sheet from colder inflows. Using a semi-analytical model, we find that the observed heating of the current sheet is consistent with being produced by electron-ion drag, rather than the conversion of magnetic to kinetic energy., Comment: Submitted to Physics of Plasmas. 19 pages (total), 14 figures, 2 tables
Published: 2024

5. Rhinitis associated with asthma is distinct from rhinitis alone:The ARIA-MeDALL hypothesis

Author: Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickman, M, Akdis, M, Aguilar, D, Bedbrook, A, Bindslev-Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia-Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makela, M, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Ansotegui, I J, Arshad, S H, Asayag, E, Barbara, C, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, M, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R S, Bush, A, Calderon, M, Calvo-Gil, M, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia de Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, A F, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Grutta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohammad, Y, Moniuszko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, M S, Robalo Cordeiro, C, Roche, N, Rodriguez-Gonzalez, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Serpa, F S, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, Van Ganse, E, van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, Anto, J M, Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickman, M, Akdis, M, Aguilar, D, Bedbrook, A, Bindslev-Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia-Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makela, M, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Ansotegui, I J, Arshad, S H, Asayag, E, Barbara, C, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, M, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R S, Bush, A, Calderon, M, Calvo-Gil, M, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia de Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, A F, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Grutta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohammad, Y, Moniuszko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, M S, Robalo Cordeiro, C, Roche, N, Rodriguez-Gonzalez, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Serpa, F S, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, Van Ganse, E, van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, and Anto, J M
Abstract: Asthma, rhinitis, and atopic dermatitis (AD) are interrelated clinical phenotypes that partly overlap in the human interactome. The concept of “one-airway-one-disease,” coined over 20 years ago, is a simplistic approach of the links between upper- and lower-airway allergic diseases. With new data, it is time to reassess the concept. This article reviews (i) the clinical observations that led to Allergic Rhinitis and its Impact on Asthma (ARIA), (ii) new insights into polysensitization and multimorbidity, (iii) advances in mHealth for novel phenotype definitions, (iv) confirmation in canonical epidemiologic studies, (v) genomic findings, (vi) treatment approaches, and (vii) novel concepts on the onset of rhinitis and multimorbidity. One recent concept, bringing together upper- and lower-airway allergic diseases with skin, gut, and neuropsychiatric multimorbidities, is the “Epithelial Barrier Hypothesis.” This review determined that the “one-airway-one-disease” concept does not always hold true and that several phenotypes of disease can be defined. These phenotypes include an extreme “allergic” (asthma) phenotype combining asthma, rhinitis, and conjunctivitis. Rhinitis alone and rhinitis and asthma multimorbidity represent two distinct diseases with the following differences: (i) genomic and transcriptomic background (Toll-Like Receptors and IL-17 for rhinitis alone as a local disease; IL-33 and IL-5 for allergic and non-allergic multimorbidity as a systemic disease), (ii) allergen sensitization patterns (mono- or pauci-sensitization versus polysensitization), (iii) severity of symptoms, and (iv) treatment response. In conclusion, rhinitis alone (local disease) and rhinitis with asthma multimorbidity (systemic disease) should be considered as two distinct diseases, possibly modulated by the microbiome, and may be a model for understanding the epidemics of chronic and autoimmune diseases., Asthma, rhinitis, and atopic dermatitis (AD) are interrelated clinical phenotypes that partly overlap in the human interactome. The concept of "one-airway-one-disease," coined over 20 years ago, is a simplistic approach of the links between upper- and lower-airway allergic diseases. With new data, it is time to reassess the concept. This article reviews (i) the clinical observations that led to Allergic Rhinitis and its Impact on Asthma (ARIA), (ii) new insights into polysensitization and multimorbidity, (iii) advances in mHealth for novel phenotype definitions, (iv) confirmation in canonical epidemiologic studies, (v) genomic findings, (vi) treatment approaches, and (vii) novel concepts on the onset of rhinitis and multimorbidity. One recent concept, bringing together upper- and lower-airway allergic diseases with skin, gut, and neuropsychiatric multimorbidities, is the "Epithelial Barrier Hypothesis." This review determined that the "one-airway-one-disease" concept does not always hold true and that several phenotypes of disease can be defined. These phenotypes include an extreme "allergic" (asthma) phenotype combining asthma, rhinitis, and conjunctivitis. Rhinitis alone and rhinitis and asthma multimorbidity represent two distinct diseases with the following differences: (i) genomic and transcriptomic background (Toll-Like Receptors and IL-17 for rhinitis alone as a local disease; IL-33 and IL-5 for allergic and non-allergic multimorbidity as a systemic disease), (ii) allergen sensitization patterns (mono- or pauci-sensitization versus polysensitization), (iii) severity of symptoms, and (iv) treatment response. In conclusion, rhinitis alone (local disease) and rhinitis with asthma multimorbidity (systemic disease) should be considered as two distinct diseases, possibly modulated by the microbiome, and may be a model for understanding the epidemics of chronic and autoimmune diseases.
Published: 2023

6. Search for inelastic WIMP-iodine scattering with COSINE-100

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We report the results of a search for inelastic scattering of weakly interacting massive particles (WIMPs) off $^{127}$I nuclei using NaI(Tl) crystals with a data exposure of 97.7 kg$\cdot$years from the COSINE-100 experiment. The signature of inelastic WIMP-$^{127}$I scattering is a nuclear recoil accompanied by a 57.6 keV $\gamma$-ray from the prompt deexcitation, producing a more energetic signal compared to the typical WIMP nuclear recoil signal. We found no evidence for this inelastic scattering signature and set a 90 $\%$ confidence level upper limit on the WIMP-proton spin-dependent, inelastic scattering cross section of $1.2 \times 10^{-37} {\rm cm^{2}}$ at the WIMP mass 500 ${\rm GeV/c^{2}}$., Comment: 8 pages, 5 figures. arXiv admin note: text overlap with arXiv:2104.03537
Published: 2023
Full Text: View/download PDF

7. Rhinitis associated with asthma is distinct from rhinitis alone: The ARIA-MeDALL hypothesis

Author: Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickmann, M, Aguilar, D, Akdis, M, Ansotegui, I J, Barbara, C, Bedbrook, A, Bindslev Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves-Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Arshad, H S, Asayag, E, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, Michael, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R, Bush, A, Calderon, M, Calvo, G, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia da Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, O, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Gruta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Mäkelä, M J, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohamad, Y, Moniusko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R E, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, R, Roballo-Cordeiro, C, Roche, N, Rodriguez-Gonzales, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Sarquis-Serpa, F, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, van Ganse, E, Van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, Anto, J M, Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickmann, M, Aguilar, D, Akdis, M, Ansotegui, I J, Barbara, C, Bedbrook, A, Bindslev Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves-Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Arshad, H S, Asayag, E, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, Michael, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R, Bush, A, Calderon, M, Calvo, G, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia da Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, O, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Gruta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Mäkelä, M J, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohamad, Y, Moniusko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R E, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, R, Roballo-Cordeiro, C, Roche, N, Rodriguez-Gonzales, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Sarquis-Serpa, F, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, van Ganse, E, Van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, and Anto, J M
Abstract: Asthma, rhinitis and atopic dermatitis (AD) are interrelated clinical phenotypes that partly overlap in the human interactome. The concept of "one-airway-one-disease", coined over 20 years ago, is a simplistic approach of the links between upper- and lower-airway allergic diseases. With new data, it is time to reassess the concept. This article reviews (i) the clinical observations that led to Allergic Rhinitis and its Impact on Asthma (ARIA), (ii) new insights into polysensitisation and multimorbidity, (iii) advances in mHealth for novel phenotype definition, (iv) confirmation in canonical epidemiologic studies, (v) genomic findings, (vi) treatment approaches and (vii) novel concepts on the onset of rhinitis and multimorbidity. One recent concept, bringing together upper- and lower-airway allergic diseases with skin, gut and neuropsychiatric multimorbidities, is the "Epithelial Barrier Hypothesis". This review determined that the "one-airway-one-disease" concept does not always hold true and that several phenotypes of disease can be defined. These phenotypes include an extreme "allergic" (asthma) phenotype combining asthma, rhinitis and conjunctivitis. Rhinitis alone and rhinitis and asthma multimorbidity represent two distinct diseases with the following differences: (i) genomic and transcriptomic background (Toll-Like Receptors and IL-17 for rhinitis alone as a local disease; IL-33 and IL-5 for allergic and non-allergic multimorbidity as a systemic disease), (ii) allergen sensitisation patterns (mono- or pauci-sensitisation versus polysensitisation), (iii) severity of symptoms and (iv) treatment response. In conclusion, rhinitis alone (local disease) and rhinitis with asthma multimorbidity (systemic disease) should be considered as two distinct diseases, possibly modulated by the microbiome, and may be a model for understanding the epidemics of chronic and auto-immune diseases. [Abstract copyright: This article is protected by copyright. All rights reserved.]
Published: 2023

8. Search for Boosted Dark Matter in COSINE-100

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We search for energetic electron recoil signals induced by boosted dark matter (BDM) from the galactic center using the COSINE-100 array of NaI(Tl) crystal detectors at the Yangyang Underground Laboratory. The signal would be an excess of events with energies above 4 MeV over the well-understood background. Because no excess of events are observed in a 97.7 kg$\cdot$years exposure, we set limits on BDM interactions under a variety of hypotheses. Notably, we explored the dark photon parameter space, leading to competitive limits compared to direct dark photon search experiments, particularly for dark photon masses below 4\,MeV and considering the invisible decay mode. Furthermore, by comparing our results with a previous BDM search conducted by the Super-Kamionkande experiment, we found that the COSINE-100 detector has advantages in searching for low-mass dark matter. This analysis demonstrates the potential of the COSINE-100 detector to search for MeV electron recoil signals produced by the dark sector particle interactions., Comment: 7 pages, 4 figures
Published: 2023
Full Text: View/download PDF

9. Search for solar bosonic dark matter annual modulation with COSINE-100

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We present results from a search for solar bosonic dark matter using the annual modulation method with the COSINE-100 experiment. The results were interpreted considering three dark sector bosons models: solar dark photon; DFSZ and KSVZ solar axion; and Kaluza-Klein solar axion. No modulation signal that is compatible with the expected from the models was found from a data-set of 2.82 yr, using 61.3 kg of NaI(Tl) crystals. Therefore, we set a 90$\%$ confidence level upper limits for each of the three models studied. For the solar dark photon model, the most stringent mixing parameter upper limit is $1.61 \times 10^{-14}$ for dark photons with a mass of 215 eV. For the DFSZ and KSVZ solar axion, and the Kaluza-Klein axion models, the upper limits exclude axion-electron couplings, $g_{ae}$, above $1.61 \times 10^{-11}$ for axion mass below 0.2 keV; and axion-photon couplings, $g_{a\gamma\gamma}$, above $1.83 \times 10^{-11}$ GeV$^{-1}$ for an axion number density of $4.07 \times 10^{13}$ cm$^{-3}$. This is the first experimental search for solar dark photons and DFSZ and KSVZ solar axions using the annual modulation method. The lower background, higher light yield and reduced threshold of NaI(Tl) crystals of the future COSINE-200 experiment are expected to enhance the sensitivity of the analysis shown in this paper. We show the sensitivities for the three models studied, considering the same search method with COSINE-200., Comment: 13 pages, 16 figures
Published: 2023
Full Text: View/download PDF

10. Search for bosonic super-weakly interacting massive particles at COSINE-100

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Cavalcante, D. F. F. S., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We present results of a search for bosonic super-weakly interacting massive particles (BSW) as keV scale dark matter candidates that is based on an exposure of 97.7 kg$\cdot$year from the COSINE experiment. In this search, we employ, for the first time, Compton-like as well as absorption processes for pseudoscalar and vector BSWs. No evidence for BSWs is found in the mass range from 10 $\mathrm{keV/c}^2$ to 1 $\mathrm{MeV/c}^2$, and we present the exclusion limits on the dimensionless coupling constants to electrons $g_{ae}$ for pseudoscalar and $\kappa$ for vector BSWs at 90% confidence level. Our results show that these limits are improved by including the Compton-like process in masses of BSW, above $\mathcal{O}(100\,\mathrm{keV/c}^2)$.
Published: 2023
Full Text: View/download PDF

11. Rhinitis associated with asthma is distinct from rhinitis alone: The ARIA-MeDALL hypothesis

Author: Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickmann, M, Aguilar, D, Akdis, M, Ansotegui, I J, Barbara, C, Bedbrook, A, Bindslev Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves-Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Arshad, H S, Asayag, E, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, Michael, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R, Bush, A, Calderon, M, Calvo, G, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia da Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, O, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Gruta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Mäkelä, M J, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohamad, Y, Moniusko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R E, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, R, Roballo-Cordeiro, C, Roche, N, Rodriguez-Gonzales, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Sarquis-Serpa, F, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, van Ganse, E, Van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, Anto, J M, Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickmann, M, Aguilar, D, Akdis, M, Ansotegui, I J, Barbara, C, Bedbrook, A, Bindslev Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves-Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Arshad, H S, Asayag, E, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, Michael, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R, Bush, A, Calderon, M, Calvo, G, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia da Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, O, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Gruta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Mäkelä, M J, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohamad, Y, Moniusko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R E, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, R, Roballo-Cordeiro, C, Roche, N, Rodriguez-Gonzales, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Sarquis-Serpa, F, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, van Ganse, E, Van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, and Anto, J M
Abstract: Asthma, rhinitis and atopic dermatitis (AD) are interrelated clinical phenotypes that partly overlap in the human interactome. The concept of "one-airway-one-disease", coined over 20 years ago, is a simplistic approach of the links between upper- and lower-airway allergic diseases. With new data, it is time to reassess the concept. This article reviews (i) the clinical observations that led to Allergic Rhinitis and its Impact on Asthma (ARIA), (ii) new insights into polysensitisation and multimorbidity, (iii) advances in mHealth for novel phenotype definition, (iv) confirmation in canonical epidemiologic studies, (v) genomic findings, (vi) treatment approaches and (vii) novel concepts on the onset of rhinitis and multimorbidity. One recent concept, bringing together upper- and lower-airway allergic diseases with skin, gut and neuropsychiatric multimorbidities, is the "Epithelial Barrier Hypothesis". This review determined that the "one-airway-one-disease" concept does not always hold true and that several phenotypes of disease can be defined. These phenotypes include an extreme "allergic" (asthma) phenotype combining asthma, rhinitis and conjunctivitis. Rhinitis alone and rhinitis and asthma multimorbidity represent two distinct diseases with the following differences: (i) genomic and transcriptomic background (Toll-Like Receptors and IL-17 for rhinitis alone as a local disease; IL-33 and IL-5 for allergic and non-allergic multimorbidity as a systemic disease), (ii) allergen sensitisation patterns (mono- or pauci-sensitisation versus polysensitisation), (iii) severity of symptoms and (iv) treatment response. In conclusion, rhinitis alone (local disease) and rhinitis with asthma multimorbidity (systemic disease) should be considered as two distinct diseases, possibly modulated by the microbiome, and may be a model for understanding the epidemics of chronic and auto-immune diseases. [Abstract copyright: This article is protected by copyright. All rights reserved.]
Published: 2023

12. Rhinitis associated with asthma is distinct from rhinitis alone: The ARIA-MeDALL hypothesis

Author: Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickmann, M, Aguilar, D, Akdis, M, Ansotegui, I J, Barbara, C, Bedbrook, A, Bindslev Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves-Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Arshad, H S, Asayag, E, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, Michael, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R, Bush, A, Calderon, M, Calvo, G, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia da Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, O, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Gruta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Mäkelä, M J, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohamad, Y, Moniusko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R E, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, R, Roballo-Cordeiro, C, Roche, N, Rodriguez-Gonzales, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Sarquis-Serpa, F, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, van Ganse, E, Van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, Anto, J M, Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickmann, M, Aguilar, D, Akdis, M, Ansotegui, I J, Barbara, C, Bedbrook, A, Bindslev Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves-Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Arshad, H S, Asayag, E, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, Michael, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R, Bush, A, Calderon, M, Calvo, G, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia da Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, O, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Gruta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Mäkelä, M J, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohamad, Y, Moniusko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R E, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, R, Roballo-Cordeiro, C, Roche, N, Rodriguez-Gonzales, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Sarquis-Serpa, F, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, van Ganse, E, Van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, and Anto, J M
Abstract: Asthma, rhinitis and atopic dermatitis (AD) are interrelated clinical phenotypes that partly overlap in the human interactome. The concept of "one-airway-one-disease", coined over 20 years ago, is a simplistic approach of the links between upper- and lower-airway allergic diseases. With new data, it is time to reassess the concept. This article reviews (i) the clinical observations that led to Allergic Rhinitis and its Impact on Asthma (ARIA), (ii) new insights into polysensitisation and multimorbidity, (iii) advances in mHealth for novel phenotype definition, (iv) confirmation in canonical epidemiologic studies, (v) genomic findings, (vi) treatment approaches and (vii) novel concepts on the onset of rhinitis and multimorbidity. One recent concept, bringing together upper- and lower-airway allergic diseases with skin, gut and neuropsychiatric multimorbidities, is the "Epithelial Barrier Hypothesis". This review determined that the "one-airway-one-disease" concept does not always hold true and that several phenotypes of disease can be defined. These phenotypes include an extreme "allergic" (asthma) phenotype combining asthma, rhinitis and conjunctivitis. Rhinitis alone and rhinitis and asthma multimorbidity represent two distinct diseases with the following differences: (i) genomic and transcriptomic background (Toll-Like Receptors and IL-17 for rhinitis alone as a local disease; IL-33 and IL-5 for allergic and non-allergic multimorbidity as a systemic disease), (ii) allergen sensitisation patterns (mono- or pauci-sensitisation versus polysensitisation), (iii) severity of symptoms and (iv) treatment response. In conclusion, rhinitis alone (local disease) and rhinitis with asthma multimorbidity (systemic disease) should be considered as two distinct diseases, possibly modulated by the microbiome, and may be a model for understanding the epidemics of chronic and auto-immune diseases. [Abstract copyright: This article is protected by copyright. All rights reserved.]
Published: 2023

