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5,326 results on '"Rodríguez G"'

1. First Measurement of $a^0_2(1320)$ Polarized Photoproduction Cross Section

Author

GlueX Collaboration, Afzal, F., Akondi, C. S., Albrecht, M., Amaryan, M., Arrigo, S., Arroyave, V., Asaturyan, A., Austregesilo, A., Baldwin, Z., Barbosa, F., Barlow, J., Barriga, E., Barsotti, R., Barton, D., Baturin, V., Berdnikov, V. V., Black, T., Boeglin, W., Boer, M., Briscoe, W. J., Britton, T., Cao, S., Chudakov, E., Chung, G., Cole, P. L., Cortes, O., Crede, V., Dalton, M. M., Darulis, D., Deur, A., Dobbs, S., Dolgolenko, A., Dugger, M., Dzhygadlo, R., Ebersole, D., Edo, M., Egiyan, H., Erbora, T., Eugenio, P., Fabrizi, A., Fanelli, C., Fang, S., Fitches, J., Foda, A. M., Furletov, S., Gan, L., Gao, H., Gardner, A., Gasparian, A., Glazier, D. I., Gleason, C., Goryachev, V. S., Grube, B., Guo, J., Guo, L., Hernandez, J., Hernandez, K., Hoffman, N. D., Hornidge, D., Hou, G., Hurck, P., Hurley, A., Imoehl, W., Ireland, D. G., Ito, M. M., Jaegle, I., Jarvis, N. S., Jeske, T., Jing, M., Jones, R. T., Kakoyan, V., Kalicy, G., Khachatryan, V., Kourkoumelis, C., LaDuke, A., Larin, I., Lawrence, D., Lersch, D. I., Li, H., Liu, B., Livingston, K., Lolos, G. J., Lorenti, L., Lyubovitskij, V., Ma, R., Mahmood, A., Marukyan, H., Matveev, V., McCaughan, M., McCracken, M., Meyer, C. A., Miskimen, R., Mitchell, R. E., Mizutani, K., Moran, P., Neelamana, V., Ng, L., Nissen, E., Orešić, S., Ostrovidov, A. I., Papandreou, Z., Paudel, C., Pedroni, R., Pentchev, L., Peters, K. J., Prather, E., Veetil, L. Puthiya, Rakshit, S., Reinhold, J., Remington, A., Ritchie, B. G., Ritman, J., Rodriguez, G., Romanov, D., Saldana, K., Salgado, C., Schadmand, S., Schertz, A. M., Scheuer, K., Schick, A., Schmidt, A., Schumacher, R. A., Schwiening, J., Scott, M., Septian, N., Sharp, P., Shen, X., Shepherd, M. R., Sikes, J., Smith, A., Smith, E. S., Sober, D. I., Somov, A., Somov, S., Stevens, J. R., Strakovsky, I. I., Sumner, B., Suresh, K., Tarasov, V. V., Taylor, S., Teymurazyan, A., Thiel, A., Viducic, T., Whitlatch, T., Wickramaarachchi, N., Wunderlich, Y., Yu, B., Zarling, J., Zhang, Z., Zhou, X., and Zihlmann, B.

Subjects
Nuclear Experiment, High Energy Physics - Experiment
Abstract

We measure for the first time the differential photoproduction cross section $d\sigma/dt$ of the $a_2(1320)$ meson at an average photon beam energy of 8.5~GeV, using data with an integrated luminosity of 104~pb$^{-1}$ collected by the GlueX experiment. We fully reconstruct the $\gamma p \to \eta\pi^0 p$ reaction and perform a partial-wave analysis in the $a_2(1320)$ mass region with amplitudes that incorporate the linear polarization of the beam. This allows us to separate for the first time the contributions of natural- and unnatural-parity exchanges. These measurements provide novel information about the photoproduction mechanism, which is critical for the search for spin-exotic states., Comment: 8 pages, 4 figures plus supplemental material