13. Alpha backgrounds in NaI(Tl) crystals of COSINE-100

Author: Adhikari, G., Carlin, N., Cavalcante, D. F. F. S., Cho, J. Y., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, S. W., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, J. C., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Scar, A., Shin, K. A., Son, M. K., Spooner, N. J. C., Truc, L. T., Yang, L., Yu, G. H., COSINE-100, for, Adhikari, G., Carlin, N., Cavalcante, D. F. F. S., Cho, J. Y., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, S. W., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Luan, N. T., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, J. C., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Scar, A., Shin, K. A., Son, M. K., Spooner, N. J. C., Truc, L. T., Yang, L., Yu, G. H., and COSINE-100, for
Abstract: COSINE-100 is a dark matter direct detection experiment with 106 kg NaI(Tl) as the target material. 210Pb and daughter isotopes are a dominant background in the WIMP region of interest and are detected via beta decay and alpha decay. Analysis of the alpha channel complements the background model as observed in the beta/gamma channel. We present the measurement of the quenching factors and Monte Carlo simulation results and activity quantification of the alpha decay components of the COSINE-100 NaI(Tl) crystals. The data strongly indicate that the alpha decays probabilistically undergo two possible quenching factors but require further investigation. The fitted results are consistent with independent measurements and improve the overall understanding of the COSINE-100 backgrounds. Furthermore, the half-life of 216Po has been measured to be 143.4 +/- 1.2 ms, which is consistent with and more precise than recent measurements.
Published: 2023
Full Text: View/download PDF

14. Rhinitis associated with asthma is distinct from rhinitis alone:The ARIA-MeDALL hypothesis

Author: Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickman, M, Akdis, M, Aguilar, D, Bedbrook, A, Bindslev-Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia-Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makela, M, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Ansotegui, I J, Arshad, S H, Asayag, E, Barbara, C, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, M, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R S, Bush, A, Calderon, M, Calvo-Gil, M, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia de Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, A F, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Grutta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohammad, Y, Moniuszko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, M S, Robalo Cordeiro, C, Roche, N, Rodriguez-Gonzalez, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Serpa, F S, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, Van Ganse, E, van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, Anto, J M, Bousquet, J, Melén, E, Haahtela, T, Koppelman, G H, Togias, A, Valenta, R, Akdis, C A, Czarlewski, W, Rothenberg, M, Valiulis, A, Wickman, M, Akdis, M, Aguilar, D, Bedbrook, A, Bindslev-Jensen, C, Bosnic-Anticevich, S, Boulet, L P, Brightling, C E, Brussino, L, Burte, E, Bustamante, M, Canonica, G W, Cecchi, L, Celedon, J C, Chaves Loureiro, C, Costa, E, Cruz, A A, Erhola, M, Gemicioglu, B, Fokkens, W J, Garcia-Aymerich, J, Guerra, S, Heinrich, J, Ivancevich, J C, Keil, T, Klimek, L, Kuna, P, Kupczyk, M, Kvedariene, V, Larenas-Linnemann, D E, Lemonnier, N, Lodrup Carlsen, K C, Louis, R, Makela, M, Makris, M, Maurer, M, Momas, I, Morais-Almeida, M, Mullol, J, Naclerio, R N, Nadeau, K, Nadif, R, Niedoszytko, M, Okamoto, Y, Ollert, M, Papadopoulos, N G, Passalacqua, G, Patella, V, Pawankar, R, Pham-Thi, N, Pfaar, O, Regateiro, F S, Ring, J, Rouadi, P W, Samolinski, B, Sastre, J, Savouré, M, Scichilone, N, Shamji, M H, Sheikh, A, Siroux, V, Sousa-Pinto, B, Standl, M, Sunyer, J, Taborda-Barata, L, Toppila-Salmi, S, Torres, M J, Tsiligianni, I, Valovirta, E, Vandenplas, O, Ventura, M T, Weiss, S, Yorgancioglu, A, Zhang, L, Abdul Latiff, A H, Aberer, W, Agache, I, Al-Ahmad, M, Alobid, I, Ansotegui, I J, Arshad, S H, Asayag, E, Barbara, C, Baharudin, A, Battur, L, Bennoor, K S, Berghea, E C, Bergmann, K C, Bernstein, D, Bewick, M, Blain, H, Bonini, M, Braido, F, Buhl, R, Bumbacea, R S, Bush, A, Calderon, M, Calvo-Gil, M, Camargos, P, Caraballo, L, Cardona, V, Carr, W, Carreiro-Martins, P, Casale, T, Cepeda Sarabia, A M, Chandrasekharan, R, Charpin, D, Chen, Y Z, Cherrez-Ojeda, I, Chivato, T, Chkhartishvili, E, Christoff, G, Chu, D K, Cingi, C, Correia de Sousa, J, Corrigan, C, Custovic, A, D'Amato, G, Del Giacco, S, De Blay, F, Devillier, P, Didier, A, do Ceu Teixeira, M, Dokic, D, Douagui, H, Doulaptsi, M, Durham, S, Dykewicz, M, Eiwegger, T, El-Sayed, Z A, Emuzyte, R, Fiocchi, A, Fyhrquist, N, Gomez, R M, Gotua, M, Guzman, M A, Hagemann, J, Hamamah, S, Halken, S, Halpin, D M G, Hofmann, M, Hossny, E, Hrubiško, M, Irani, C, Ispayeva, Z, Jares, E, Jartti, T, Jassem, E, Julge, K, Just, J, Jutel, M, Kaidashev, I, Kalayci, O, Kalyoncu, A F, Kardas, P, Kirenga, B, Kraxner, H, Kull, I, Kulus, M, La Grutta, S, Lau, S, Le Tuyet Thi, L, Levin, M, Lipworth, B, Lourenço, O, Mahboub, B, Martinez-Infante, E, Matricardi, P, Miculinic, N, Migueres, N, Mihaltan, F, Mohammad, Y, Moniuszko, M, Montefort, S, Neffen, H, Nekam, K, Nunes, E, Nyembue Tshipukane, D, O'Hehir, R, Ogulur, I, Ohta, K, Okubo, K, Ouedraogo, S, Olze, H, Pali-Schöll, I, Palomares, O, Palosuo, K, Panaitescu, C, Panzner, P, Park, H S, Pitsios, C, Plavec, D, Popov, T A, Puggioni, F, Quirce, S, Recto, M, Repka-Ramirez, M S, Robalo Cordeiro, C, Roche, N, Rodriguez-Gonzalez, M, Romantowski, J, Rosario Filho, N, Rottem, M, Sagara, H, Serpa, F S, Sayah, Z, Scheire, S, Schmid-Grendelmeier, P, Sisul, J C, Sole, D, Soto-Martinez, M, Sova, M, Sperl, A, Spranger, O, Stelmach, R, Suppli Ulrik, C, Thomas, M, To, T, Todo-Bom, A, Tomazic, P V, Urrutia-Pereira, M, Valentin-Rostan, M, Van Ganse, E, van Hage, M, Vasankari, T, Vichyanond, P, Viegi, G, Wallace, D, Wang, D Y, Williams, S, Worm, M, Yiallouros, P, Yusuf, O, Zaitoun, F, Zernotti, M, Zidarn, M, Zuberbier, J, Fonseca, J A, Zuberbier, T, and Anto, J M
Abstract: Asthma, rhinitis, and atopic dermatitis (AD) are interrelated clinical phenotypes that partly overlap in the human interactome. The concept of “one-airway-one-disease,” coined over 20 years ago, is a simplistic approach of the links between upper- and lower-airway allergic diseases. With new data, it is time to reassess the concept. This article reviews (i) the clinical observations that led to Allergic Rhinitis and its Impact on Asthma (ARIA), (ii) new insights into polysensitization and multimorbidity, (iii) advances in mHealth for novel phenotype definitions, (iv) confirmation in canonical epidemiologic studies, (v) genomic findings, (vi) treatment approaches, and (vii) novel concepts on the onset of rhinitis and multimorbidity. One recent concept, bringing together upper- and lower-airway allergic diseases with skin, gut, and neuropsychiatric multimorbidities, is the “Epithelial Barrier Hypothesis.” This review determined that the “one-airway-one-disease” concept does not always hold true and that several phenotypes of disease can be defined. These phenotypes include an extreme “allergic” (asthma) phenotype combining asthma, rhinitis, and conjunctivitis. Rhinitis alone and rhinitis and asthma multimorbidity represent two distinct diseases with the following differences: (i) genomic and transcriptomic background (Toll-Like Receptors and IL-17 for rhinitis alone as a local disease; IL-33 and IL-5 for allergic and non-allergic multimorbidity as a systemic disease), (ii) allergen sensitization patterns (mono- or pauci-sensitization versus polysensitization), (iii) severity of symptoms, and (iv) treatment response. In conclusion, rhinitis alone (local disease) and rhinitis with asthma multimorbidity (systemic disease) should be considered as two distinct diseases, possibly modulated by the microbiome, and may be a model for understanding the epidemics of chronic and autoimmune diseases., Asthma, rhinitis, and atopic dermatitis (AD) are interrelated clinical phenotypes that partly overlap in the human interactome. The concept of "one-airway-one-disease," coined over 20 years ago, is a simplistic approach of the links between upper- and lower-airway allergic diseases. With new data, it is time to reassess the concept. This article reviews (i) the clinical observations that led to Allergic Rhinitis and its Impact on Asthma (ARIA), (ii) new insights into polysensitization and multimorbidity, (iii) advances in mHealth for novel phenotype definitions, (iv) confirmation in canonical epidemiologic studies, (v) genomic findings, (vi) treatment approaches, and (vii) novel concepts on the onset of rhinitis and multimorbidity. One recent concept, bringing together upper- and lower-airway allergic diseases with skin, gut, and neuropsychiatric multimorbidities, is the "Epithelial Barrier Hypothesis." This review determined that the "one-airway-one-disease" concept does not always hold true and that several phenotypes of disease can be defined. These phenotypes include an extreme "allergic" (asthma) phenotype combining asthma, rhinitis, and conjunctivitis. Rhinitis alone and rhinitis and asthma multimorbidity represent two distinct diseases with the following differences: (i) genomic and transcriptomic background (Toll-Like Receptors and IL-17 for rhinitis alone as a local disease; IL-33 and IL-5 for allergic and non-allergic multimorbidity as a systemic disease), (ii) allergen sensitization patterns (mono- or pauci-sensitization versus polysensitization), (iii) severity of symptoms, and (iv) treatment response. In conclusion, rhinitis alone (local disease) and rhinitis with asthma multimorbidity (systemic disease) should be considered as two distinct diseases, possibly modulated by the microbiome, and may be a model for understanding the epidemics of chronic and autoimmune diseases.
Published: 2023

15. Insensitivity of a turbulent laser-plasma dynamo to initial conditions

Author: Bott, A. F. A., Chen, L., Tzeferacos, P., Palmer, C. A. J., Bell, A. R., Bingham, R., Birkel, A., Froula, D. H., Katz, J., Kunz, M. W., Li, C. -K., Park, H-S., Petrasso, R., Ross, J. S., Reville, B., Ryu, D., Séguin, F. H., White, T. G., Schekochihin, A. A., Lamb, D. Q., Gregori, G., Bott, A. F. A., Chen, L., Tzeferacos, P., Palmer, C. A. J., Bell, A. R., Bingham, R., Birkel, A., Froula, D. H., Katz, J., Kunz, M. W., Li, C. -K., Park, H-S., Petrasso, R., Ross, J. S., Reville, B., Ryu, D., Séguin, F. H., White, T. G., Schekochihin, A. A., Lamb, D. Q., and Gregori, G.
Abstract: It has recently been demonstrated experimentally that a turbulent plasma created by the collision of two inhomogeneous, asymmetric, weakly magnetised laser-produced plasma jets can generate strong stochastic magnetic fields via the small-scale turbulent dynamo mechanism, provided the magnetic Reynolds number of the plasma is sufficiently large. In this paper, we compare such a plasma with one arising from two pre-magnetised plasma jets whose creation is identical save for the addition of a strong external magnetic field imposed by a pulsed magnetic field generator (`MIFEDS'). We investigate the differences between the two turbulent systems using a Thomson-scattering diagnostic, X-ray self-emission imaging and proton radiography. The Thomson-scattering spectra and X-ray images suggest that the presence of the external magnetic field has a limited effect on the plasma dynamics in the experiment. While the presence of the external magnetic field induces collimation of the flows in the colliding plasma jets and the initial strengths of the magnetic fields arising from the interaction between the colliding jets are significantly larger as a result of the external field, the energy and morphology of the stochastic magnetic fields post-amplification are indistinguishable. We conclude that, for turbulent laser-plasmas with super-critical magnetic Reynolds numbers, the dynamo-amplified magnetic fields are determined by the turbulent dynamics rather than the seed fields and modest changes in the initial flow dynamics of the plasma, a finding consistent with theoretical expectations and simulations of turbulent dynamos., Comment: 13 pages, 12 figures
Published: 2022

16. A lab scale experiment for keV sterile neutrino search

Author: Lee, Y. C., Kim, H. B., Kim, H. L., Kim, S. K., Kim, Y. H., Kwon, D. H., Lim, H. S., Park, H. S., Woo, K. R., Yoon, Y. S., Lee, Y. C., Kim, H. B., Kim, H. L., Kim, S. K., Kim, Y. H., Kwon, D. H., Lim, H. S., Park, H. S., Woo, K. R., and Yoon, Y. S.
Abstract: We developed a simple small-scale experiment to measure the beta decay spectrum of $^{3}$H. The aim of this research is to investigate the presence of sterile neutrinos in the keV region. Tritium nuclei were embedded in a 1$\times$1$\times$1 cm$^3$ LiF crystal from the $^6$Li(n,$\alpha$)$^3$H reaction. The energy of the beta electrons absorbed in the LiF crystal was measured with a magnetic microcalorimeter at 40 mK. We report a new method of sample preparation, experiments, and analysis of $^3$H beta measurements. The spectrum of a 10-hour measurement agrees well with the expected spectrum of $^3$H beta decay. The analysis results indicate that this method can be used to search for keV-scale sterile neutrinos.
Published: 2022
Full Text: View/download PDF

17. An induced annual modulation signature in COSINE-100 data by DAMA/LIBRA's analysis method

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: The DAMA/LIBRA collaboration has reported the observation of an annual modulation in the event rate that has been attributed to dark matter interactions over the last two decades. However, even though tremendous efforts to detect similar dark matter interactions were pursued, no definitive evidence has been observed to corroborate the DAMA/LIBRA signal. Many studies assuming various dark matter models have attempted to reconcile DAMA/LIBRA's modulation signals and null results from other experiments, however no clear conclusion can be drawn. Apart from the dark matter hypothesis, several studies have examined the possibility that the modulation is induced by variations in their detector's environment or their specific analysis methods. In particular, a recent study presents a possible cause of the annual modulation from an analysis method adopted by the DAMA/LIBRA experiment in which the observed annual modulation could be reproduced by a slowly varying time-dependent background. Here, we study the COSINE-100 data using an analysis method similar to the one adopted by the DAMA/LIBRA experiment and observe a significant annual modulation, although the modulation phase is almost opposite to that of the DAMA/LIBRA data. Assuming the same background composition for COSINE-100 and DAMA/LIBRA, simulated experiments for the DAMA/LIBRA without dark matter signals also provide significant annual modulation with an amplitude similar to DAMA/LIBRA with opposite phase. Even though this observation does not explain the DAMA/LIBRA's results directly, this interesting phenomenon motivates deeper studies of the time-dependent DAMA/LIBRA background data.
Published: 2022
Full Text: View/download PDF

18. An induced annual modulation signature in COSINE-100 data by DAMA/LIBRA's analysis method

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, B. H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Lee, Y. J., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Nikkel, J. A., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: The DAMA/LIBRA collaboration has reported the observation of an annual modulation in the event rate that has been attributed to dark matter interactions over the last two decades. However, even though tremendous efforts to detect similar dark matter interactions were pursued, no definitive evidence has been observed to corroborate the DAMA/LIBRA signal. Many studies assuming various dark matter models have attempted to reconcile DAMA/LIBRA's modulation signals and null results from other experiments, however no clear conclusion can be drawn. Apart from the dark matter hypothesis, several studies have examined the possibility that the modulation is induced by variations in their detector's environment or their specific analysis methods. In particular, a recent study presents a possible cause of the annual modulation from an analysis method adopted by the DAMA/LIBRA experiment in which the observed annual modulation could be reproduced by a slowly varying time-dependent background. Here, we study the COSINE-100 data using an analysis method similar to the one adopted by the DAMA/LIBRA experiment and observe a significant annual modulation, although the modulation phase is almost opposite to that of the DAMA/LIBRA data. Assuming the same background composition for COSINE-100 and DAMA/LIBRA, simulated experiments for the DAMA/LIBRA without dark matter signals also provide significant annual modulation with an amplitude similar to DAMA/LIBRA with opposite phase. Even though this observation does not explain the DAMA/LIBRA's results directly, this interesting phenomenon motivates deeper studies of the time-dependent DAMA/LIBRA background data.
Published: 2022
Full Text: View/download PDF

19. Insensitivity of a turbulent laser-plasma dynamo to initial conditions

Author: Bott, A. F. A., Chen, L., Tzeferacos, P., Palmer, C. A. J., Bell, A. R., Bingham, R., Birkel, A., Froula, D. H., Katz, J., Kunz, M. W., Li, C. -K., Park, H-S., Petrasso, R., Ross, J. S., Reville, B., Ryu, D., Séguin, F. H., White, T. G., Schekochihin, A. A., Lamb, D. Q., Gregori, G., Bott, A. F. A., Chen, L., Tzeferacos, P., Palmer, C. A. J., Bell, A. R., Bingham, R., Birkel, A., Froula, D. H., Katz, J., Kunz, M. W., Li, C. -K., Park, H-S., Petrasso, R., Ross, J. S., Reville, B., Ryu, D., Séguin, F. H., White, T. G., Schekochihin, A. A., Lamb, D. Q., and Gregori, G.
Abstract: It has recently been demonstrated experimentally that a turbulent plasma created by the collision of two inhomogeneous, asymmetric, weakly magnetised laser-produced plasma jets can generate strong stochastic magnetic fields via the small-scale turbulent dynamo mechanism, provided the magnetic Reynolds number of the plasma is sufficiently large. In this paper, we compare such a plasma with one arising from two pre-magnetised plasma jets whose creation is identical save for the addition of a strong external magnetic field imposed by a pulsed magnetic field generator (`MIFEDS'). We investigate the differences between the two turbulent systems using a Thomson-scattering diagnostic, X-ray self-emission imaging and proton radiography. The Thomson-scattering spectra and X-ray images suggest that the presence of the external magnetic field has a limited effect on the plasma dynamics in the experiment. While the presence of the external magnetic field induces collimation of the flows in the colliding plasma jets and the initial strengths of the magnetic fields arising from the interaction between the colliding jets are significantly larger as a result of the external field, the energy and morphology of the stochastic magnetic fields post-amplification are indistinguishable. We conclude that, for turbulent laser-plasmas with super-critical magnetic Reynolds numbers, the dynamo-amplified magnetic fields are determined by the turbulent dynamics rather than the seed fields and modest changes in the initial flow dynamics of the plasma, a finding consistent with theoretical expectations and simulations of turbulent dynamos., Comment: 13 pages, 12 figures
Published: 2022

20. Three-year annual modulation search with COSINE-100

Author: Collaboration, COSINE-100, Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Collaboration, COSINE-100, Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: COSINE-100 is a direct detection dark matter experiment that aims to test DAMA/LIBRA's claim of dark matter discovery by searching for a dark matter-induced annual modulation signal with NaI(Tl) detectors. We present new constraints on the annual modulation signal from a dataset with a 2.82 yr livetime utilizing an active mass of 61.3 kg, for a total exposure of 173 kg$\cdot$yr. This new result features an improved event selection that allows for both lowering the energy threshold to 1 keV and a more precise time-dependent background model. In the 1-6 keV and 2-6 keV energy intervals, we observe best-fit values for the modulation amplitude of 0.0067$\pm$0.0042 and 0.0050$\pm$0.0047 counts/(day$\cdot$kg$\cdot$keV), respectively, with a phase fixed at 152.5 days., Comment: 9 pages, 8 figures
Published: 2021

21. Searching for low-mass dark matter via Migdal effect in COSINE-100

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We report on the search for weakly interacting massive particle (WIMP) dark matter candidates in the galactic halo that interact with sodium and iodine nuclei in the COSINE-100 experiment and produce energetic electrons that accompany recoil nuclei via the the Migdal effect. The WIMP mass sensitivity of previous COSINE-100 searches that relied on the detection of ionization signals produced by target nuclei recoiling from elastic WIMP-nucleus scattering was restricted to WIMP masses above $\sim$5 GeV/$c^2$ by the detectors' 1 keVee energy-electron-equivalent threshold. The search reported here looks for recoil signals enhanced by the Migdal electrons that are ejected during the scattering process. This is particularly effective for the detection of low-mass WIMP scattering from the crystals' sodium nuclei in which a relatively larger fraction of the WIMP's energy is transferred to the nucleus recoil energy and the excitation of its orbital electrons. In this analysis, the low-mass WIMP search window of the COSINE-100 experiment is extended to WIMP mass down to 200 MeV/$c^2$. The low-mass WIMP sensitivity will be further improved by lowering the analysis threshold based on a multivariable analysis technique. We consider the influence of these improvements and recent developments in detector performance to re-evaluate sensitivities for the future COSINE-200 experiment. With a 0.2 keVee analysis threshold and high light-yield NaI(Tl) detectors (22 photoelectrons/keVee), the COSINE-200 experiment can explore low-mass WIMPs down to 20 MeV/$c^2$ and probe previously unexplored regions of parameter space., Comment: 10 pages, 8 figures
Published: 2021
Full Text: View/download PDF

22. Alpha backgrounds in the AMoRE-Pilot experiment

Author: Alenkov, V., Beyer, J., Boiko, R. S., Boonin, K., Buzanov, O., Chanthima, N., Cheoun, M. K., Choi, S. H., Danevich, F. A., Djamal, M., Drung, D., Enss, C., Fleischmann, A., Gangapshev, A., Gastaldo, L., Gavriljuk, Yu. M., Gezhaev, A., Grigoryeva, V. D., Gurentsov, V., Ha, D. H., Ha, C., Ha, E. J., Hahn, I., Jeon, E. J., Jeon, J., Jo, H. S., Kaewkhao, J., Kang, C. S., Kang, S. J., Kang, W. G., Karki, S., Kazalov, V., Khan, A., Khan, S., Kim, D. -Y., Kim, G. W., Kim, H. B., Kim, H. J., Kim, H. L., Kim, H. S., Kim, I., Kim, W. T., Kim, S., Kim, S. C., Kim, S. K., Kim, Y. D., Kim, Y. H., Kirdsiri, K., Ko, Y. J., Kobychev, V. V., Kornoukhov, V., Kuzminov, V., Kwon, D. H., Lee, C., Lee, E. K., Lee, H. J., Lee, H. S., Lee, J., Lee, J. S., Lee, J. Y., Lee, K. B., Lee, M. H., Lee, M. K., Lee, S. H., Lee, S. W., Leonard, D. S., Li, J., Li, Y., Limkitjaroenporn, P., Mailyan, B., Makarov, E. P., Oh, S. Y., Oh, Y. M., Gileva, O., Olsen, S., Pabitra, A., Panasenko, S., Pandey, I., Park, C. W., Park, H. K., Park, H. S., Park, K. S., Park, S. Y., Polischuk, O. G., Prihtiadi, H., Ra, S. J., Ratkevich, S., Rooh, G., Sari, M. B., Seo, J., Seo, K. M., Shin, J. W., Shin, K. A., Shlegel, V. N., Siyeon, K., Sokur, N. V., Son, J. -K., Srisittipokakun, N., Toibaev, N., Tretyak, V. I., Wirawan, R., Woo, K. R., Yoon, Y. S., Yue, Q., Alenkov, V., Beyer, J., Boiko, R. S., Boonin, K., Buzanov, O., Chanthima, N., Cheoun, M. K., Choi, S. H., Danevich, F. A., Djamal, M., Drung, D., Enss, C., Fleischmann, A., Gangapshev, A., Gastaldo, L., Gavriljuk, Yu. M., Gezhaev, A., Grigoryeva, V. D., Gurentsov, V., Ha, D. H., Ha, C., Ha, E. J., Hahn, I., Jeon, E. J., Jeon, J., Jo, H. S., Kaewkhao, J., Kang, C. S., Kang, S. J., Kang, W. G., Karki, S., Kazalov, V., Khan, A., Khan, S., Kim, D. -Y., Kim, G. W., Kim, H. B., Kim, H. J., Kim, H. L., Kim, H. S., Kim, I., Kim, W. T., Kim, S., Kim, S. C., Kim, S. K., Kim, Y. D., Kim, Y. H., Kirdsiri, K., Ko, Y. J., Kobychev, V. V., Kornoukhov, V., Kuzminov, V., Kwon, D. H., Lee, C., Lee, E. K., Lee, H. J., Lee, H. S., Lee, J., Lee, J. S., Lee, J. Y., Lee, K. B., Lee, M. H., Lee, M. K., Lee, S. H., Lee, S. W., Leonard, D. S., Li, J., Li, Y., Limkitjaroenporn, P., Mailyan, B., Makarov, E. P., Oh, S. Y., Oh, Y. M., Gileva, O., Olsen, S., Pabitra, A., Panasenko, S., Pandey, I., Park, C. W., Park, H. K., Park, H. S., Park, K. S., Park, S. Y., Polischuk, O. G., Prihtiadi, H., Ra, S. J., Ratkevich, S., Rooh, G., Sari, M. B., Seo, J., Seo, K. M., Shin, J. W., Shin, K. A., Shlegel, V. N., Siyeon, K., Sokur, N. V., Son, J. -K., Srisittipokakun, N., Toibaev, N., Tretyak, V. I., Wirawan, R., Woo, K. R., Yoon, Y. S., and Yue, Q.
Abstract: Searches for neutrinoless double beta decay generally require ultimate low backgrounds. Surface $\alpha$ decays on the crystals themselves or nearby materials can deposit a continuum of energies that can be as high as the $Q$-value of the decay and may cover in the region of interest (ROI). The AMoRE-Pilot experiment is an initial phase of the AMoRE search for neutrinoless double beta decay of $^{100}$Mo, with the purpose of investigating the level and sources of backgrounds. To understand those background events, we have studied backgrounds from radioactive contaminations internal to and on the surface of the crystals or nearby materials with Geant4-based Monte Carlo simulations. In this paper, we report the measured $\alpha$ energy spectra fitted with the simulated $\alpha$ energy spectra for the six crystal detectors, where sources of background contributions can be identified at high energy by $\alpha$ peaks for both surface and internal contaminations. We determine the low-energy contributions from internal and surface $\alpha$ contaminations by extrapolating from the $\alpha$ background fitting model.
Published: 2021

23. Strong suppression of heat conduction in a laboratory replica of galaxy-cluster turbulent plasmas

Author: Meinecke, J., Tzeferacos, P., Ross, J. S., Bott, A. F. A., Feister, S., Park, H. -S., Bell, A. R., Blandford, R., Berger, R. L., Bingham, R., Casner, A., Chen, L. E., Foster, J., Froula, D. H., Goyon, C., Kalantar, D., Koenig, M., Lahmann, B., Li, C. -K., Lu, Y., Palmer, C. A. J., Petrasso, R., Poole, H., Remington, B., Reville, B., Reyes, A., Rigby, A., Ryu, D., Swadling, G., Zylstra, A., Miniati, F., Sarkar, S., Schekochihin, A. A., Lamb, D. Q., Gregori, G., Meinecke, J., Tzeferacos, P., Ross, J. S., Bott, A. F. A., Feister, S., Park, H. -S., Bell, A. R., Blandford, R., Berger, R. L., Bingham, R., Casner, A., Chen, L. E., Foster, J., Froula, D. H., Goyon, C., Kalantar, D., Koenig, M., Lahmann, B., Li, C. -K., Lu, Y., Palmer, C. A. J., Petrasso, R., Poole, H., Remington, B., Reville, B., Reyes, A., Rigby, A., Ryu, D., Swadling, G., Zylstra, A., Miniati, F., Sarkar, S., Schekochihin, A. A., Lamb, D. Q., and Gregori, G.
Abstract: Galaxy clusters are filled with hot, diffuse X-ray emitting plasma, with a stochastically tangled magnetic field whose energy is close to equipartition with the energy of the turbulent motions \cite{zweibel1997, Vacca}. In the cluster cores, the temperatures remain anomalously high compared to what might be expected considering that the radiative cooling time is short relative to the Hubble time \cite{cowie1977,fabian1994}. While feedback from the central active galactic nuclei (AGN) \cite{fabian2012,birzan2012,churazov2000} is believed to provide most of the heating, there has been a long debate as to whether conduction of heat from the bulk to the core can help the core to reach the observed temperatures \cite{narayan2001,ruszkowski2002,kunz2011}, given the presence of tangled magnetic fields. Interestingly, evidence of very sharp temperature gradients in structures like cold fronts implies a high degree of suppression of thermal conduction \cite{markevitch2007}. To address the problem of thermal conduction in a magnetized and turbulent plasma, we have created a replica of such a system in a laser laboratory experiment. Our data show a reduction of local heat transport by two orders of magnitude or more, leading to strong temperature variations on small spatial scales, as is seen in cluster plasmas \cite{markevitch2003}.
Published: 2021
Full Text: View/download PDF

24. Searching for low-mass dark matter via Migdal effect in COSINE-100

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We report on the search for weakly interacting massive particle (WIMP) dark matter candidates in the galactic halo that interact with sodium and iodine nuclei in the COSINE-100 experiment and produce energetic electrons that accompany recoil nuclei via the the Migdal effect. The WIMP mass sensitivity of previous COSINE-100 searches that relied on the detection of ionization signals produced by target nuclei recoiling from elastic WIMP-nucleus scattering was restricted to WIMP masses above $\sim$5 GeV/$c^2$ by the detectors' 1 keVee energy-electron-equivalent threshold. The search reported here looks for recoil signals enhanced by the Migdal electrons that are ejected during the scattering process. This is particularly effective for the detection of low-mass WIMP scattering from the crystals' sodium nuclei in which a relatively larger fraction of the WIMP's energy is transferred to the nucleus recoil energy and the excitation of its orbital electrons. In this analysis, the low-mass WIMP search window of the COSINE-100 experiment is extended to WIMP mass down to 200 MeV/$c^2$. The low-mass WIMP sensitivity will be further improved by lowering the analysis threshold based on a multivariable analysis technique. We consider the influence of these improvements and recent developments in detector performance to re-evaluate sensitivities for the future COSINE-200 experiment. With a 0.2 keVee analysis threshold and high light-yield NaI(Tl) detectors (22 photoelectrons/keVee), the COSINE-200 experiment can explore low-mass WIMPs down to 20 MeV/$c^2$ and probe previously unexplored regions of parameter space., Comment: 10 pages, 8 figures
Published: 2021
Full Text: View/download PDF

25. Strong constraints from COSINE-100 on the DAMA dark matter results using the same sodium iodide target

Author: Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scar, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scar, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We present new constraints on dark matter interactions using 1.7 years of COSINE-100 data. The COSINE-100 experiment, consisting of 106 kg of tallium-doped sodium iodide (NaI(Tl)) target material, is aimed at testing DAMA's claim of dark matter observation using the same NaI(Tl) detectors. Improved event selection requirements, a more precise understanding of the detector background and the use of a larger data set considerably enhances the COSINE-100 sensitivity for dark matter detection. No signal consistent with the dark matter interaction is identified, and rules out model-dependent dark matter interpretations of the DAMA signals in the specific context of standard halo model with the same NaI(Tl) target for various interaction hypotheses.
Published: 2021
Full Text: View/download PDF

26. Identification of new isomers in $^{228}$Ac : Impact on dark matter searches

Author: Kim, K. W., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Kim, K. W., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We report the identification of metastable isomeric states of $^{228}$Ac at 6.28 keV, 6.67 keV and 20.19 keV, with lifetimes of an order of 100 ns. These states are produced by the $\beta$-decay of $^{228}$Ra, a component of the $^{232}$Th decay chain, with $\beta$ Q-values of 39.52 keV, 39.13 keV and 25.61 keV, respectively. Due to its low Q-value as well as the relative abundance of $^{232}$Th and their progeny in low background experiments, these observations potentially impact the low-energy background modeling of dark matter search experiments., Comment: 9 pages, 9 figures
Published: 2021
Full Text: View/download PDF

27. Three-year annual modulation search with COSINE-100

Author: Collaboration, COSINE-100, Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Collaboration, COSINE-100, Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: COSINE-100 is a direct detection dark matter experiment that aims to test DAMA/LIBRA's claim of dark matter discovery by searching for a dark matter-induced annual modulation signal with NaI(Tl) detectors. We present new constraints on the annual modulation signal from a dataset with a 2.82 yr livetime utilizing an active mass of 61.3 kg, for a total exposure of 173 kg$\cdot$yr. This new result features an improved event selection that allows for both lowering the energy threshold to 1 keV and a more precise time-dependent background model. In the 1-6 keV and 2-6 keV energy intervals, we observe best-fit values for the modulation amplitude of 0.0067$\pm$0.0042 and 0.0051$\pm$0.0047 counts/(day$\cdot$kg$\cdot$keV), respectively, with a phase fixed at 152.5 days., Comment: 11 pages, 8 figures
Published: 2021
Full Text: View/download PDF

28. Searching for low-mass dark matter via Migdal effect in COSINE-100

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We report on the search for weakly interacting massive particle (WIMP) dark matter candidates in the galactic halo that interact with sodium and iodine nuclei in the COSINE-100 experiment and produce energetic electrons that accompany recoil nuclei via the the Migdal effect. The WIMP mass sensitivity of previous COSINE-100 searches that relied on the detection of ionization signals produced by target nuclei recoiling from elastic WIMP-nucleus scattering was restricted to WIMP masses above $\sim$5 GeV/$c^2$ by the detectors' 1 keVee energy-electron-equivalent threshold. The search reported here looks for recoil signals enhanced by the Migdal electrons that are ejected during the scattering process. This is particularly effective for the detection of low-mass WIMP scattering from the crystals' sodium nuclei in which a relatively larger fraction of the WIMP's energy is transferred to the nucleus recoil energy and the excitation of its orbital electrons. In this analysis, the low-mass WIMP search window of the COSINE-100 experiment is extended to WIMP mass down to 200 MeV/$c^2$. The low-mass WIMP sensitivity will be further improved by lowering the analysis threshold based on a multivariable analysis technique. We consider the influence of these improvements and recent developments in detector performance to re-evaluate sensitivities for the future COSINE-200 experiment. With a 0.2 keVee analysis threshold and high light-yield NaI(Tl) detectors (22 photoelectrons/keVee), the COSINE-200 experiment can explore low-mass WIMPs down to 20 MeV/$c^2$ and probe previously unexplored regions of parameter space., Comment: 10 pages, 8 figures
Published: 2021
Full Text: View/download PDF