Published
2025

2. Upper Limit on the Photoproduction Cross Section of the Spin-Exotic $\pi_1(1600)$

Author

GlueX Collaboration, Afzal, F., Akondi, C. S., Albrecht, M., Amaryan, M., Arrigo, S., Arroyave, V., Asaturyan, A., Austregesilo, A., Baldwin, Z., Barbosa, F., Barlow, J., Barriga, E., Barsotti, R., Barton, D., Baturin, V., Berdnikov, V. V., Black, T., Boeglin, W., Boer, M., Briscoe, W. J., Britton, T., Cao, S., Chudakov, E., Chung, G., Cole, P. L., Cortes, O., Crede, V., Dalton, M. M., Darulis, D., Deur, A., Dobbs, S., Dolgolenko, A., Dugger, M., Dzhygadlo, R., Ebersole, D., Edo, M., Egiyan, H., Erbora, T., Eugenio, P., Fabrizi, A., Fanelli, C., Fang, S., Fitches, J., Foda, A. M., Furletov, S., Gan, L., Gao, H., Gardner, A., Gasparian, A., Glazier, D., Gleason, C., Goryachev, V. S., Grube, B., Guo, J., Guo, L., Hernandez, J., Hernandez, K., Hoffman, N. D., Hornidge, D., Hou, G., Hurck, P., Hurley, A., Imoehl, W., Ireland, D. G., Ito, M. M., Jaegle, I., Jarvis, N. S., Jeske, T., Jing, M., Jones, R. T., Kakoyan, V., Kalicy, G., Khachatryan, V., Kourkoumelis, C., LaDuke, A., Larin, I., Lawrence, D., Lersch, D. I., Li, H., Liu, B., Livingston, K., Lolos, G. J., Lorenti, L., Lyubovitskij, V., Ma, R., Mack, D., Mahmood, A., Marukyan, H., Matveev, V., McCaughan, M., McCracken, M., Meyer, C. A., Miskimen, R., Mitchell, R. E., Mizutani, K., Neelamana, V., Ng, L., Nissen, E., Orešić, S., Ostrovidov, A. I., Papandreou, Z., Paudel, C., Pedroni, R., Pentchev, L., Peters, K. J., Prather, E., Rakshit, S., Reinhold, J., Remington, A., Ritchie, B. G., Ritman, J., Rodriguez, G., Romanov, D., Saldana, K., Salgado, C., Schadmand, S., Schertz, A. M., Scheuer, K., Schick, A., Schmidt, A., Schumacher, R. A., Schwiening, J., Septian, N., Sharp, P., Shen, X., Shepherd, M. R., Sikes, J., Smith, A., Smith, E. S., Sober, D. I., Somov, A., Somov, S., Stevens, J. R., Strakovsky, I. I., Sumner, B., Suresh, K., Tarasov, V. V., Taylor, S., Teymurazyan, A., Thiel, A., Viducic, T., Whitlatch, T., Wickramaarachchi, N., Wunderlich, Y., Yu, B., Zarling, J., Zhang, Z., Zhou, X., and Zihlmann, B.

Subjects
Nuclear Experiment, High Energy Physics - Experiment
Abstract

The spin-exotic hybrid meson $\pi_{1}(1600)$ is predicted to have a large decay rate to the $\omega\pi\pi$ final state. Using 76.6~pb$^{-1}$ of data collected with the GlueX detector, we measure the cross sections for the reactions $\gamma p \to \omega \pi^+ \pi^- p$, $\gamma p \to \omega \pi^0 \pi^0 p$, and $\gamma p\to\omega\pi^-\pi^0\Delta^{++}$ in the range $E_\gamma =$ 8-10 GeV. Using isospin conservation, we set the first upper limits on the photoproduction cross sections of the $\pi^{0}_{1}(1600)$ and $\pi^{-}_{1}(1600)$. We combine these limits with lattice calculations of decay widths and find that photoproduction of $\eta'\pi$ is the most sensitive two-body system to search for the $\pi_1(1600)$., Comment: 7 pages, 3 figures plus supplemental materials

Published
2024
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3. Measurement of Spin-Density Matrix Elements in $\Delta^{++}(1232)$ photoproduction

Author

Afzal, F., Akondi, C. S., Albrecht, M., Amaryan, M., Arrigo, S., Arroyave, V., Asaturyan, A., Austregesilo, A., Baldwin, Z., Barbosa, F., Barlow, J., Barriga, E., Barsotti, R., Barton, D., Baturin, V., Berdnikov, V. V., Black, T., Boeglin, W., Boer, M., Briscoe, W. J., Britton, T., Cao, S., Chudakov, E., Chung, G., Cole, P. L., Cortes, O., Crede, V., Dalton, M. M., Darulis, D., Deur, A., Dobbs, S., Dolgolenko, A., Dugger, M., Dzhygadlo, R., Ebersole, D., Edo, M., Egiyan, H., Erbora, T., Eugenio, P., Fabrizi, A., Fanelli, C., Fang, S., Fitches, J., Foda, A. M., Furletov, S., Gan, L., Gao, H., Gardner, A., Gasparian, A., Glazier, D. I., Gleason, C., Goryachev, V. S., Grube, B., Guo, J., Guo, L., Hernandez, J., Hernandez, K., Hoffman, N. D., Hornidge, D., Hou, G., Hurck, P., Hurley, A., Imoehl, W., Ireland, D. G., Ito, M. M., Jaegle, I., Jarvis, N. S., Jeske, T., Jing, M., Jones, R. T., Kakoyan, V., Kalicy, G., Khachatryan, V., Kourkoumelis, C., LaDuke, A., Larin, I., Lawrence, D., Lersch, D. I., Li, H., Liu, B., Livingston, K., Lolos, G. J., Lorenti, L., Lyubovitskij, V., Ma, R., Mack, D., Mahmood, A., Marukyan, H., Matveev, V., McCaughan, M., McCracken, M., Meyer, C. A., Miskimen, R., Mitchell, R. E., Mizutani, K., Neelamana, V., Ng, L., Nissen, E., Orešić, S., Ostrovidov, A. I., Papandreou, Z., Paudel, C., Pedroni, R., Pentchev, L., Peters, K. J., Prather, E., Rakshit, S., Reinhold, J., Remington, A., Ritchie, B. G., Ritman, J., Rodriguez, G., Romanov, D., Saldana, K., Salgado, C., Schadmand, S., Schertz, A. M., Scheuer, K., Schick, A., Schmidt, A., Schumacher, R. A., Schwiening, J., Septian, N., Sharp, P., Shen, X., Shepherd, M. R., Sikes, J., Smith, A., Smith, E. S., Sober, D. I., Somov, A., Somov, S., Stevens, J. R., Strakovsky, I. I., Sumner, B., Suresh, K., Tarasov, V. V., Taylor, S., Teymurazyan, A., Thiel, A., Viducic, T., Whitlatch, T., Wickramaarachchi, N., Wunderlich, Y., Yu, B., Zarling, J., Zhang, Z., Zhou, X., and Zihlmann, B.