29. Strong constraints from COSINE-100 on the DAMA dark matter results using the same sodium iodide target

Author: Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scar, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scar, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We present new constraints on dark matter interactions using 1.7 years of COSINE-100 data. The COSINE-100 experiment, consisting of 106 kg of tallium-doped sodium iodide (NaI(Tl)) target material, is aimed at testing DAMA's claim of dark matter observation using the same NaI(Tl) detectors. Improved event selection requirements, a more precise understanding of the detector background and the use of a larger data set considerably enhances the COSINE-100 sensitivity for dark matter detection. No signal consistent with the dark matter interaction is identified, and rules out model-dependent dark matter interpretations of the DAMA signals in the specific context of standard halo model with the same NaI(Tl) target for various interaction hypotheses.
Published: 2021
Full Text: View/download PDF

30. Identification of new isomers in $^{228}$Ac : Impact on dark matter searches

Author: Kim, K. W., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Kim, K. W., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We report the identification of metastable isomeric states of $^{228}$Ac at 6.28 keV, 6.67 keV and 20.19 keV, with lifetimes of an order of 100 ns. These states are produced by the $\beta$-decay of $^{228}$Ra, a component of the $^{232}$Th decay chain, with $\beta$ Q-values of 39.52 keV, 39.13 keV and 25.61 keV, respectively. Due to its low Q-value as well as the relative abundance of $^{232}$Th and their progeny in low background experiments, these observations potentially impact the low-energy background modeling of dark matter search experiments., Comment: 9 pages, 9 figures
Published: 2021
Full Text: View/download PDF

31. Three-year annual modulation search with COSINE-100

Author: Collaboration, COSINE-100, Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Collaboration, COSINE-100, Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: COSINE-100 is a direct detection dark matter experiment that aims to test DAMA/LIBRA's claim of dark matter discovery by searching for a dark matter-induced annual modulation signal with NaI(Tl) detectors. We present new constraints on the annual modulation signal from a dataset with a 2.82 yr livetime utilizing an active mass of 61.3 kg, for a total exposure of 173 kg$\cdot$yr. This new result features an improved event selection that allows for both lowering the energy threshold to 1 keV and a more precise time-dependent background model. In the 1-6 keV and 2-6 keV energy intervals, we observe best-fit values for the modulation amplitude of 0.0067$\pm$0.0042 and 0.0051$\pm$0.0047 counts/(day$\cdot$kg$\cdot$keV), respectively, with a phase fixed at 152.5 days., Comment: 11 pages, 8 figures
Published: 2021
Full Text: View/download PDF

32. Searching for low-mass dark matter via Migdal effect in COSINE-100

Author: Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Carlin, N., Choi, J. J., Choi, S., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Hollick, S. J., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kwon, H. J., Lee, D. H., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Park, S. D., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We report on the search for weakly interacting massive particle (WIMP) dark matter candidates in the galactic halo that interact with sodium and iodine nuclei in the COSINE-100 experiment and produce energetic electrons that accompany recoil nuclei via the the Migdal effect. The WIMP mass sensitivity of previous COSINE-100 searches that relied on the detection of ionization signals produced by target nuclei recoiling from elastic WIMP-nucleus scattering was restricted to WIMP masses above $\sim$5 GeV/$c^2$ by the detectors' 1 keVee energy-electron-equivalent threshold. The search reported here looks for recoil signals enhanced by the Migdal electrons that are ejected during the scattering process. This is particularly effective for the detection of low-mass WIMP scattering from the crystals' sodium nuclei in which a relatively larger fraction of the WIMP's energy is transferred to the nucleus recoil energy and the excitation of its orbital electrons. In this analysis, the low-mass WIMP search window of the COSINE-100 experiment is extended to WIMP mass down to 200 MeV/$c^2$. The low-mass WIMP sensitivity will be further improved by lowering the analysis threshold based on a multivariable analysis technique. We consider the influence of these improvements and recent developments in detector performance to re-evaluate sensitivities for the future COSINE-200 experiment. With a 0.2 keVee analysis threshold and high light-yield NaI(Tl) detectors (22 photoelectrons/keVee), the COSINE-200 experiment can explore low-mass WIMPs down to 20 MeV/$c^2$ and probe previously unexplored regions of parameter space., Comment: 10 pages, 8 figures
Published: 2021
Full Text: View/download PDF

33. Alpha backgrounds in the AMoRE-Pilot experiment

Author: Alenkov, V., Bae, H. W., Beyer, J., Boiko, R. S., Boonin, K., Buzanov, O., Chanthima, N., Cheoun, M. K., Choi, S. H., Danevich, F. A., Djamal, M., Drung, D., Enss, C., Fleischmann, A., Gangapshev, A., Gastaldo, L., Gavriljuk, Yu. M., Gezhaev, A., Grigoryeva, V. D., Gurentsov, V., Ha, D. H., Ha, C., Ha, E. J., Hahn, I., Jeon, E. J., Jeon, J., Jo, H. S., Kaewkhao, J., Kang, C. S., Kang, S. J., Kang, W. G., Karki, S., Kazalov, V., Khan, A., Khan, S., Kim, D. -Y., Kim, G. W., Kim, H. B., Kim, H. J., Kim, H. L., Kim, H. S., Kim, I., Kim, W. T., Kim, S., Kim, S. C., Kim, S. K., Kim, Y. D., Kim, Y. H., Kirdsiri, K., Ko, Y. J., Kobychev, V. V., Kornoukhov, V., Kuzminov, V., Kwon, D. H., Lee, C., Lee, E. K., Lee, H. J., Lee, H. S., Lee, J., Lee, J. S., Lee, J. Y., Lee, K. B., Lee, M. H., Lee, M. K., Lee, S. H., Lee, S. W., Leonard, D. S., Li, J., Li, Y., Limkitjaroenporn, P., Mailyan, B., Makarov, E. P., Oh, S. Y., Oh, Y. M., Gileva, O., Olsen, S., Pabitra, A., Panasenko, S., Pandey, I., Park, C. W., Park, H. K., Park, H. S., Park, K. S., Park, S. Y., Polischuk, O. G., Prihtiadi, H., Ra, S. J., Ratkevich, S., Rooh, G., Sari, M. B., Seo, J., Seo, K. M., Shin, J. W., Shin, K. A., Shlegel, V. N., Siyeon, K., Sokur, N. V., Son, J. -K., Srisittipokakun, N., Toibaev, N., Tretyak, V. I., Wirawan, R., Woo, K. R., Yoon, Y. S., Yue, Q., Alenkov, V., Bae, H. W., Beyer, J., Boiko, R. S., Boonin, K., Buzanov, O., Chanthima, N., Cheoun, M. K., Choi, S. H., Danevich, F. A., Djamal, M., Drung, D., Enss, C., Fleischmann, A., Gangapshev, A., Gastaldo, L., Gavriljuk, Yu. M., Gezhaev, A., Grigoryeva, V. D., Gurentsov, V., Ha, D. H., Ha, C., Ha, E. J., Hahn, I., Jeon, E. J., Jeon, J., Jo, H. S., Kaewkhao, J., Kang, C. S., Kang, S. J., Kang, W. G., Karki, S., Kazalov, V., Khan, A., Khan, S., Kim, D. -Y., Kim, G. W., Kim, H. B., Kim, H. J., Kim, H. L., Kim, H. S., Kim, I., Kim, W. T., Kim, S., Kim, S. C., Kim, S. K., Kim, Y. D., Kim, Y. H., Kirdsiri, K., Ko, Y. J., Kobychev, V. V., Kornoukhov, V., Kuzminov, V., Kwon, D. H., Lee, C., Lee, E. K., Lee, H. J., Lee, H. S., Lee, J., Lee, J. S., Lee, J. Y., Lee, K. B., Lee, M. H., Lee, M. K., Lee, S. H., Lee, S. W., Leonard, D. S., Li, J., Li, Y., Limkitjaroenporn, P., Mailyan, B., Makarov, E. P., Oh, S. Y., Oh, Y. M., Gileva, O., Olsen, S., Pabitra, A., Panasenko, S., Pandey, I., Park, C. W., Park, H. K., Park, H. S., Park, K. S., Park, S. Y., Polischuk, O. G., Prihtiadi, H., Ra, S. J., Ratkevich, S., Rooh, G., Sari, M. B., Seo, J., Seo, K. M., Shin, J. W., Shin, K. A., Shlegel, V. N., Siyeon, K., Sokur, N. V., Son, J. -K., Srisittipokakun, N., Toibaev, N., Tretyak, V. I., Wirawan, R., Woo, K. R., Yoon, Y. S., and Yue, Q.
Abstract: The Advanced Mo-based Rare process Experiment (AMoRE)-Pilot experiment is an initial phase of the AMoRE search for neutrinoless double beta decay of $^{100}$Mo, with the purpose of investigating the level and sources of backgrounds. Searches for neutrinoless double beta decay generally require ultimately low backgrounds. Surface $\alpha$ decays on the crystals themselves or nearby materials can deposit a continuum of energies that can be as high as the $Q$-value of the decay itself and may fall in the region of interest (ROI). To understand these background events, we studied backgrounds from radioactive contaminations internal to and on the surface of the crystals or nearby materials with Geant4-based Monte Carlo simulations. In this study, we report on the measured $\alpha$ energy spectra fitted with the corresponding simulated spectra for six crystal detectors, where sources of background contributions could be identified through high energy $\alpha$ peaks and continuum parts in the energy spectrum for both internal and surface contaminations. We determine the low-energy contributions from internal and surface $\alpha$ contaminations by extrapolating from the $\alpha$ background fitting model.
Published: 2021
Full Text: View/download PDF

34. Strong suppression of heat conduction in a laboratory replica of galaxy-cluster turbulent plasmas

Author: Meinecke, J., Tzeferacos, P., Ross, J. S., Bott, A. F. A., Feister, S., Park, H. -S., Bell, A. R., Blandford, R., Berger, R. L., Bingham, R., Casner, A., Chen, L. E., Foster, J., Froula, D. H., Goyon, C., Kalantar, D., Koenig, M., Lahmann, B., Li, C. -K., Lu, Y., Palmer, C. A. J., Petrasso, R., Poole, H., Remington, B., Reville, B., Reyes, A., Rigby, A., Ryu, D., Swadling, G., Zylstra, A., Miniati, F., Sarkar, S., Schekochihin, A. A., Lamb, D. Q., Gregori, G., Meinecke, J., Tzeferacos, P., Ross, J. S., Bott, A. F. A., Feister, S., Park, H. -S., Bell, A. R., Blandford, R., Berger, R. L., Bingham, R., Casner, A., Chen, L. E., Foster, J., Froula, D. H., Goyon, C., Kalantar, D., Koenig, M., Lahmann, B., Li, C. -K., Lu, Y., Palmer, C. A. J., Petrasso, R., Poole, H., Remington, B., Reville, B., Reyes, A., Rigby, A., Ryu, D., Swadling, G., Zylstra, A., Miniati, F., Sarkar, S., Schekochihin, A. A., Lamb, D. Q., and Gregori, G.
Abstract: Galaxy clusters are filled with hot, diffuse X-ray emitting plasma, with a stochastically tangled magnetic field whose energy is close to equipartition with the energy of the turbulent motions \cite{zweibel1997, Vacca}. In the cluster cores, the temperatures remain anomalously high compared to what might be expected considering that the radiative cooling time is short relative to the Hubble time \cite{cowie1977,fabian1994}. While feedback from the central active galactic nuclei (AGN) \cite{fabian2012,birzan2012,churazov2000} is believed to provide most of the heating, there has been a long debate as to whether conduction of heat from the bulk to the core can help the core to reach the observed temperatures \cite{narayan2001,ruszkowski2002,kunz2011}, given the presence of tangled magnetic fields. Interestingly, evidence of very sharp temperature gradients in structures like cold fronts implies a high degree of suppression of thermal conduction \cite{markevitch2007}. To address the problem of thermal conduction in a magnetized and turbulent plasma, we have created a replica of such a system in a laser laboratory experiment. Our data show a reduction of local heat transport by two orders of magnitude or more, leading to strong temperature variations on small spatial scales, as is seen in cluster plasmas \cite{markevitch2003}.
Published: 2021
Full Text: View/download PDF

35. Strong constraints from COSINE-100 on the DAMA dark matter results using the same sodium iodide target

Author: Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scar, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scar, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We present new constraints on dark matter interactions using 1.7 years of COSINE-100 data. The COSINE-100 experiment, consisting of 106 kg of tallium-doped sodium iodide (NaI(Tl)) target material, is aimed at testing DAMA's claim of dark matter observation using the same NaI(Tl) detectors. Improved event selection requirements, a more precise understanding of the detector background and the use of a larger data set considerably enhances the COSINE-100 sensitivity for dark matter detection. No signal consistent with the dark matter interaction is identified, and rules out model-dependent dark matter interpretations of the DAMA signals in the specific context of standard halo model with the same NaI(Tl) target for various interaction hypotheses.
Published: 2021
Full Text: View/download PDF

36. Background modeling for dark matter search with 1.7 years of COSINE-100 data

Author: Adhikari, G., Adhikari, P., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, G. S., Kim, H., Kim, H. J., Kim, K. W., Kim, N. Y., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kudryavtsev, V. A., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Lynch, W. A., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., Adhikari, P., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, G. S., Kim, H., Kim, H. J., Kim, K. W., Kim, N. Y., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Kudryavtsev, V. A., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Lynch, W. A., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We present a background model for dark matter searches using an array of NaI(Tl) crystals in the COSINE-100 experiment that is located in the Yangyang underground laboratory. The model includes background contributions from both internal and external sources, including cosmogenic radionuclides and surface $^{210}$Pb contamination. To build the model in the low energy region, with a threshold of 1 keV, we used a depth profile of $^{210}$Pb contamination in the surface of the NaI(Tl) crystals determined in a comparison between measured and simulated spectra. We also considered the effect of the energy scale errors propagated from the statistical uncertainties and the nonlinear detector response at low energies. The 1.7 years COSINE-100 data taken between October 21, 2016 and July 18, 2018 were used for this analysis. Our Monte Carlo simulation provides a non-Gaussian peak around 50 keV originating from beta decays of bulk $^{210}$Pb in a good agreement with the measured background. This model estimates that the activities of bulk $^{210}$Pb and $^{3}$H are dominating the background rate that amounts to an average level of 2.85$\pm$0.15 counts/day/keV/kg in the energy region of (1-6) keV, using COSINE-100 data with a total exposure of 97.7 kg$\cdot$years.
Published: 2021
Full Text: View/download PDF

37. The environmental monitoring system at the COSINE-100 experiment

Author: Kim, H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H. J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Kim, H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Joo, H. W., Kang, W. G., Kauer, M., Kim, H. J., Kim, K. W., Kim, S. H., Kim, S. K., Kim, W. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H., Lee, H. S., Lee, H. Y., Lee, I. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Lee, S. M., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: The COSINE-100 experiment is designed to test the DAMA experiment which claimed an observation of a dark matter signal from an annual modulation in their residual event rate. To measure the 1 %-level signal amplitude, it is crucial to control and monitor nearly all environmental quantities that might systematically mimic the signal. The environmental monitoring also helps ensure a stable operation of the experiment. Here, we describe the design and performance of the centralized environmental monitoring system for the COSINE-100 experiment., Comment: 13 pages, 11 figures
Published: 2021
Full Text: View/download PDF

38. Improving the production efficiency of high-titania slag in Ti extraction process : fluxing effect on formation of pseudobrookite

Author: Kim, D. H., Heo, J. H., Park, H. S., Kim, J. K., Park, Joo Hyun, Kim, D. H., Heo, J. H., Park, H. S., Kim, J. K., and Park, Joo Hyun
Abstract: We investigated the carbothermic reduction process of ilmenite ore at 1873 K with flux addition. Without flux, the pseudobrookite phase with a high melting temperature was precipitated during ilmenite smelting. This could be the main reason for decreased reduction of iron in ilmenite. To accelerate reduction of ilmenite, two factors were considered. One is increasing the reduction driving force during smelting. Activity of FeO is the major factor to control reduction in driving force. The other factor is delay in formation of the pseudobrookite phase, a high-melting point precipitation phase. In this system, MgO in ilmenite could be used to form pseudobrookite. To control these factors, in this study, flux agent (i.e., Na2O or SiO2) addition was considered. The thermochemical simulation program, FactSageTM7.0 was used to calculate the viscosity of slag and the activity of components as fluxing agents were added. High-temperature experiments using an induction furnace were also conducted to confirm the computational results. To determine the composition of final products, i.e., titanium slag, X-ray fluorescence analysis was executed. As a result of Fe and Ti behaviours in slag, SiO2 addition showed no significant difference from the slag without flux. However, Fe reduction in ilmenite, i.e. TiO2-enrichment, was more accelerated when Na2O was added. X-ray diffraction, scanning electron microscopic and transmission electron microscopic analyses results also showed that even 1 wt% Na2O addition significantly influenced the titanium slag production compared to no flux addition., QC 20200618
Published: 2020
Full Text: View/download PDF

39. The COSINE-100 Liquid Scintillator Veto System

Author: Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: This paper describes the liquid scintillator veto system for the COSINE-100 dark matter experiment and its performance. The COSINE-100 detector consists of eight NaI(Tl) crystals immersed in 2200~L of linear alkylbenzene-based liquid scintillator. The liquid scintillator tags between 65 and 75\% of the internal $^{40}$K background in the 2--6 keV energy region. We also describe the background model for the liquid scintillator, which is primarily used to assess its energy calibration and threshold.
Published: 2020
Full Text: View/download PDF