Subjects
Nuclear Experiment
Abstract

We measure the spin-density matrix elements (SDMEs) of the $\Delta^{++}(1232)$ in the photoproduction reaction $\gamma p \to \pi^-\Delta^{++}(1232)$ with the GlueX experiment in Hall D at Jefferson Lab. The measurement uses a linearly--polarized photon beam with energies from $8.2$ to $8.8$~GeV and the statistical precision of the SDMEs exceeds the previous measurement by three orders of magnitude for the momentum transfer squared region below $1.4$ GeV$^2$. The data are sensitive to the previously undetermined relative sign between couplings in existing Regge-exchange models. Linear combinations of the extracted SDMEs allow for a decomposition into natural and unnatural--exchange amplitudes. We find that the unnatural exchange plays an important role in the low momentum transfer region.

Published
2024

4. Gliese 12 b: A temperate Earth-sized planet at 12 pc ideal for atmospheric transmission spectroscopy

Author

Kuzuhara, M., Fukui, A., Livingston, J. H., Caballero, J. A., de Leon, J. P., Hirano, T., Kasagi, Y., Murgas, F., Narita, N., Omiya, M., Orell-Miquel, Jaume, Palle, E., Changeat, Q., Esparza-Borges, E., Harakawa, H., Hellier, C., Hori, Yasunori, Ikuta, Kai, Ishikawa, H. T., Kodama, T., Kotani, T., Kudo, T., Morales, J. C., Mori, M., Nagel, E., Parviainen, H., Perdelwitz, V., Reiners, A., Ribas, I., Sanz-Forcada, J., Sato, B., Schweitzer, A., Tabernero, H. M., Takarada, T., Uyama, T., Watanabe, N., Zechmeister, M., García, N. Abreu, Aoki, W., Beichman, C., Béjar, V. J. S., Brandt, T. D., Calatayud-Borras, Y., Carleo, I., Charbonneau, D., Collins, K. A., Currie, T., Doty, J. P., Dreizler, S., Fernández-Rodríguez, G., Fukuda, I., Galán, D., Geraldía-González, S., González-Garcia, J., Hayashi, Y., Hedges, C., Henning, T., Hodapp, K., Ikoma, M., Isogai, K., Jacobson, S., Janson, M., Jenkins, J. M., Kagetani, T., Kambe, E., Kawai, Y., Kawauchi, K., Kokubo, E., Konishi, M., Korth, J., Krishnamurthy, V., Kurokawa, T., Kusakabe, N., Kwon, J., Laza-Ramos, A., Libotte, F., Luque, R., Madrigal-Aguado, A., Matsumoto, Y., Mawet, D., McElwain, M. W., Gallardo, P. P. Meni, Morello, G., Torres, S. Mu~noz, Nishikawa, J., Nugroho, S. K., Ogihara, M., Pel'aez-Torres, A., Rapetti, D., S'anchez-Benavente, M., Schlecker, M., Seager, S., Serabyn, E., Serizawa, T., Stangret, M., Takahashi, A., Teng, H., Tamura, M., Terada, Y., Ueda, A., Usuda, T., Vanderspek, R., Vievard, S., Watanabe, D., Winn, J. N., and Osorio, M. R. Zapatero

Subjects
Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Solar and Stellar Astrophysics
Abstract

Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets receiving low insolation is still small, limiting our ability to understand the diversity of the atmospheric composition and climates of temperate terrestrial planets. We report the discovery of an Earth-sized planet transiting the nearby (12 pc) inactive M3.0 dwarf Gliese 12 (TOI-6251) with an orbital period ($P_{\rm{orb}}$) of 12.76 days. The planet, Gliese 12b, was initially identified as a candidate with an ambiguous $P_{\rm{orb}}$ from TESS data. We confirmed the transit signal and $P_{\rm{orb}}$ using ground-based photometry with MuSCAT2 and MuSCAT3, and validated the planetary nature of the signal using high-resolution images from Gemini/NIRI and Keck/NIRC2 as well as radial velocity (RV) measurements from the InfraRed Doppler instrument on the Subaru 8.2 m telescope and from CARMENES on the CAHA 3.5 m telescope. X-ray observations with XMM-Newton showed the host star is inactive, with an X-ray-to-bolometric luminosity ratio of $\log L_{\rm X}/L_{\rm bol} \approx -5.7$. Joint analysis of the light curves and RV measurements revealed that Gliese 12b has a radius of 0.96 $\pm$ 0.05 $R_\oplus$, a 3$\sigma$ mass upper limit of 3.9 $M_\oplus$, and an equilibrium temperature of 315 $\pm$ 6 K assuming zero albedo. The transmission spectroscopy metric (TSM) value of Gliese 12b is close to the TSM values of the TRAPPIST-1 planets, adding Gliese 12b to the small list of potentially terrestrial, temperate planets amenable to atmospheric characterization with JWST., Comment: 29 pages (20 pages in main body), 13 figures (10 figures in main body). Equal contributions from M. K. and A. F.. Accepted for Publication in ApJL at 2024 March 21

Published
2024
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12. Measurement of Spin-Density Matrix Elements in $\rho(770)$ Production with a Linearly Polarized Photon Beam at $E_\gamma = 8.2\,-\,8.8\,\text{GeV}$

Author

GlueX Collaboration, Adhikari, S., Afzal, F., Akondi, C. S., Albrecht, M., Amaryan, M., Arroyave, V., Asaturyan, A., Austregesilo, A., Baldwin, Z., Barbosa, F., Barlow, J., Barriga, E., Barsotti, R., Beattie, T. D., Berdnikov, V. V., Black, T., Boeglin, W., Briscoe, W. J., Britton, T., Brooks, W. K., Byer, D., Chudakov, E., Cole, P. L., Cortes, O., Crede, V., Dalton, M. M., Darulis, D., Deur, A., Dobbs, S., Dolgolenko, A., Dotel, R., Dugger, M., Dzhygadlo, R., Ebersole, D., Edo, M., Egiyan, H., Erbora, T., Eugenio, P., Fabrizi, A., Fanelli, C., Fang, S., Fegan, S., Fitches, J., Foda, A. M., Furletov, S., Gan, L., Gao, H., Gardner, A., Gasparian, A., Gleason, C., Goetzen, K., Goryachev, V. S., Grube, B., Guo, J., Guo, L., Hague, T. J., Hakobyan, H., Hernandez, J., Hoffman, N. D., Hornidge, D., Hou, G., Huber, G. M., Hurck, P., Hurley, A., Imoehl, W., Ireland, D. G., Ito, M. M., Jaegle, I., Jarvis, N. S., Jeske, T., Jones, R. T., Kakoyan, V., Kalicy, G., Khachatryan, V., Khatchatryan, M., Kourkoumelis, C., LaDuke, A., Larin, I., Lawrence, D., Lersch, D. I., Li, H., Liu, B., Livingston, K., Lolos, G. J., Lorenti, L., Lyubovitskij, V., Ma, R., Mack, D., Mahmood, A., Marukyan, H., Matveev, V., McCaughan, M., McCracken, M., Meyer, C. A., Miskimen, R., Mitchell, R. E., Mizutani, K., Neelamana, V., Ng, L., Nissen, E., Orešić, S., Ostrovidov, A. I., Papandreou, Z., Paudel, C., Pedroni, R., Pentchev, L., Peters, K. J., Prather, E., Rakshit, S., Reinhold, J., Remington, A., Ritchie, B. G., Ritman, J., Rodriguez, G., Romanov, D., Saldana, K., Salgado, C., Schadmand, S., Schertz, A. M., Scheuer, K., Schick, A., Schmidt, A., Schumacher, R. A., Schwiening, J., Sharp, P., Shen, X., Shepherd, M. R., Smith, A., Smith, E. S., Sober, D. I., Somov, A., Somov, S., Stevens, J. R., Strakovsky, I. I., Sumner, B., Suresh, K., Tarasov, V. V., Taylor, S., Teymurazyan, A., Thiel, A., Viducic, T., Whitlatch, T., Wickramaarachchi, N., Williams, M., Wunderlich, Y., Yu, B., Zarling, J., Zhang, Z., Zhao, Z., Zhou, J., Zhou, X., and Zihlmann, B.

Subjects
Nuclear Experiment, High Energy Physics - Experiment
Abstract

The GlueX experiment at Jefferson Lab studies photoproduction of mesons using linearly polarized $8.5\,\text{GeV}$ photons impinging on a hydrogen target which is contained within a detector with near-complete coverage for charged and neutral particles. We present measurements of spin-density matrix elements for the photoproduction of the vector meson $\rho$(770). The statistical precision achieved exceeds that of previous experiments for polarized photoproduction in this energy range by orders of magnitude. We confirm a high degree of $s$-channel helicity conservation at small squared four-momentum transfer $t$ and are able to extract the $t$-dependence of natural and unnatural-parity exchange contributions to the production process in detail. We confirm the dominance of natural-parity exchange over the full $t$ range. We also find that helicity amplitudes in which the helicity of the incident photon and the photoproduced $\rho(770)$ differ by two units are negligible for $-t<0.5\,\text{GeV}^{2}/c^{2}$., Comment: 15 pages, 11 figures

Published
2023
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13. Measurement of the J/$\psi $ photoproduction cross section over the full near-threshold kinematic region

Author

GlueX Collaboration, Adhikari, S., Afzal, F., Akondi, C. S., Albrecht, M., Amaryan, M., Arroyave, V., Asaturyan, A., Austregesilo, A., Baldwin, Z., Barbosa, F., Barlow, J., Barriga, E., Barsotti, R., Beattie, T. D., Berdnikov, V. V., Black, T., Boeglin, W., Briscoe, W. J., Britton, T., Brooks, W. K., Byer, D., Chudakov, E., Cole, P. L., Cortes, O., Crede, V., Dalton, M. M., Darulis, D., Deur, A., Dobbs, S., Dolgolenko, A., Dotel, R., Dugger, M., Dzhygadlo, R., Ebersole, D., Egiyan, H., Erbora, T., Eugenio, P., Fabrizi, A., Fanelli, C., Fang, S., Fegan, S., Fitches, J., Foda, A. M., Furletov, S., Gan, L., Gao, H., Gardner, A., Gasparian, A., Gleason, C., Goetzen, K., Goryachev, V. S., Grube, B., Guo, J., Guo, L., Hague, T. J., Hakobyan, H., Hernandez, J., Hoffman, N. D., Hornidge, D., Hou, G., Huber, G. M., Hurck, P., Hurley, A., Imoehl, W., Ireland, D. G., Ito, M. M., Jaegle, I., Jarvis, N. S., Jeske, T., Jones, R. T., Kakoyan, V., Kalicy, G., Khachatryan, V., Khatchatryan, M., Kourkoumelis, C., LaDuke, A., Larin, I., Lawrence, D., Lersch, D. I., Li, H., Li, W. B., Liu, B., Livingston, K., Lolos, G. J., Lorenti, L., Lyubovitskij, V., Mack, D., Mahmood, A., Martel, P. P., Marukyan, H., Matveev, V., McCaughan, M., McCracken, M., Meyer, C. A., Miskimen, R., Mitchell, R. E., Mizutani, K., Neelamana, V., Ng, L., Nissen, E., Orei, S., Ostrovidov, A. I., Papandreou, Z., Paudel, C., Pedroni, R., Pentchev, L., Peters, K. J., Prather, E., Rakshit, S., Reinhold, J., Remington, A., Ritchie, B. G., Ritman, J., Rodriguez, G., Romanov, D., Saldana, K., Salgado, C., Schadmand, S., Schertz, A. M., Scheuer, K., Schick, A., Schmidt, A., Schumacher, R. A., Schwiening, J., Sharp, P., Shen, X., Shepherd, M. R., Smith, A., Smith, E. S., Sober, D. I., Somov, S., Somov, A., Stevens, J. R., Strakovsky, I. I., Sumner, B., Suresh, K., Tarasov, V. V., Taylor, S., Teymurazyan, A., Thiel, A., Viducic, T., Whitlatch, T., Wickramaarachchi, N., Williams, M., Wunderlich, Y., Yu, B., Zarling, J., Zhang, Z., Zhao, Z., Zhou, X., Zhou, J., and Zihlmann, B.

Subjects
Nuclear Experiment, High Energy Physics - Experiment
Abstract

We report the total and differential cross sections for $J/\psi$ photoproduction with the large acceptance GlueX spectrometer for photon beam energies from the threshold at 8.2~GeV up to 11.44~GeV and over the full kinematic range of momentum transfer squared, $t$. Such coverage facilitates the extrapolation of the differential cross sections to the forward ($t = 0$) point beyond the physical region. The forward cross section is used by many theoretical models and plays an important role in understanding $J/\psi$ photoproduction and its relation to the $J/\psi-$proton interaction. These measurements of $J/\psi$ photoproduction near threshold are also crucial inputs to theoretical models that are used to study important aspects of the gluon structure of the proton, such as the gluon Generalized Parton Distribution (GPD) of the proton, the mass radius of the proton, and the trace anomaly contribution to the proton mass. We observe possible structures in the total cross section energy dependence and find evidence for contributions beyond gluon exchange in the differential cross section close to threshold, both of which are consistent with contributions from open-charm intermediate states., Comment: 15 pages 18 figures

Published
2023
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22. Estudio cinético de la descomposición térmica del carbonato de Estroncio en el sistema SrCO3-Al2O3-SrSO4

Author

Torres T, J., Rodríguez G, J. A., and Almanza R, J. M.