40. Search for sterile neutrino oscillation using RENO and NEOS data

Author: Atif, Z., Choi, J. H., Han, B. Y., Jang, C. H., Jang, H. I., Jang, J. S., Jeon, E. J., Jeon, S. H., Joo, K. K., Ju, K., Jung, D. E., Kim, H. J., Kim, H. S., Kim, J. G., Kim, J. H., Kim, B. R., Kim, J. Y., Kim, S. B., Kim, S. Y., Kim, W., Kim, Y. D., Ko, Y. J., Kwon, E., Lee, D. H., Lee, H. G., Lee, J., Lee, J. Y., Lee, M. H., Oh, Y. M., Lim, I. T., Moon, D. H., Park, H. K., Park, H. S., Park, K. S., Pac, M. Y., Seo, H., Seo, J. W., Seo, K. M., Shin, C. D., Siyeon, K., Sun, G. M., Yang, B. S., Yoo, J., Yoon, S. G., Yeo, I. S., Yu, I., Atif, Z., Choi, J. H., Han, B. Y., Jang, C. H., Jang, H. I., Jang, J. S., Jeon, E. J., Jeon, S. H., Joo, K. K., Ju, K., Jung, D. E., Kim, H. J., Kim, H. S., Kim, J. G., Kim, J. H., Kim, B. R., Kim, J. Y., Kim, S. B., Kim, S. Y., Kim, W., Kim, Y. D., Ko, Y. J., Kwon, E., Lee, D. H., Lee, H. G., Lee, J., Lee, J. Y., Lee, M. H., Oh, Y. M., Lim, I. T., Moon, D. H., Park, H. K., Park, H. S., Park, K. S., Pac, M. Y., Seo, H., Seo, J. W., Seo, K. M., Shin, C. D., Siyeon, K., Sun, G. M., Yang, B. S., Yoo, J., Yoon, S. G., Yeo, I. S., and Yu, I.
Abstract: We present a reactor model independent search for sterile neutrino oscillation using 2\,509\,days of RENO near detector data and 180 days of NEOS data. The reactor related systematic uncertainties are significantly suppressed as both detectors are located at the same reactor complex of Hanbit Nuclear Power Plant. The search is performed by electron antineutrino\,($\overline{\nu}_e$) disappearance between six reactors and two detectors with baselines of 294\,m\,(RENO) and 24\,m\,(NEOS). A spectral comparison of the NEOS prompt-energy spectrum with a no-oscillation prediction from the RENO measurement can explore reactor $\overline{\nu}_e$ oscillations to sterile neutrino. Based on the comparison, we obtain a 95\% C.L. excluded region of $0.1<|\Delta m_{41}^2|<7$\,eV$^2$. We also obtain a 68\% C.L. allowed region with the best fit of $|\Delta m_{41}^2|=2.41\,\pm\,0.03\,$\,eV$^2$ and $\sin^2 2\theta_{14}$=0.08$\,\pm\,$0.03 with a p-value of 8.2\%. Comparisons of obtained reactor antineutrino spectra at reactor sources are made among RENO, NEOS, and Daya Bay to find a possible spectral variation., Comment: 6 pages, 5 figures: This manuscript has been significantly revised by the joint reanalysis by RENO and NEOS Collaborations. (In the previous edition, the RENO collaboration used publicly available NEOS data to evaluate the expected neutrino spectrum at NEOS.); auxiliary file for data release including error matrix (RENO_NEOS_data_release.txt)
Published: 2020
Full Text: View/download PDF

41. Search for sterile neutrino oscillation using RENO and NEOS data

Author: Atif, Z., Choi, J. H., Han, B. Y., Jang, C. H., Jang, H. I., Jang, J. S., Jeon, E. J., Jeon, S. H., Joo, K. K., Ju, K., Jung, D. E., Kim, H. J., Kim, H. S., Kim, J. G., Kim, J. H., Kim, B. R., Kim, J. Y., Kim, S. B., Kim, S. Y., Kim, W., Kim, Y. D., Ko, Y. J., Kwon, E., Lee, D. H., Lee, H. G., Lee, J., Lee, J. Y., Lee, M. H., Oh, Y. M., Lim, I. T., Moon, D. H., Park, H. K., Park, H. S., Park, K. S., Pac, M. Y., Seo, H., Seo, J. W., Seo, K. M., Shin, C. D., Siyeon, K., Sun, G. M., Yang, B. S., Yoo, J., Yoon, S. G., Yeo, I. S., Yu, I., Atif, Z., Choi, J. H., Han, B. Y., Jang, C. H., Jang, H. I., Jang, J. S., Jeon, E. J., Jeon, S. H., Joo, K. K., Ju, K., Jung, D. E., Kim, H. J., Kim, H. S., Kim, J. G., Kim, J. H., Kim, B. R., Kim, J. Y., Kim, S. B., Kim, S. Y., Kim, W., Kim, Y. D., Ko, Y. J., Kwon, E., Lee, D. H., Lee, H. G., Lee, J., Lee, J. Y., Lee, M. H., Oh, Y. M., Lim, I. T., Moon, D. H., Park, H. K., Park, H. S., Park, K. S., Pac, M. Y., Seo, H., Seo, J. W., Seo, K. M., Shin, C. D., Siyeon, K., Sun, G. M., Yang, B. S., Yoo, J., Yoon, S. G., Yeo, I. S., and Yu, I.
Abstract: We present a reactor model independent search for sterile neutrino oscillation using 2\,509\,days of RENO near detector data and 180 days of NEOS data. The reactor related systematic uncertainties are significantly suppressed as both detectors are located at the same reactor complex of Hanbit Nuclear Power Plant. The search is performed by electron antineutrino\,($\overline{\nu}_e$) disappearance between six reactors and two detectors with baselines of 294\,m\,(RENO) and 24\,m\,(NEOS). A spectral comparison of the NEOS prompt-energy spectrum with a no-oscillation prediction from the RENO measurement can explore reactor $\overline{\nu}_e$ oscillations to sterile neutrino. Based on the comparison, we obtain a 95\% C.L. excluded region of $0.1<|\Delta m_{41}^2|<7$\,eV$^2$. We also obtain a 68\% C.L. allowed region with the best fit of $|\Delta m_{41}^2|=2.41\,\pm\,0.03\,$\,eV$^2$ and $\sin^2 2\theta_{14}$=0.08$\,\pm\,$0.03 with a p-value of 8.2\%. Comparisons of obtained reactor antineutrino spectra at reactor sources are made among RENO, NEOS, and Daya Bay to find a possible spectral variation., Comment: 6 pages, 5 figures: This manuscript has been significantly revised by the joint reanalysis by RENO and NEOS Collaborations. (In the previous edition, the RENO collaboration used publicly available NEOS data to evaluate the expected neutrino spectrum at NEOS.); auxiliary file for data release including error matrix (RENO_NEOS_data_release.txt)
Published: 2020
Full Text: View/download PDF

42. Time-resolved fast turbulent dynamo in a laser plasma

Author: Bott, A. F. A., Tzeferacos, P., Chen, L., Palmer, C. A. J., Rigby, A., Bell, A., Bingham, R., Birkel, A., Graziani, C., Froula, D. H., Katz, J., Koenig, M., Kunz, M. W., Li, C. K., Meinecke, J., Miniati, F., Petrasso, R., Park, H. -S., Remington, B. A., Reville, B., Ross, J. S., Ryu, D., Ryutov, D., Séguin, F., White, T. G., Schekochihin, A. A., Lamb, D. Q., Gregori, G., Bott, A. F. A., Tzeferacos, P., Chen, L., Palmer, C. A. J., Rigby, A., Bell, A., Bingham, R., Birkel, A., Graziani, C., Froula, D. H., Katz, J., Koenig, M., Kunz, M. W., Li, C. K., Meinecke, J., Miniati, F., Petrasso, R., Park, H. -S., Remington, B. A., Reville, B., Ross, J. S., Ryu, D., Ryutov, D., Séguin, F., White, T. G., Schekochihin, A. A., Lamb, D. Q., and Gregori, G.
Abstract: Understanding magnetic-field generation and amplification in turbulent plasma is essential to account for observations of magnetic fields in the universe. A theoretical framework attributing the origin and sustainment of these fields to the so-called fluctuation dynamo was recently validated by experiments on laser facilities in low-magnetic-Prandtl-number plasmas ($\mathrm{Pm} < 1$). However, the same framework proposes that the fluctuation dynamo should operate differently when $\mathrm{Pm} \gtrsim 1$, the regime relevant to many astrophysical environments such as the intracluster medium of galaxy clusters. This paper reports a new experiment that creates a laboratory $\mathrm{Pm} \gtrsim 1$ plasma dynamo for the first time. We provide a time-resolved characterization of the plasma's evolution, measuring temperatures, densities, flow velocities and magnetic fields, which allows us to explore various stages of the fluctuation dynamo's operation. The magnetic energy in structures with characteristic scales close to the driving scale of the stochastic motions is found to increase by almost three orders of magnitude from its initial value and saturate dynamically. It is shown that the growth of these fields occurs exponentially at a rate that is much greater than the turnover rate of the driving-scale stochastic motions. Our results point to the possibility that plasma turbulence produced by strong shear can generate fields more efficiently at the driving scale than anticipated by idealized MHD simulations of the nonhelical fluctuation dynamo; this finding could help explain the large-scale fields inferred from observations of astrophysical systems., Comment: 12 pages, 9 figures
Published: 2020
Full Text: View/download PDF

43. The COSINE-100 Liquid Scintillator Veto System

Author: Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: This paper describes the liquid scintillator veto system for the COSINE-100 dark matter experiment and its performance. The COSINE-100 detector consists of eight NaI(Tl) crystals immersed in 2200~L of linear alkylbenzene-based liquid scintillator. The liquid scintillator tags between 65 and 75\% of the internal $^{40}$K background in the 2--6 keV energy region. We also describe the background model for the liquid scintillator, which is primarily used to assess its energy calibration and threshold.
Published: 2020
Full Text: View/download PDF

44. Mutation of ten-eleven translocation-2 is associated with increased risk of autoimmune disease in patients with myelodysplastic syndrome

Author: National Research Foundation of Korea, Ministry of Science, ICT and Future Planning (South Korea), Oh, Y. J., Shin, D. Y., Hwang, S. M., Kim, S. M., Im, K., Park, H. S., Kim, J. A., Song, Y. W., Márquez, Ana, Martín, J., Lee, D. S., Park, J. K., National Research Foundation of Korea, Ministry of Science, ICT and Future Planning (South Korea), Oh, Y. J., Shin, D. Y., Hwang, S. M., Kim, S. M., Im, K., Park, H. S., Kim, J. A., Song, Y. W., Márquez, Ana, Martín, J., Lee, D. S., and Park, J. K.
Abstract: Background/Aims: Myelodysplastic syndrome (MDS) is caused by genetic and epigenetic alteration of hematopoietic precursors and immune dysregulation. Approximately 20% of patients with MDS develop an autoimmune disease (AID). Here, we investigated whether particular genetic mutations are associated with AID in patients with MDS. Methods: Eighty-eight genetic mutations associated with myeloid malignancy were sequenced in 73 MDS patients. The association between these mutations and AID was then analyzed. Results: The median age of the 73 MDS patients was 70 years (interquartile range, 56 to 75), and 49 (67.1%) were male. AID was observed in 16 of 73 patients (21.9%). Mutations were detected in 57 (78.1%) patients. The percentage (68.8% vs. 80.7%, p = 0.32) and the mean number of mutations (1.8 ± 1.6 vs. 2.2 ± 1.8, p = 0.34) in MDS patients with or without AID were similar. However, the ten-eleven translocation-2 (TET2) mutation rate was significantly higher in patients with AID than in those without (31.3% vs. 5.3%, respectively; p = 0.001). All TET2 mutations were variants of strong clinical significance. Conclusions: Mutation of TET2 in patients with MDS may be associated with increased risk of developing AID.
Published: 2020

45. Lowering the energy threshold in COSINE-100 dark matter searches

Author: Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: COSINE-100 is a dark matter detection experiment that uses NaI(Tl) crystal detectors operating at the Yangyang underground laboratory in Korea since September 2016. Its main goal is to test the annual modulation observed by the DAMA/LIBRA experiment with the same target medium. Recently DAMA/LIBRA has released data with an energy threshold lowered to 1 keV, and the persistent annual modulation behavior is still observed at 9.5$\sigma$. By lowering the energy threshold for electron recoils to 1 keV, COSINE-100 annual modulation results can be compared to those of DAMA/LIBRA in a model-independent way. Additionally, the event selection methods provide an access to a few to sub-GeV dark matter particles using constant rate studies. In this article, we discuss the COSINE-100 event selection algorithm, its validation, and efficiencies near the threshold.
Published: 2020
Full Text: View/download PDF

46. Measurement of the cosmic muon annual and diurnal flux variation with the COSINE-100 detector

Author: Collaboration, COSINE-100, Prihtiadi, H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Ra, S. J., Rott, C., Shin, K. A., Scraff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Collaboration, COSINE-100, Prihtiadi, H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., França, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Ra, S. J., Rott, C., Shin, K. A., Scraff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: We report measurements of annual and diurnal modulations of the cosmic-ray muon rate in the Yangyang underground laboratory (Y2L) using 952 days of COSINE-100 data acquired between September 2016 and July 2019. A correlation of the muon rate with the atmospheric temperature is observed and its amplitude on the muon rate is determined. The effective atmospheric temperature and muon rate variations are positively correlated with a measured effective temperature coefficient of $\alpha_{T}$ = 0.80 $\pm$ 0.11. This result is consistent with a model of meson production in the atmosphere. We also searched for a diurnal modulation in the underground muon rate by comparing one-hour intervals. No significant diurnal modulation of the muon rate was observed., Comment: 12 pages, 9 figures
Published: 2020
Full Text: View/download PDF

47. The COSINE-100 Liquid Scintillator Veto System

Author: Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., Yu, G. H., Adhikari, G., de Souza, E. Barbosa, Carlin, N., Choi, J. J., Choi, S., Djamal, M., Ezeribe, A. C., Franca, L. E., Ha, C., Hahn, I. S., Jeon, E. J., Jo, J. H., Kang, W. G., Kauer, M., Kim, H., Kim, H. J., Kim, K. W., Kim, S. K., Kim, Y. D., Kim, Y. H., Ko, Y. J., Lee, E. K., Lee, H. S., Lee, J., Lee, J. Y., Lee, M. H., Lee, S. H., Leonard, D. S., Manzato, B. B., Maruyama, R. H., Neal, R. J., Olsen, S. L., Park, B. J., Park, H. K., Park, H. S., Park, K. S., Pitta, R. L. C., Prihtiadi, H., Ra, S. J., Rott, C., Shin, K. A., Scarff, A., Spooner, N. J. C., Thompson, W. G., Yang, L., and Yu, G. H.
Abstract: This paper describes the liquid scintillator veto system for the COSINE-100 dark matter experiment and its performance. The COSINE-100 detector consists of eight NaI(Tl) crystals immersed in 2200~L of linear alkylbenzene-based liquid scintillator. The liquid scintillator tags between 65 and 75\% of the internal $^{40}$K background in the 2--6 keV energy region. We also describe the background model for the liquid scintillator, which is primarily used to assess its energy calibration and threshold.
Published: 2020
Full Text: View/download PDF