Subjects
Kinetics, thermal gravimetric analysis, isothermal method, Mechanical activation, activation energy, Cinética, análisis termo gravimétrico, método isotérmico, activación mecánica, energía de activación, Clay industries. Ceramics. Glass, TP785-869
Abstract

The thermal decomposition of strontium carbonate in the SrCO3-Al2O3-SrSO4 system was studied by thermal analysis under isothermal experiments. Powder of reactive grade of SrCO3, Al2O3 y SrSO4 in molar ratio 3:3:1 were prepared. The powders were heat treated from 750 to 1000 °C for 4 h. Loss weight for each temperature was registered and the kinetics parameter were determine using the classical fit method. The effect of mechanical activation of SrCO3 was studied as well. The reaction mechanism for 750 to 900 °C temperature range corresponded to a geometric shrinkage in the grain boundary (R1.1) with an activation energy of 106. 21 Kjmol-1. The reaction mechanism for 900 to 1100 °C temperature range corresponded to a nucleation and growing (P1.1) with an activation energy of 44.87 Kjmol-1. The activation energy was reduced in 35% for the samples that contained SrCO3 mechanically activated.La cinética de descomposición térmica del carbonato de Estroncio (SrCO3) en el sistema SrCO3-Al2O3-SrSO4 se estudió por medio de análisis térmico gravimétrico (ATG), utilizando el método isotérmico. Se prepararon mezclas de polvos 3:3:1 molar de SrCO3, Al2O3 y SrSO4 grado reactivo, las cuales fueron homogenizadas y tratadas a temperaturas entre 750 hasta 1100°C, por periodo de 4 horas. Adicionalmente se estudio el efecto del tiempo de activación mecánica del SrCO3 sobre la cinética de descomposición. Se obtuvieron curvas representativas de la pérdida de peso de las muestras al incrementar la temperatura, a partir de ellas se realizó el estudio cinético. Para el rango de temperatura de 750 a 900°C, el mecanismo de reacción que rige el proceso de descomposición corresponde a una contracción geométrica mediante la frontera de grano (R1.1) con una energía de activación (Ea) de 106.21KJmol-1. En el rango de temperatura de 950 a 1100°C, el mecanismo de reacción que rige la descomposición corresponde a un proceso de nucleación y crecimiento (P1.1), con un valor de Ea de 44.87KJmol-1. La energía de activación disminuye conforme se incrementa el tiempo de activado mecánico hasta un 35% para el caso de siete horas.

Published
2008

25. Repeatability and reproducibility of the measurement of prepreg tack following ASTM D8336: Results of a round-robin study

Author

Joesbury, A.M., Endruweit, A., Budelmann, D., Giannis, S.P., De Focatiis, D.S.A., Call, D.B., Chan, C., Choong, G.Y.H., Clark, R.A., Collins, J.A., Fishpool, D.T., Garber, J.M., Ghose, S., Golding, J., Good, S.T., Jones, B.R., Meiners, D., Niitsoo, O., Palmer, C.T., Qian, C.C., Rivas, A.W., Santacruz Rodriguez, G., Stillwell, R.E., Vincent, J.D.S., and Yuan, H.

Published
2025
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26. A transient ultraluminous X-ray source in NGC 55

Author

Robba, A., Pinto, C., Pintore, F., Rodriguez, G., Ambrosi, E., Barra, F., Cusumano, G., D'Aì, A., Del Santo, M., Kosec, P., Marino, A., Middleton, M., Roberts, T., Salvaggio, C., Soria, R., Wolter, A., and Walton, D.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10$^{39}$ erg s$^{-1}$. The average number of ULXs per galaxy is still not well constrained, especially given the uncertainty on the fraction of ULX transients. Here, we report the identification of a new transient ULX in the galaxy NGC 55 (which we label as ULX-2), thanks to recent XMM-Newton and the Neil Gehrels Swift Observatory observations. This object was previously classified as a transient X-ray source with a luminosity around a few 10$^{38}$ erg s$^{-1}$ in a 2010 XMM-Newton observation. Thanks to new and deeper observations ($\sim$ 130 ks each), we show that the source reaches a luminosity peak $>1.6 \times 10^{39}$ erg s$^{-1}$. The X-ray spectrum of ULX-2 is much softer than in previous observations and fits in the class of soft ULXs. It can be well described using a model with two thermal components, as often found in ULXs. The time scales of the X-ray variability are of the order of a month and are likely driven by small changes in the accretion rate or due to super-orbital modulations, attributed to precession of the accretion disc, which is similar to other ULXs., Comment: 6 pages, including 4 figures and 2 tables, accepted for pubblication in MNRAS

Published
2022
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27. Inoculación de granadilla Passiflora ligularis L. con MVA

Author

Sánchez de Prager Marina, Rodríguez G. Angela María, and Hurtado Miguel

Subjects
fertilización fosfórica, inoculación, hongos micorrizógenos, cultivo, granadilla, Passiflora ligularis L., Agriculture
Abstract

For evaluating the possibilities of substitution of the phosphoric fertilization by means of the inoculation with micorrizogen fungi, in a granadilla crop in nursery stage; it was used hillside type soil with a pH of 4.8 and 2.0 ppm of P, in natural conditions and previous dessinfection. Individually was inoculated Acaulospora foveata, Glomus occultum, Acaulospora longula and it had a control in the native flora. Two hundred spores per experimental unit were applied in small granadilla plants transplanted recently. Three levels of P fertilization were proved (0, 25 and 50 kg of Triple Superphosphate per ha). After four months the variable were evaluated. Disinfection had a negative influence in plant development and in the efficientcy of Superphosphate captation. The best response in the development variables evaluated was obtained using 50 kg of Triple Superphosphate per ha, which indicates that in such type of soil, with low P availability, VAM do not reduce the use of fertilizer, but increases its efficiency in utilization for the plant. A. longula was the more effective micorrizal variety.Para evaluar las posibilidades de sustitución de fertilización fosfórica, mediante inoculación con hongos micorrizógenos, en el cultivo de la granadilla Passiflora ligularis L., en etapa de vivero, se trabajó con un suelo característico de zona de ladera con pH 4.8 y 2.1 ppm de P, en condiciones naturales y previa des infestación. Se inoculó individualmente: Acaulospora foveata, Glomus occultum, Acaulospora longula y se tuvo una condición testigo correspondiente a flora nativa. Se aplicó un promedio de 200 esporas/unidad experimental, en las plántulas de granadilla recién trasplantadas. Se probaron tres niveles de fertilización: (0, 25 y 50 kg de superfosfato triple/ha). La evaluación de las variables se hizo a los 4 meses de trasplante. La desinfestación influye negativamente en el desarrollo de las plantas y en la eficiencia de captación del superfosfato triple. La mejor respuesta en las variables de desarrollo evaluadas, se obtuvo con la aplicación de 50 kg de superfosfato triple/ha, lo cual indica que en este suelo, dada la baja disponibilidad de P, el recurso micorriza no permite disminuir dosis de fertilizante, sino que incrementa considerablemente su eficiencia de utilización por la planta. A. longula se comportó como la cepa más efectiva.

Published
1995

28. Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf

Author

Kawauchi, K., Murgas, F., Palle, E., Narita, N., Fukui, A., Hirano, T., Parviainen, H., Ishikawa, H. T., Watanabe, N., Esparaza-Borges, E., Kuzuhara, M., Orell-Miquel, J., Krishnamurthy, V., Mori, M., Kagetani, T., Zou, Y., Isogai, K., Livingston, J. H., Howell, S. B., Crouzet, N., de Leon, J. P., Kimura, T., Kodama, T., Korth, J., Kurita, S., Laza-Ramos, A., Luque, R., Madrigal-Aguado, A., Miyakawa, K., Morello, G., Nishiumi, T., Rodríguez, G. E. F., Sánchez-Benavente, M., Stangret, M., Teng, H., Terada, Y., Gnilka, C. L., Guerrero, N., Harakawa, H., Hodapp, K., Hori, Y., Ikoma, M., Jacobson, S., Konishi, M., Kotani, T., Kudo, T., Kurokowa, T., Kusakabe, N., Nishikawa, J., Omiya, M., Serizawa, T., Tamura, M., Ueda, A., and Vievard, S.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

The NASA space telescope $TESS$ is currently in the extended mission of its all-sky search for new transiting planets. Of the thousands of candidates that TESS is expected to deliver, transiting planets orbiting nearby M dwarfs are particularly interesting targets since they provide a great opportunity to characterize their atmospheres by transmission spectroscopy. We aim to validate and characterize the new sub-Neptune-sized planet candidate TOI-2136.01 orbiting a nearby M dwarf ($d = 33.36 \pm 0.02$ pc, $T_{eff} = 3373 \pm 108$ K) with an orbital period of 7.852 days. We use TESS data, ground-based multicolor photometry, and radial velocity measurements with the InfraRed Doppler (IRD) instrument on the Subaru Telescope to validate the planetary nature of TOI-2136.01 and estimate the stellar and planetary parameters. We also conduct high-resolution transmission spectroscopy to search for helium in its atmosphere. We confirmed that TOI-2136.01 (now named as TOI-2136b) is a bona fide planet with a planetary radius of $R_p = 2.2 \pm 0.07$ $R_{Earth}$ and a mass of $M_p = 4.7^{+3.1}_{-2.6}$ $M_{Earth}$. We also search for helium 10830 \r{A} absorption lines and place an upper limit on the equivalent width of $<$ 7.8 m\r{A} and on the absorption signal of $<$ 1.44 % with 95 % confidence. TOI-2136b is a sub-Neptune transiting a nearby and bright star (J=10.8) and is a potentially hycean planet, which is a new class of habitable planets with large oceans under a H$_2$-rich atmosphere, making it an excellent target for atmospheric studies to understand the formation, evolution, and habitability of the small planets., Comment: 19 pages, 16 figures, accepted for publication in Astronomy & Astrophysics