48. ARIA pharmacy 2018 'Allergic rhinitis care pathways for community pharmacy'

Author: Bosnic-Anticevich, S, Costa, E, Menditto, E, Lourenço, O, Novellino, E, Bialek, S, Briedis, V, Buonaiuto, R, Chrystyn, H, Cvetkovski, B, Capua, S Di, Kritikos, V, Mair, A, Orlando, V, Paulino, E, Salimäki, J, Söderlund, R, Tan, R, Williams, D M, Wroczynski, P, Agache, I, Ansotegui, I J, Anto, J M, Bedbrook, A, Bachert, C, Bewick, M, Bindslev-Jensen, C, Brozek, J, Canonica, G W, Cardona, V, Carr, W, Casale, T, Chavannes, N H, Correia de Sousa, J, Cruz, A A, Czarlewski, W, De Carlo, G, Demoly, P, Devillier, P, Dykewicz, M S, Gaga, M, El-Gamal, Y, Fonseca, J, Fokkens, W J, Guzmán, M A, Haahtela, T, Hellings, P W, Illario, M, Ivancevich, J C, Just, J, Kaidashev, I, Khaitov, M, Khaltaev, N, Keil, T, Klimek, L, Kowalski, M L, Kuna, P, Kvedariene, V, Larenas-Linnemann, D, Laune, D, Le, L T T, Carlsen, K C Lodrup, Mahboub, B, Maier, D, Malva, J, Manning, P, Morais-Almeida, M, Mösges, R, Mullol, J, Münter, L, Murray, R, Naclerio, R, Namazova-Baranova, L, Nekam, K, Nyembue, T D, Okubo, K, O'Hehir, R E, Ohta, K, Okamoto, Y, Onorato, G L, Palkonen, S, Panzner, P, Papadopoulos, N G, Park, H S, Pawankar, R, Pfaar, O, Phillips, J, Plavec, D, Popov, T A, Potter, P, Prokopakis, E P, Roller-Wirnsberger, R E, Rottem, M, Ryan, D, Samolinski, B, Sanchez-Borges, M, Schunemann, H J, Sheikh, A, Sisul, J C, Somekh, D, Stellato, C, To, T, Todo-Bom, A, Tomazic, P V, Toppila-Salmi, S, Valero, A, Valiulis, A, Valovirta, E, Ventura, M T, Wagenmann, M, Wallace, D, Waserman, S, Wickman, Magnus, Yiallouros, P K, Yorgancioglu, A, Yusuf, O M, Zar, H J, Zernotti, M E, Zhang, L, Zidarn, M, Zuberbier, T, Bousquet, J, Bosnic-Anticevich, S, Costa, E, Menditto, E, Lourenço, O, Novellino, E, Bialek, S, Briedis, V, Buonaiuto, R, Chrystyn, H, Cvetkovski, B, Capua, S Di, Kritikos, V, Mair, A, Orlando, V, Paulino, E, Salimäki, J, Söderlund, R, Tan, R, Williams, D M, Wroczynski, P, Agache, I, Ansotegui, I J, Anto, J M, Bedbrook, A, Bachert, C, Bewick, M, Bindslev-Jensen, C, Brozek, J, Canonica, G W, Cardona, V, Carr, W, Casale, T, Chavannes, N H, Correia de Sousa, J, Cruz, A A, Czarlewski, W, De Carlo, G, Demoly, P, Devillier, P, Dykewicz, M S, Gaga, M, El-Gamal, Y, Fonseca, J, Fokkens, W J, Guzmán, M A, Haahtela, T, Hellings, P W, Illario, M, Ivancevich, J C, Just, J, Kaidashev, I, Khaitov, M, Khaltaev, N, Keil, T, Klimek, L, Kowalski, M L, Kuna, P, Kvedariene, V, Larenas-Linnemann, D, Laune, D, Le, L T T, Carlsen, K C Lodrup, Mahboub, B, Maier, D, Malva, J, Manning, P, Morais-Almeida, M, Mösges, R, Mullol, J, Münter, L, Murray, R, Naclerio, R, Namazova-Baranova, L, Nekam, K, Nyembue, T D, Okubo, K, O'Hehir, R E, Ohta, K, Okamoto, Y, Onorato, G L, Palkonen, S, Panzner, P, Papadopoulos, N G, Park, H S, Pawankar, R, Pfaar, O, Phillips, J, Plavec, D, Popov, T A, Potter, P, Prokopakis, E P, Roller-Wirnsberger, R E, Rottem, M, Ryan, D, Samolinski, B, Sanchez-Borges, M, Schunemann, H J, Sheikh, A, Sisul, J C, Somekh, D, Stellato, C, To, T, Todo-Bom, A, Tomazic, P V, Toppila-Salmi, S, Valero, A, Valiulis, A, Valovirta, E, Ventura, M T, Wagenmann, M, Wallace, D, Waserman, S, Wickman, Magnus, Yiallouros, P K, Yorgancioglu, A, Yusuf, O M, Zar, H J, Zernotti, M E, Zhang, L, Zidarn, M, Zuberbier, T, and Bousquet, J
Abstract: Pharmacists are trusted health professionals. Many patients use over-the-counter (OTC) medications and are seen by pharmacists who are the initial point of contact of allergic rhinitis management in most countries. The role of pharmacists in integrated care pathways (ICPs) for allergic diseases is important. This paper builds on existing studies and provides tools intended to help pharmacists provide optimal advice/interventions/strategies to patients with rhinitis. The ARIA-pharmacy ICP includes a diagnostic questionnaire specifically focusing attention on key symptoms and markers of the disease, a systematic Diagnosis Guide (including differential diagnoses) and a simple flowchart with proposed treatment for rhinitis and asthma multimorbidity. Key prompts for referral within the ICP are included. The use of technology is critical to enhance the management of AR. However, the ARIA-pharmacy ICP should be adapted to local health care environments/situations as regional (national) differences exist in pharmacy care.
Published: 2019
Full Text: View/download PDF

49. Allergic Rhinitis and its Impact on Asthma (ARIA) Phase 4 (2018) : Change management in allergic rhinitis and asthma multimorbidity using mobile technology

Author: Bousquet, Jean, Hellings, Peter W., Agache, Ioana, Amat, Flore, Annesi-Maesano, Isabella, Ansotegui, Ignacio J., Anto, Josep M., Bachert, Claus, Bateman, Eric D., Bedbrook, Anna, Bennoor, Kazi, Bewick, Mickael, Bindslev-Jensen, Carsten, Bosnic-Anticevich, Sinthia, Bosse, Isabelle, Brozek, Jan, Brussino, Luisa, Canonica, Giorgio W., Cardona, Victoria, Casale, Thomas, Sarabia, Alfonso M. Cepeda, Chavannes, Niels H., Cecchi, Lorenzo, de Sousa, Jaime Correia, Costa, Elisio, Cruz, Alvaro A., Czarlewski, Wienczyslawa, De Carlo, Giuseppe, De Feo, Giulia, Demoly, Pascal, Devillier, Philippe, Dykewicz, Mark S., El-Gamal, Yehia, Eller, Esben E., Fonseca, Joao A., Fontaine, Jean-Francois, Fokkens, Wytske J., Guzman, Maria-Antonieta, Haahtela, Tari, Illario, Maddalena, Ivancevich, Juan-Carlos, Just, Jocelyne, Kaidashev, Igor, Khaitov, Musa, Kalayci, Omer, Keil, Thomas, Klimek, Ludger, Kowalski, Marek L., Kuna, Piotr, Kvedariene, Violeta, Larenas-Linnemann, Desiree, Laune, Daniel, Le, Lan T. T., Carlsen, Karin Lodrup, Lourenco, Olga, Mahboub, Bassam, Mair, Alpana, Menditto, Enrica, Milenkovic, Branislava, Morais-Almeida, Mario, Mosges, Ralph, Mullol, Joaquim, Murray, Ruth, Naclerio, Robert, Namazova-Baranova, Leyla, Novellino, Ettore, O'Hehir, Robyn E., Ohta, Ken, Okamoto, Yoshitaka, Okubo, Kimi, Onorato, Gabrielle L., Palkonen, Susanna, Panzner, Petr, Papadopoulos, Nikos G., Park, Hae-Sim, Paulino, Ema, Pawankar, Ruby, Pfaar, Oliver, Plavec, Davor, Popov, Ted A., Potter, Paul, Prokopakis, Emmanuel P., Rottem, Menachem, Ryan, Dermot, Salimaki, Johanna, Samolinski, Boleslaw, Sanchez-Borges, Mario, Schunemann, Holger J., Sheikh, Aziz, Sisul, Juan-Carlos, Rajabian-Soderlund, Rojin, Sooronbaev, Talant, Stellato, Cristiana, To, Teresa, Todo-Bom, Ana-Maria, Tomazic, Peter-Valentin, Toppila-Salmi, Sanna, Valero, Antonio, Valiulis, Arunas, Valovirta, Erkka, Ventura, Maria-Teresa, Wagenmann, Martin, Wang, De Yun, Wallace, Dana, Waserman, Susan, Wickman, Magnus, Yorgancioglu, Arzu, Zhang, Luo, Zhong, Nanshan, Zidarn, Mihaela, Zuberbier, Torsten, Bousquet, J., Hellings, P. W., Aberer, W., Agache, I., Akdis, C. A., Akdis, M., Alberti, M. R., Almeida, R., Amat, F., Angles, R., Annesi-Maesano, I., Ansotegui, I. J., Anto, J. M., Arnavielle, S., Asayag, E., Asarnoj, A., Arshad, H., Avolio, F., Bacci, E., Bachert, C., Baiardini, I., Barbara, C., Barbagallo, M., Baroni, I., Barreto, B. A., Basagana, X., Bateman, E. D., Bedolla-Barajas, M., Bedbrook, A., Bewick, M., Beghe, B., Bel, E. H., Bergmann, K. C., Bennoor, K. S., Benson, M., Bertorello, L., Biaoszewski, A. Z., Bieber, T., Bialek, S., Bindslev-Jensen, C., Bjermer, L., Blain, H., Blasi, F., Blua, A., Marciniak, M. Bochenska, Bogus-Buczynska, I., Boner, A. L., Bonini, M., Bonini, S., Bosnic-Anticevich, C. S., Bosse, I., Bouchard, J., Boulet, L. P., Bourret, R., Bousquet, P. J., Braido, F., Briedis, V., Brightling, C. E., Brozek, J., Bucca, C., Buhl, R., Buonaiuto, R., Panaitescu, C., Cabanas, M. T. Burguete, Burte, E., Bush, A., Caballero-Fonseca, F., Caillot, D., Caimmi, D., Calderon, M. A., Camargos, P. A. M., Camuzat, T., Canfora, G., Canonica, G. W., Cardona, V., Carlsen, K. H., Carreiro-Martins, P., Carriazo, A. M., Carr, W., Cartier, C., Casale, T., Castellano, G., Cecchi, L., Sarabia, A. M. Cepeda, Chavannes, N. H., Chen, Y., Chiron, R., Chivato, T., Chkhartishvili, E., Chuchalin, A. G., Chung, K. F., Ciaravolo, M. M., Ciceran, A., Cingi, C., Ciprandi, G., Coehlo, A. C. Carvalho, Colas, L., Colgan, E., Coll, J., Conforti, D., de Sousa, J. Correia, Cortes-Grimaldo, R. M., Corti, F., Costa, E., Costa-Dominguez, C., Courbis, A. L., Cox, L., Crescenzo, M., Cruz, A. A., Custovic, A., Czarlewski, W., Dahlen, S. E., Dario, C., da Silva, J., Dauvilliers, Y., Darsow, U., De Blay, F., De Carlo, G., Dedeu, T., Emerson, M. de Fatima, De Feo, G., De Vries, G., De Martino, B., Rubini, N. de Paula Motta, Deleanu, D., Demoly, P., Denburg, J. A., Devillier, P., Ercolano, S. Di Capua, Di Carluccio, N., Didier, A., Dokic, D., Dominguez-Silva, M. G., Douagui, H., Dray, G., Dubakiene, R., Durham, S. R., Du Toit, G., Dykewicz, M. S., El-Gamal, Y., Eklund, Patrik, Eller, E., Emuzyte, R., Farrell, J., Farsi, A., de Mello, J. Ferreira, Jr., Ferrero, J., Fink-Wagner, A., Fiocchi, A., Fokkens, W. J., Fonseca, J. A., Fontaine, J. F., Forti, S., Fuentes-Perez, J. M., Galvez-Romero, J. L., Gamkrelidze, A., Garcia-Aymerich, J., Garcia-Cobas, C. Y., Garcia-Cruz, M. H., Gemicioglu, B., Genova, S., Christoff, G., Gereda, J. E., van Wijk, R. Gerth, Gomez, R. M., Gomez-Vera, J., Diaz, S. Gonzalez, Gotua, M., Grisle, I., Guidacci, M., Guldemond, N. A., Gutter, Z., Guzman, M. A., Haahtela, T., Hajjam, J., Hernandez, L., Hourihane, J. O 'B., Huerta-Villalobos, Y. R., Humbert, M., Iaccarino, G., Illario, M., Ivancevich, J. C., Jares, E. J., Jassem, E., Johnston, S. L., Joos, G., Jung, K. S., Jutel, M., Kaidashev, I., Kalayci, O., Kalyoncu, A. F., Karjalainen, J., Kardas, P., Keil, T., Keith, P. K., Khaitov, M., Khaltaev, N., Kleine-Tebbe, J., Klimek, L., Kowalski, M. L., Kuitunen, M., Kull, I., Kuna, P., Kupczyk, M., Kvedariene, V., Krzych-Fata, E., Lacwik, P., Larenas-Linnemann, D., Laune, D., Lauri, D., Lavrut, J., Le, L. T. T., Lessa, M., Levato, G., Li, J., Lieberman, P., Lipiec, A., Lipworth, B., Carlsen, K. C. Lodrup, Louis, R., Lourenco, O., Luna-Pech, J. A., Maciej, K., Magnan, A., Mahboub, B., Maier, D., Mair, A., Majer, I., Malva, J., Mandajieva, E., Manning, P., Keenoy, E. De Manuel, Marshall, G. D., Masjedi, M. R., Maspero, J. F., Mathieu-Dupas, E., Campos, J. J. Matta, Matos, A. L., Maurer, M., Mavale-Manuel, S., Mayora, O., Medina-Avalos, M. A., Melen, E., Melo-Gomes, E., Meltzer, E. O., Menditto, E., Mercier, J., Miculinic, N., Mihaltan, F., Milenkovic, B., Moda, G., Mogica-Martinez, M. D., Mohammad, Y., Momas, I., Montefort, S., Monti, R., Bogado, D. Mora, Morais-Almeida, M., Morato-Castro, F. F., Mosges, R., Mota-Pinto, A., Santo, P. Moura, Mullol, J., Munter, L., Muraro, A., Murray, R., Naclerio, R., Nadif, R., Nalin, M., Napoli, L., Namazova-Baranova, L., Neffen, H., Niedeberger, V., Nekam, K., Neou, A., Nieto, A., Nogueira-Silva, L., Nogues, M., Novellino, E., Nyembue, T. D., O'Hehir, R. E., Odzhakova, C., Ohta, K., Okamoto, Y., Okubo, K., Onorato, G. L., Cisneros, M. Ortega, Ouedraogo, S., Pali-Scholl, I., Palkonen, S., Panzner, P., Papadopoulos, N. G., Park, H. S., Papi, A., Passalacqua, G., Paulino, E., Pawankar, R., Pedersen, S., Pepin, J. L., Pereira, A. M., Persico, M., Pfaar, O., Phillips, J., Picard, R., Pigearias, B., Pin, I., Pitsios, C., Plavec, D., Pohl, W., Popov, T. A., Portejoie, F., Potter, P., Pozzi, A. C., Price, D., Prokopakis, E. P., Puy, R., Pugin, B., Ross, R. E. Pulido, Przemecka, M., Rabe, K. F., Raciborski, F., Rajabian-Soderlund, R., Reitsma, S., Ribeirinho, I., Rimmer, J., Rivero-Yeverino, D., Rizzo, J. A., Rizzo, M. C., Robalo-Cordeiro, C., Rodenas, F., Rodo, X., Gonzalez, M. Rodriguez, Rodriguez-Manas, L., Rolland, C., Valle, S. Rodrigues, Rodriguez, M. Roman, Romano, A., Rodriguez-Zagal, E., Rolla, G., Roller-Wirnsberger, R. E., Romano, M., Rosado-Pinto, J., Rosario, N., Rottem, M., Ryan, D., Sagara, H., Salimaki, J., Samolinski, B., Sanchez-Borges, M., Sastre-Dominguez, J., Scadding, G. K., Schunemann, H. J., Scichilone, N., Schmid-Grendelmeier, P., Serpa, F. S., Shamai, S., Sheikh, A., Sierra, M., Simons, F. E. R., Siroux, V., Sisul, J. C., Skrindo, I., Sole, D., Somekh, D., Sondermann, M., Sooronbaev, T., Sova, M., Sorensen, M., Sorlini, M., Spranger, O., Stellato, C., Stelmach, R., Stukas, R., Sunyer, J., Strozek, J., Szylling, A., Tebyrica, J. N., Thibaudon, M., To, T., Todo-Bom, A., Tomazic, P. V., Toppila-Salmi, S., Trama, U., Triggiani, M., Ulrik, C. Suppli, Urrutia-Pereira, M., Valenta, R., Valero, A., Valiulis, A., Valovirta, E., van Eerd, M., van Ganse, E., van Hague, M., Vandenplas, O., Ventura, M. T., Vezzani, G., Vasankari, T., Vatrella, A., Verissimo, M. T., Viart, F., Viegi, M., Vicheva, D., Vontetsianos, T., Wagenmann, M., Walker, S., Wallace, D., Wang, D. Y., Waserman, S., Werfel, T., Westman, M., Wickman, M., Williams, D. M., Williams, S., Wilson, N., Wright, J., Wroczynski, P., Yakovliev, P., Yawn, B. P., Yiallouros, P. K., Yorgancioglu, A., Yusuf, O. M., Zar, H. J., Zhang, L., Zhong, N., Zernotti, M. E., Zidarn, M., Zuberbier, T., Zubrinich, C., Zurkuhlen, A., Bousquet, Jean, Hellings, Peter W., Agache, Ioana, Amat, Flore, Annesi-Maesano, Isabella, Ansotegui, Ignacio J., Anto, Josep M., Bachert, Claus, Bateman, Eric D., Bedbrook, Anna, Bennoor, Kazi, Bewick, Mickael, Bindslev-Jensen, Carsten, Bosnic-Anticevich, Sinthia, Bosse, Isabelle, Brozek, Jan, Brussino, Luisa, Canonica, Giorgio W., Cardona, Victoria, Casale, Thomas, Sarabia, Alfonso M. Cepeda, Chavannes, Niels H., Cecchi, Lorenzo, de Sousa, Jaime Correia, Costa, Elisio, Cruz, Alvaro A., Czarlewski, Wienczyslawa, De Carlo, Giuseppe, De Feo, Giulia, Demoly, Pascal, Devillier, Philippe, Dykewicz, Mark S., El-Gamal, Yehia, Eller, Esben E., Fonseca, Joao A., Fontaine, Jean-Francois, Fokkens, Wytske J., Guzman, Maria-Antonieta, Haahtela, Tari, Illario, Maddalena, Ivancevich, Juan-Carlos, Just, Jocelyne, Kaidashev, Igor, Khaitov, Musa, Kalayci, Omer, Keil, Thomas, Klimek, Ludger, Kowalski, Marek L., Kuna, Piotr, Kvedariene, Violeta, Larenas-Linnemann, Desiree, Laune, Daniel, Le, Lan T. T., Carlsen, Karin Lodrup, Lourenco, Olga, Mahboub, Bassam, Mair, Alpana, Menditto, Enrica, Milenkovic, Branislava, Morais-Almeida, Mario, Mosges, Ralph, Mullol, Joaquim, Murray, Ruth, Naclerio, Robert, Namazova-Baranova, Leyla, Novellino, Ettore, O'Hehir, Robyn E., Ohta, Ken, Okamoto, Yoshitaka, Okubo, Kimi, Onorato, Gabrielle L., Palkonen, Susanna, Panzner, Petr, Papadopoulos, Nikos G., Park, Hae-Sim, Paulino, Ema, Pawankar, Ruby, Pfaar, Oliver, Plavec, Davor, Popov, Ted A., Potter, Paul, Prokopakis, Emmanuel P., Rottem, Menachem, Ryan, Dermot, Salimaki, Johanna, Samolinski, Boleslaw, Sanchez-Borges, Mario, Schunemann, Holger J., Sheikh, Aziz, Sisul, Juan-Carlos, Rajabian-Soderlund, Rojin, Sooronbaev, Talant, Stellato, Cristiana, To, Teresa, Todo-Bom, Ana-Maria, Tomazic, Peter-Valentin, Toppila-Salmi, Sanna, Valero, Antonio, Valiulis, Arunas, Valovirta, Erkka, Ventura, Maria-Teresa, Wagenmann, Martin, Wang, De Yun, Wallace, Dana, Waserman, Susan, Wickman, Magnus, Yorgancioglu, Arzu, Zhang, Luo, Zhong, Nanshan, Zidarn, Mihaela, Zuberbier, Torsten, Bousquet, J., Hellings, P. W., Aberer, W., Agache, I., Akdis, C. A., Akdis, M., Alberti, M. R., Almeida, R., Amat, F., Angles, R., Annesi-Maesano, I., Ansotegui, I. J., Anto, J. M., Arnavielle, S., Asayag, E., Asarnoj, A., Arshad, H., Avolio, F., Bacci, E., Bachert, C., Baiardini, I., Barbara, C., Barbagallo, M., Baroni, I., Barreto, B. A., Basagana, X., Bateman, E. D., Bedolla-Barajas, M., Bedbrook, A., Bewick, M., Beghe, B., Bel, E. H., Bergmann, K. C., Bennoor, K. S., Benson, M., Bertorello, L., Biaoszewski, A. Z., Bieber, T., Bialek, S., Bindslev-Jensen, C., Bjermer, L., Blain, H., Blasi, F., Blua, A., Marciniak, M. Bochenska, Bogus-Buczynska, I., Boner, A. L., Bonini, M., Bonini, S., Bosnic-Anticevich, C. S., Bosse, I., Bouchard, J., Boulet, L. P., Bourret, R., Bousquet, P. J., Braido, F., Briedis, V., Brightling, C. E., Brozek, J., Bucca, C., Buhl, R., Buonaiuto, R., Panaitescu, C., Cabanas, M. T. Burguete, Burte, E., Bush, A., Caballero-Fonseca, F., Caillot, D., Caimmi, D., Calderon, M. A., Camargos, P. A. M., Camuzat, T., Canfora, G., Canonica, G. W., Cardona, V., Carlsen, K. H., Carreiro-Martins, P., Carriazo, A. M., Carr, W., Cartier, C., Casale, T., Castellano, G., Cecchi, L., Sarabia, A. M. Cepeda, Chavannes, N. H., Chen, Y., Chiron, R., Chivato, T., Chkhartishvili, E., Chuchalin, A. G., Chung, K. F., Ciaravolo, M. M., Ciceran, A., Cingi, C., Ciprandi, G., Coehlo, A. C. Carvalho, Colas, L., Colgan, E., Coll, J., Conforti, D., de Sousa, J. Correia, Cortes-Grimaldo, R. M., Corti, F., Costa, E., Costa-Dominguez, C., Courbis, A. L., Cox, L., Crescenzo, M., Cruz, A. A., Custovic, A., Czarlewski, W., Dahlen, S. E., Dario, C., da Silva, J., Dauvilliers, Y., Darsow, U., De Blay, F., De Carlo, G., Dedeu, T., Emerson, M. de Fatima, De Feo, G., De Vries, G., De Martino, B., Rubini, N. de Paula Motta, Deleanu, D., Demoly, P., Denburg, J. A., Devillier, P., Ercolano, S. Di Capua, Di Carluccio, N., Didier, A., Dokic, D., Dominguez-Silva, M. G., Douagui, H., Dray, G., Dubakiene, R., Durham, S. R., Du Toit, G., Dykewicz, M. S., El-Gamal, Y., Eklund, Patrik, Eller, E., Emuzyte, R., Farrell, J., Farsi, A., de Mello, J. Ferreira, Jr., Ferrero, J., Fink-Wagner, A., Fiocchi, A., Fokkens, W. J., Fonseca, J. A., Fontaine, J. F., Forti, S., Fuentes-Perez, J. M., Galvez-Romero, J. L., Gamkrelidze, A., Garcia-Aymerich, J., Garcia-Cobas, C. Y., Garcia-Cruz, M. H., Gemicioglu, B., Genova, S., Christoff, G., Gereda, J. E., van Wijk, R. Gerth, Gomez, R. M., Gomez-Vera, J., Diaz, S. Gonzalez, Gotua, M., Grisle, I., Guidacci, M., Guldemond, N. A., Gutter, Z., Guzman, M. A., Haahtela, T., Hajjam, J., Hernandez, L., Hourihane, J. O 'B., Huerta-Villalobos, Y. R., Humbert, M., Iaccarino, G., Illario, M., Ivancevich, J. C., Jares, E. J., Jassem, E., Johnston, S. L., Joos, G., Jung, K. S., Jutel, M., Kaidashev, I., Kalayci, O., Kalyoncu, A. F., Karjalainen, J., Kardas, P., Keil, T., Keith, P. K., Khaitov, M., Khaltaev, N., Kleine-Tebbe, J., Klimek, L., Kowalski, M. L., Kuitunen, M., Kull, I., Kuna, P., Kupczyk, M., Kvedariene, V., Krzych-Fata, E., Lacwik, P., Larenas-Linnemann, D., Laune, D., Lauri, D., Lavrut, J., Le, L. T. T., Lessa, M., Levato, G., Li, J., Lieberman, P., Lipiec, A., Lipworth, B., Carlsen, K. C. Lodrup, Louis, R., Lourenco, O., Luna-Pech, J. A., Maciej, K., Magnan, A., Mahboub, B., Maier, D., Mair, A., Majer, I., Malva, J., Mandajieva, E., Manning, P., Keenoy, E. De Manuel, Marshall, G. D., Masjedi, M. R., Maspero, J. F., Mathieu-Dupas, E., Campos, J. J. Matta, Matos, A. L., Maurer, M., Mavale-Manuel, S., Mayora, O., Medina-Avalos, M. A., Melen, E., Melo-Gomes, E., Meltzer, E. O., Menditto, E., Mercier, J., Miculinic, N., Mihaltan, F., Milenkovic, B., Moda, G., Mogica-Martinez, M. D., Mohammad, Y., Momas, I., Montefort, S., Monti, R., Bogado, D. Mora, Morais-Almeida, M., Morato-Castro, F. F., Mosges, R., Mota-Pinto, A., Santo, P. Moura, Mullol, J., Munter, L., Muraro, A., Murray, R., Naclerio, R., Nadif, R., Nalin, M., Napoli, L., Namazova-Baranova, L., Neffen, H., Niedeberger, V., Nekam, K., Neou, A., Nieto, A., Nogueira-Silva, L., Nogues, M., Novellino, E., Nyembue, T. D., O'Hehir, R. E., Odzhakova, C., Ohta, K., Okamoto, Y., Okubo, K., Onorato, G. L., Cisneros, M. Ortega, Ouedraogo, S., Pali-Scholl, I., Palkonen, S., Panzner, P., Papadopoulos, N. G., Park, H. S., Papi, A., Passalacqua, G., Paulino, E., Pawankar, R., Pedersen, S., Pepin, J. L., Pereira, A. M., Persico, M., Pfaar, O., Phillips, J., Picard, R., Pigearias, B., Pin, I., Pitsios, C., Plavec, D., Pohl, W., Popov, T. A., Portejoie, F., Potter, P., Pozzi, A. C., Price, D., Prokopakis, E. P., Puy, R., Pugin, B., Ross, R. E. Pulido, Przemecka, M., Rabe, K. F., Raciborski, F., Rajabian-Soderlund, R., Reitsma, S., Ribeirinho, I., Rimmer, J., Rivero-Yeverino, D., Rizzo, J. A., Rizzo, M. C., Robalo-Cordeiro, C., Rodenas, F., Rodo, X., Gonzalez, M. Rodriguez, Rodriguez-Manas, L., Rolland, C., Valle, S. Rodrigues, Rodriguez, M. Roman, Romano, A., Rodriguez-Zagal, E., Rolla, G., Roller-Wirnsberger, R. E., Romano, M., Rosado-Pinto, J., Rosario, N., Rottem, M., Ryan, D., Sagara, H., Salimaki, J., Samolinski, B., Sanchez-Borges, M., Sastre-Dominguez, J., Scadding, G. K., Schunemann, H. J., Scichilone, N., Schmid-Grendelmeier, P., Serpa, F. S., Shamai, S., Sheikh, A., Sierra, M., Simons, F. E. R., Siroux, V., Sisul, J. C., Skrindo, I., Sole, D., Somekh, D., Sondermann, M., Sooronbaev, T., Sova, M., Sorensen, M., Sorlini, M., Spranger, O., Stellato, C., Stelmach, R., Stukas, R., Sunyer, J., Strozek, J., Szylling, A., Tebyrica, J. N., Thibaudon, M., To, T., Todo-Bom, A., Tomazic, P. V., Toppila-Salmi, S., Trama, U., Triggiani, M., Ulrik, C. Suppli, Urrutia-Pereira, M., Valenta, R., Valero, A., Valiulis, A., Valovirta, E., van Eerd, M., van Ganse, E., van Hague, M., Vandenplas, O., Ventura, M. T., Vezzani, G., Vasankari, T., Vatrella, A., Verissimo, M. T., Viart, F., Viegi, M., Vicheva, D., Vontetsianos, T., Wagenmann, M., Walker, S., Wallace, D., Wang, D. Y., Waserman, S., Werfel, T., Westman, M., Wickman, M., Williams, D. M., Williams, S., Wilson, N., Wright, J., Wroczynski, P., Yakovliev, P., Yawn, B. P., Yiallouros, P. K., Yorgancioglu, A., Yusuf, O. M., Zar, H. J., Zhang, L., Zhong, N., Zernotti, M. E., Zidarn, M., Zuberbier, T., Zubrinich, C., and Zurkuhlen, A.
Abstract: Allergic Rhinitis and its Impact on Asthma (ARIA) has evolved from a guideline by using the best approach to integrated care pathways using mobile technology in patients with allergic rhinitis (AR) and asthma multimorbidity. The proposed next phase of ARIA is change management, with the aim of providing an active and healthy life to patients with rhinitis and to those with asthma multimorbidity across the lifecycle irrespective of their sex or socioeconomic status to reduce health and social inequities incurred by the disease. ARIA has followed the 8-step model of Kotter to assess and implement the effect of rhinitis on asthma multimorbidity and to propose multimorbid guidelines. A second change management strategy is proposed by ARIA Phase 4 to increase self-medication and shared decision making in rhinitis and asthma multimorbidity. An innovation of ARIA has been the development and validation of information technology evidence-based tools (Mobile Airways Sentinel Network [MASK]) that can inform patient decisions on the basis of a self-care plan proposed by the health care professional.
Published: 2019
Full Text: View/download PDF

50. Adherence to treatment in allergic rhinitis using mobile technology : The MASK Study

Author: Menditto, Enrica, Costa, Elisio, Midao, Luis, Bosnic-Anticevich, Sinthia, Novellino, Ettore, Bialek, Slawomir, Briedis, Vitalis, Mair, Alpana, Rajabian-Soderlund, Rojin, Arnavielhe, Sylvie, Bedbrook, Anna, Czarlewski, Wienczyslawa, Annesi-Maesano, Isabella, Anto, Josep M., Devillier, Philippe, De Vries, Govert, Keil, Thomas, Sheikh, Aziz, Orlando, Valentina, Larenas-Linnemann, Desiree, Cecchi, Lorenzo, De Feo, Giulia, Illario, M., Stellato, Cristiana, Fonseca, Joao, Malva, Joao, Morais-Almeida, Mario, Pereira, Ana Maria, Todo-Bom, Ana Maria, Kvedariene, Violeta, Valiulis, Arunas, Bergmann, Karl Christian, Klimek, Ludger, Moesges, Ralph, Pfaar, Oliver, Zuberbier, Torsten, Cardona, Vicky, Mullol, Joaquim, Papadopoulos, Nikos G., Prokopakis, Emmanuel P., Bewick, Mike, Ryan, Dermot, Roller-Wirnsberger, Regina E., Tomazic, Peter Valentin, Cruz, Alvaro A., Kuna, Piotr, Samolinski, Boleslaw, Fokkens, Wytske J., Reitsma, Sietze, Bosse, Isabelle, Fontaine, Jean-Francois, Laune, Daniel, Haahtela, Tari, Toppila-Salmi, Sanna, Bachert, Claus, Hellings, Peter W., Melen, Erik, Wickman, Magnus, Bindslev-Jensen, Carsten, Eller, Esben, O'Hehir, Robyn E., Cingi, Cemal, Gemicioglu, Bilun, Kalayci, Omer, Ivancevich, Juan Carlos, Bousquet, Jean, Bousquet, J., Hellings, P. W., Aberer, W., Agache, I., Akdis, C. A., Akdis, M., Aliberti, M. R., Almeida, R., Amat, F., Angles, R., Annesi-Maesano, I., Ansotegui, I. J., Anto, J. M., Arnavielle, S., Asayag, E., Asarnoj, A., Arshad, H., Avolio, F., Bacci, E., Bachert, C., Baiar-Dini, I., Barbara, C., Barbagallo, M., Baroni, I., Barreto, B. A., Basagana, X., Bateman, E. D., Bedolla-Barajas, M., Bedbrook, A., Bewick, M., Beghe, B., Bel, E. H., Bergmann, K. C., Bennoor, K. S., Benson, M., Bertorello, L., Bialoszewski, A. Z., Bieber, T., Bialek, S., Bindslev-Jensen, C., Bjermer, L., Blain, H., Blasi, F., Blua, A., Marciniak, M. Bochenska, Bogus-Buczynska, I., Boner, A. L., Bonini, M., Bonini, S., Bosnic-Anticevich, C. S., Bosse, I., Bouchard, J., Boulet, L. P., Bourret, R., Bousquet, Pj, Braido, F., Briedis, V., Brightling, C. E., Brozek, J., Bucca, C., Buhl, R., Buonaiuto, R., Panaitescu, C., Cabanas, M. T. Burguete, Burte, E., Bush, A., Caballero-Fonseca, F., Caillaud, D., Caimmi, D., Calderon, M. A., Camargos, P. A. M., Camuzat, T., Canfora, G., Canonica, G. W., Cardona, V., Carlsen, K. H., Carreiro-Martins, P., Carriazo, A. M., Carr, W., Cartier, C., Casale, T., Castellano, G., Cecchi, L., Cepeda, A. M., Chavannes, N. H., Chen, Y., Chiron, R., Chivato, T., Chkhartishvili, E., Chuchalin, A. G., Chung, K. F., Ciaravolo, M. M., Ciceran, A., Cingi, C., Ciprandi, G., Coehlo, A. C. Carvalho, Colas, L., Colgan, E., Coll, J., Conforti, D., De Sousa, J. Correia, Cortes-Grimaldo, R. M., Corti, F., Costa, E., Costa-Dominguez, Mc, Al Courbis, F., Cox, L., Crescenzo, M., Cruz, A. A., Custovic, A., Czarlewski, W., Dahlen, S. E., D'Amato, Dario, C., da Silva, J., Dauvilliers, Y., Darsow, U., De Blay, F., De Carlo, G., Dedeu, T., Emerson, M. De Fatima, De Feo, G., De Vries, G., De Martino, B., Rubina, N. P. Motta, Deleanu, D., Demoly, P., Denburg, Ja, Devillier, P., Ercolano, S. Di Capua, Di Carluccio, N., Didier, A., Dokic, D., Dominguez-Silva, M. G., Douagui, H., Dray, G., Dubakiene, R., Durham, S. R., Du Toit, G., Dykewicz, M. S., El-Gamal, Y., Eklund, Patrik, Eller, E., Emuzyte, R., Farrell, J., Farsi, A., De Mello, J. Ferreira, Jr., Ferrero, J., Fink-Wagner, A., Fiocchi, A., Fok-Kens, W. J., Fonseca, Ja, Fontaine, J. F., Forti, S., Fuentes-Perez, J. M., Galvez-Romero, J. L., Gamkrelidze, A., Garcia-Aymerich, J., Garcia-Cobas, C. Y., Garcia-Cruz, M. H., Gemicioglu, B., Genova, S., Christoff, G., Gereda, J. E., Van Wijk, R. Gerth, Gomez, R. M., Gomez-Vera, J., Diaz, S. Gonzalez, Gotua, M., Grisle, I., Guidacci, M., Guldemond, Na, Gutter, Z., Guzman, Ma, Haahtela, T., Hajjam, J., Hernandez, L., Houri-Hane, J O ' B, Huerta-Villalobos, Y. R., Humbert, M., Iaccarino, G., Ispayeva, Z., Ivancevich, J. C., Jares, Ej, Jassem, E., Johnston, S. L., Joos, G., Jung, K. S., Just, J., Jutel, M., Kaidashev, I., Kalayci, O., Kalyoncu, A. F., Karjalainen, J., Kardas, P., Keil, T., Keith, P. K., Khaitov, M., Khaltaev, N., Kleine-Tebbe, J., Klimek, L., Kowalski, M. L., Kuitunen, M., Kull, I., Kuna, P., Kupczyk, M., Kvedariene, V., Krzych-Falta, E., Lacwik, P., Larenas-Linnemann, D., Laune, D., Lauri, D., Lavrut, J., Le, L. T. T., Lessa, M., Levato, G., Li, J., Lieberman, P., Liplec, A., Lipworth, B., Carlsen, K. C. Lodrup, Louis, R., Lourenco, O., Luna-Pech, J. A., Magnan, A., Mahboub, B., Maier, D., Mair, A., Majer, I., Malva, J., Mandajieva, E., Manning, P., Keenoy, E. De Manuel, Marshall, G. D., Masjedi, M. R., Maspero, J. F., Mathieu-Dupas, E., Campos, J. J. Matta, Matos, Al, Maurer, M., Mavale-Manuel, S., Mayora, O., Medina-Avalos, M. A., Melen, E., Melo-Gomes, E., Meltzer, Eo, Menditto, E., Mercier, J., Miculinic, N., Mihaltan, F., Milenkovic, B., Moda, G., Mogica-Martinez, M. D., Mohammad, Y., Momas, I., Monte-Fort, S., Monti, R., Bogado, D. Mora, Morais-Almeida, M., Morato-Castro, Mosges, R., Mota-Pinto, A., Santo, P. Moura, Mullol, J., Munter, L., Muraro, A., Murray, R., Naclerio, R., Nadif, R., Nalin, M., Napoli, L., Namazova-Baranova, L., Neffen, H., Niedeberger, V., Nekam, K., Neou, A., Nieto, A., Nogueira-Silva, L., Nogues, M., Novellino, E., Nyembue, Td, O'Hehir, Re, Odzhakova, C., Ohta, K., Okamoto, Y., Okubo, K., Onorato, G. L., Cisneros, M. Ortega, Ouedraogo, S., Pali-Scholl, I., Palkonen, S., Panzner, P., Papadopoulos, N. G., Park, H. S., Papi, A., Passalacqua, G., Paulino, E., Pawankar, R., Pedersen, S., Pepin, J. L., Pereira, A. M., Persico, M., Pfaar, O., Phillips, J., Picard, R., Pigearias, B., Pin, I., Pitsios, C., Plavec, D., Pohl, W., Popov, T. A., Portejoie, F., Potter, P., Pozzi, A. C., Price, D., Prokopakis, E. P., Puy, R., Pugin, B., Ross, R. E. Pulido, Przemecka, M., Rabe, K. F., Raciborski, F., Raja-Bian-Soderlund, R., Reitsma, S., Ribeirinho, I., Rimmer, J., Riv-Ero-Yeverino, D., Rizzo, J. A., Rizzo, M. C., Robalo-Cordeiro, C., Rodenas, F., Rodo, X., Gonzalez, M. Rodriguez, Rodriguez-Manas, L., Rolland, C., Valle, S. Rodrigues, Rodriguez, M. Roman, Romano, A., Rodriguez-Zagal, E., Rolla, G., Roller-Wirnsberger, R. E., Romano, M., Rosado-Pinto, J., Rosario, N., Rottem, M., Ryan, D., Sagara, H., Salimaki, J., Samolinski, B., Sanchez-Borges, M., Sastre-Dominguez, J., Scadding, G. K., Schunemann, H. J., Scichilone, N., Schmid-Grendelmeier, P., Serpa, F. S., Shamai, S., Sheikh, A., Sierra, M., Simons, F. E. R., Sir-Oux, V., Sisul, J. C., Skrindo, I., Sole, D., Somekh, D., Sonder-Mann, M., Sooronbaev, T., Sova, M., Sorensen, M., Sorlini, M., Spranger, O., Stellato, C., Stelmach, R., Stukas, R., Sunyer, J., Strozek, J., Szylling, A., Tebyrica, Jn, Thibaudon, M., To, T., Todo-Bom, A., Tomazic, P. V., Toppila-Salmi, S., Trama, U., Triggiani, M., Ulrik, C. Suppli, Urrutia-Pereira, M., Valenta, R., Valero, A., Valiulis, A., Valovirta, E., Van Eerd, M., Van Ganse, E., Van Hague, M., Vandenplas, O., Ventura, M. T., Vezzani, G., Vasankari, T., Vatrella, A., Verissimo, M. T., Viart, F., Viegi, G., Vicheva, D., Vontetsianos, T., Wagenmann, M., Walker, S., Wallace, D., Wang, D. Y., Waserman, S., Werfel, T., Westman, M., Wickman, M., Williams, D. M., Williams, S., Wilson, N., Wright, J., Wroczynski, P., Yakovliev, P., Yawn, B. P., Yiallouros, P. K., Yorgancioglu, A., Yusuf, O. M., Zar, H. J., Zhang, L., Zhong, N., Zernotti, M. E., Zhanat, I., Zidarn, M., Zuberbier, T., Zubrinich, C., Zurkuhlen, A., Menditto, Enrica, Costa, Elisio, Midao, Luis, Bosnic-Anticevich, Sinthia, Novellino, Ettore, Bialek, Slawomir, Briedis, Vitalis, Mair, Alpana, Rajabian-Soderlund, Rojin, Arnavielhe, Sylvie, Bedbrook, Anna, Czarlewski, Wienczyslawa, Annesi-Maesano, Isabella, Anto, Josep M., Devillier, Philippe, De Vries, Govert, Keil, Thomas, Sheikh, Aziz, Orlando, Valentina, Larenas-Linnemann, Desiree, Cecchi, Lorenzo, De Feo, Giulia, Illario, M., Stellato, Cristiana, Fonseca, Joao, Malva, Joao, Morais-Almeida, Mario, Pereira, Ana Maria, Todo-Bom, Ana Maria, Kvedariene, Violeta, Valiulis, Arunas, Bergmann, Karl Christian, Klimek, Ludger, Moesges, Ralph, Pfaar, Oliver, Zuberbier, Torsten, Cardona, Vicky, Mullol, Joaquim, Papadopoulos, Nikos G., Prokopakis, Emmanuel P., Bewick, Mike, Ryan, Dermot, Roller-Wirnsberger, Regina E., Tomazic, Peter Valentin, Cruz, Alvaro A., Kuna, Piotr, Samolinski, Boleslaw, Fokkens, Wytske J., Reitsma, Sietze, Bosse, Isabelle, Fontaine, Jean-Francois, Laune, Daniel, Haahtela, Tari, Toppila-Salmi, Sanna, Bachert, Claus, Hellings, Peter W., Melen, Erik, Wickman, Magnus, Bindslev-Jensen, Carsten, Eller, Esben, O'Hehir, Robyn E., Cingi, Cemal, Gemicioglu, Bilun, Kalayci, Omer, Ivancevich, Juan Carlos, Bousquet, Jean, Bousquet, J., Hellings, P. W., Aberer, W., Agache, I., Akdis, C. A., Akdis, M., Aliberti, M. R., Almeida, R., Amat, F., Angles, R., Annesi-Maesano, I., Ansotegui, I. J., Anto, J. M., Arnavielle, S., Asayag, E., Asarnoj, A., Arshad, H., Avolio, F., Bacci, E., Bachert, C., Baiar-Dini, I., Barbara, C., Barbagallo, M., Baroni, I., Barreto, B. A., Basagana, X., Bateman, E. D., Bedolla-Barajas, M., Bedbrook, A., Bewick, M., Beghe, B., Bel, E. H., Bergmann, K. C., Bennoor, K. S., Benson, M., Bertorello, L., Bialoszewski, A. Z., Bieber, T., Bialek, S., Bindslev-Jensen, C., Bjermer, L., Blain, H., Blasi, F., Blua, A., Marciniak, M. Bochenska, Bogus-Buczynska, I., Boner, A. L., Bonini, M., Bonini, S., Bosnic-Anticevich, C. S., Bosse, I., Bouchard, J., Boulet, L. P., Bourret, R., Bousquet, Pj, Braido, F., Briedis, V., Brightling, C. E., Brozek, J., Bucca, C., Buhl, R., Buonaiuto, R., Panaitescu, C., Cabanas, M. T. Burguete, Burte, E., Bush, A., Caballero-Fonseca, F., Caillaud, D., Caimmi, D., Calderon, M. A., Camargos, P. A. M., Camuzat, T., Canfora, G., Canonica, G. W., Cardona, V., Carlsen, K. H., Carreiro-Martins, P., Carriazo, A. M., Carr, W., Cartier, C., Casale, T., Castellano, G., Cecchi, L., Cepeda, A. M., Chavannes, N. H., Chen, Y., Chiron, R., Chivato, T., Chkhartishvili, E., Chuchalin, A. G., Chung, K. F., Ciaravolo, M. M., Ciceran, A., Cingi, C., Ciprandi, G., Coehlo, A. C. Carvalho, Colas, L., Colgan, E., Coll, J., Conforti, D., De Sousa, J. Correia, Cortes-Grimaldo, R. M., Corti, F., Costa, E., Costa-Dominguez, Mc, Al Courbis, F., Cox, L., Crescenzo, M., Cruz, A. A., Custovic, A., Czarlewski, W., Dahlen, S. E., D'Amato, Dario, C., da Silva, J., Dauvilliers, Y., Darsow, U., De Blay, F., De Carlo, G., Dedeu, T., Emerson, M. De Fatima, De Feo, G., De Vries, G., De Martino, B., Rubina, N. P. Motta, Deleanu, D., Demoly, P., Denburg, Ja, Devillier, P., Ercolano, S. Di Capua, Di Carluccio, N., Didier, A., Dokic, D., Dominguez-Silva, M. G., Douagui, H., Dray, G., Dubakiene, R., Durham, S. R., Du Toit, G., Dykewicz, M. S., El-Gamal, Y., Eklund, Patrik, Eller, E., Emuzyte, R., Farrell, J., Farsi, A., De Mello, J. Ferreira, Jr., Ferrero, J., Fink-Wagner, A., Fiocchi, A., Fok-Kens, W. J., Fonseca, Ja, Fontaine, J. F., Forti, S., Fuentes-Perez, J. M., Galvez-Romero, J. L., Gamkrelidze, A., Garcia-Aymerich, J., Garcia-Cobas, C. Y., Garcia-Cruz, M. H., Gemicioglu, B., Genova, S., Christoff, G., Gereda, J. E., Van Wijk, R. Gerth, Gomez, R. M., Gomez-Vera, J., Diaz, S. Gonzalez, Gotua, M., Grisle, I., Guidacci, M., Guldemond, Na, Gutter, Z., Guzman, Ma, Haahtela, T., Hajjam, J., Hernandez, L., Houri-Hane, J O ' B, Huerta-Villalobos, Y. R., Humbert, M., Iaccarino, G., Ispayeva, Z., Ivancevich, J. C., Jares, Ej, Jassem, E., Johnston, S. L., Joos, G., Jung, K. S., Just, J., Jutel, M., Kaidashev, I., Kalayci, O., Kalyoncu, A. F., Karjalainen, J., Kardas, P., Keil, T., Keith, P. K., Khaitov, M., Khaltaev, N., Kleine-Tebbe, J., Klimek, L., Kowalski, M. L., Kuitunen, M., Kull, I., Kuna, P., Kupczyk, M., Kvedariene, V., Krzych-Falta, E., Lacwik, P., Larenas-Linnemann, D., Laune, D., Lauri, D., Lavrut, J., Le, L. T. T., Lessa, M., Levato, G., Li, J., Lieberman, P., Liplec, A., Lipworth, B., Carlsen, K. C. Lodrup, Louis, R., Lourenco, O., Luna-Pech, J. A., Magnan, A., Mahboub, B., Maier, D., Mair, A., Majer, I., Malva, J., Mandajieva, E., Manning, P., Keenoy, E. De Manuel, Marshall, G. D., Masjedi, M. R., Maspero, J. F., Mathieu-Dupas, E., Campos, J. J. Matta, Matos, Al, Maurer, M., Mavale-Manuel, S., Mayora, O., Medina-Avalos, M. A., Melen, E., Melo-Gomes, E., Meltzer, Eo, Menditto, E., Mercier, J., Miculinic, N., Mihaltan, F., Milenkovic, B., Moda, G., Mogica-Martinez, M. D., Mohammad, Y., Momas, I., Monte-Fort, S., Monti, R., Bogado, D. Mora, Morais-Almeida, M., Morato-Castro, Mosges, R., Mota-Pinto, A., Santo, P. Moura, Mullol, J., Munter, L., Muraro, A., Murray, R., Naclerio, R., Nadif, R., Nalin, M., Napoli, L., Namazova-Baranova, L., Neffen, H., Niedeberger, V., Nekam, K., Neou, A., Nieto, A., Nogueira-Silva, L., Nogues, M., Novellino, E., Nyembue, Td, O'Hehir, Re, Odzhakova, C., Ohta, K., Okamoto, Y., Okubo, K., Onorato, G. L., Cisneros, M. Ortega, Ouedraogo, S., Pali-Scholl, I., Palkonen, S., Panzner, P., Papadopoulos, N. G., Park, H. S., Papi, A., Passalacqua, G., Paulino, E., Pawankar, R., Pedersen, S., Pepin, J. L., Pereira, A. M., Persico, M., Pfaar, O., Phillips, J., Picard, R., Pigearias, B., Pin, I., Pitsios, C., Plavec, D., Pohl, W., Popov, T. A., Portejoie, F., Potter, P., Pozzi, A. C., Price, D., Prokopakis, E. P., Puy, R., Pugin, B., Ross, R. E. Pulido, Przemecka, M., Rabe, K. F., Raciborski, F., Raja-Bian-Soderlund, R., Reitsma, S., Ribeirinho, I., Rimmer, J., Riv-Ero-Yeverino, D., Rizzo, J. A., Rizzo, M. C., Robalo-Cordeiro, C., Rodenas, F., Rodo, X., Gonzalez, M. Rodriguez, Rodriguez-Manas, L., Rolland, C., Valle, S. Rodrigues, Rodriguez, M. Roman, Romano, A., Rodriguez-Zagal, E., Rolla, G., Roller-Wirnsberger, R. E., Romano, M., Rosado-Pinto, J., Rosario, N., Rottem, M., Ryan, D., Sagara, H., Salimaki, J., Samolinski, B., Sanchez-Borges, M., Sastre-Dominguez, J., Scadding, G. K., Schunemann, H. J., Scichilone, N., Schmid-Grendelmeier, P., Serpa, F. S., Shamai, S., Sheikh, A., Sierra, M., Simons, F. E. R., Sir-Oux, V., Sisul, J. C., Skrindo, I., Sole, D., Somekh, D., Sonder-Mann, M., Sooronbaev, T., Sova, M., Sorensen, M., Sorlini, M., Spranger, O., Stellato, C., Stelmach, R., Stukas, R., Sunyer, J., Strozek, J., Szylling, A., Tebyrica, Jn, Thibaudon, M., To, T., Todo-Bom, A., Tomazic, P. V., Toppila-Salmi, S., Trama, U., Triggiani, M., Ulrik, C. Suppli, Urrutia-Pereira, M., Valenta, R., Valero, A., Valiulis, A., Valovirta, E., Van Eerd, M., Van Ganse, E., Van Hague, M., Vandenplas, O., Ventura, M. T., Vezzani, G., Vasankari, T., Vatrella, A., Verissimo, M. T., Viart, F., Viegi, G., Vicheva, D., Vontetsianos, T., Wagenmann, M., Walker, S., Wallace, D., Wang, D. Y., Waserman, S., Werfel, T., Westman, M., Wickman, M., Williams, D. M., Williams, S., Wilson, N., Wright, J., Wroczynski, P., Yakovliev, P., Yawn, B. P., Yiallouros, P. K., Yorgancioglu, A., Yusuf, O. M., Zar, H. J., Zhang, L., Zhong, N., Zernotti, M. E., Zhanat, I., Zidarn, M., Zuberbier, T., Zubrinich, C., and Zurkuhlen, A.
Abstract: Background: Mobile technology may help to better understand the adherence to treatment. MASK-rhinitis (Mobile Airways Sentinel NetworK for allergic rhinitis) is a patient-centred ICT system. A mobile phone app (the Allergy Diary) central to MASK is available in 22 countries. Objectives: To assess the adherence to treatment in allergic rhinitis patients using the Allergy Diary App. Methods: An observational cross-sectional study was carried out on all users who filled in the Allergy Diary from 1 January 2016 to 1 August 2017. Secondary adherence was assessed by using the modified Medication Possession Ratio (MPR) and the Proportion of days covered (PDC) approach. Results: A total of 12143 users were registered. A total of 6949 users reported at least one VAS data recording. Among them, 1887 users reported >= 7 VAS data. About 1195 subjects were included in the analysis of adherence. One hundred and thirty-six (11.28%) users were adherent (MPR >= 70% and PDC <= 1.25), 51 (4.23%) were partly adherent (MPR >= 70% and PDC = 1.50) and 176 (14.60%) were switchers. On the other hand, 832 (69.05%) users were non-adherent to medications (MPR <70%). Of those, the largest group was non-adherent to medications and the time interval was increased in 442 (36.68%) users. Conclusion and clinical relevance: Adherence to treatment is low. The relative efficacy of continuous vs on-demand treatment for allergic rhinitis symptoms is still a matter of debate. This study shows an approach for measuring retrospective adherence based on a mobile app. This also represents a novel approach for analysing medication-taking behaviour in a real-world setting.
Published: 2019
Full Text: View/download PDF

Catalog

Books, media, physical & digital resources

See catalog results

Searchworks

Select search scope, currently: Articles Catalog books, media & more in Jio Institute collections Articles journal articles & other e-resources

Search

Search Constraints

Refine your results

Search Limiters

Publication Year Range

Publication Type

Database

Publisher

242 results on '"Park, H. -S."'

Search Results

Catalog

Select search scope, currently: Articles

Catalog

books, media & more in Jio Institute collections

Articles

journal articles & other e-resources