Published
2022
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29. TOI-1442 b and TOI-2445 b: two potentially rocky ultra-short period planets around M dwarfs

Author

Morello, G., Parviainen, H., Murgas, F., Pallé, E., Oshagh, M., Fukui, A., Hirano, T., Ishikawa, H. T., Mori, M., Narita, N., Collins, K. A., Barkaoui, K., Lewin, P., Cadieux, C., de Leon, J. P., Soubkiou, A., Garcia, N. Abreu, Crouzet, N., Esparza-Borges, E., Rodríguez, G. E. Fernández, Galán, D., Hori, Y., Ikoma, M., Isogai, K., Kagetani, T., Kawauchi, K., Kimura, T., Kodama, T., Korth, J., Kotani, T., Krishnamurthy, V., Kurita, S., Laza-Ramos, A., Livingston, J. H., Luque, R., Madrigal-Aguado, A., Nishiumi, T., Orell-Miquel, J., Puig-Subirà, M., Sánchez-Benavente, M., Stangret, M., Tamura, M., Terada, Y., Watanabe, N., Zou, Y., Benkhaldoun, Z., Collins, K. I., Doyon, R., Garcia, L., Ghachoui, M., Gillon, M., Jehin, E., Pozuelos, F. J., Schwarz, R. P., and Timmermans, M.

Subjects
Astrophysics - Earth and Planetary Astrophysics
Abstract

Context. Exoplanets with orbital periods of less than one day are known as ultra-short period (USP) planets. They are relatively rare products of planetary formation and evolution processes, but especially favourable for characterisation with current planet detection methods. At the time of writing, 125 USP planets have already been confirmed. Aims. Our aim is to validate the planetary nature of two new transiting planet candidates around M dwarfs announced by the NASA Transiting Exoplanet Survey Satellite (TESS), registered as TESS Objects of Interest (TOIs) TOI-1442.01 and TOI-2445.01. Methods. We used TESS data, ground-based photometric light curves, and Subaru/IRD spectrograph radial velocity (RV) measurements to validate both planetary candidates and to establish their physical properties. Results. TOI-1442 b is a validated exoplanet with an orbital period of $P$=0.4090682+/-0.0000004 d, a radius of $R_p$=1.15+/-0.06$R_{\oplus}$, and equilibrium temperature of $T_{p,eq}$=1357$_{-42}^{+49}$K. TOI-2445 b is also validated with an orbital period of $P$=0.3711286+/-0.0000004 d, a radius of $R_p$= 1.33+/-0.09$R_{\oplus}$, and equilibrium temperature of $T_{p,eq}$=1330$_{-56}^{+61}$K. Their physical properties align with current empirical trends and formation theories of USP planets. Based on the RV measurements, we set 3$\sigma$ upper mass limits of 8$M_{\oplus}$ and 20$M_{\oplus}$, thus confirming the non-stellar, sub-Jovian nature of both transiting objects. More RV measurements will be needed to constrain the planetary masses and mean densities, and the predicted presence of outer planetary companions. These targets extend the small sample of USP planets orbiting around M dwarfs up to 21 members. They are also among the 20 most suitable terrestrial planets for atmospheric characterisation via secondary eclipse with the JWST, according to a widespread emission spectroscopy metric., Comment: Published in A&A, 18 pages, 6 tables, 8 figures

Published
2022
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31. Search for photoproduction of axion-like particles at GlueX

Author

GlueX Collaboration, Adhikari, S., Akondi, C. S., Albrecht, M., Ali, A., Amaryan, M., Asaturyan, A., Austregesilo, A., Baldwin, Z., Barbosa, F., Barlow, J., Barriga, E., Barsotti, R., Beattie, T. D., Berdnikov, V. V., Black, T., Boeglin, W., Briscoe, W. J., Britton, T., Brooks, W. K., Chudakov, E., Cole, S., Cole, P. L., Cortes, O., Crede, V., Dalton, M. M., Deur, A., Dobbs, S., Dolgolenko, A., Dotel, R., Dugger, M., Dzhygadlo, R., Ebersole, D., Egiyan, H., Erbora, T., Ernst, A., Eugenio, P., Fanelli, C., Fegan, S., Fitches, J., Foda, A. M., Furletov, S., Gan, L., Gao, H., Gasparian, A., Gleason, C., Goetzen, K., Goryachev, V. S., Guo, L., Hagen, M., Hakobyan, H., Hamdi, A., Hernandez, J., Hoffman, N. D., Hou, G., Huber, G. M., Hurley, A., Ireland, D. G., Ito, M. M., Jaegle, I., Jarvis, N. S., Jones, R. T., Kakoyan, V., Kalicy, G., Kamel, M., Khachatryan, V., Khatchatryan, M., Kourkoumelis, C., Kuleshov, S., LaDuke, A., Larin, I., Lawrence, D., Lersch, D. I., Li, H., Li, W. B., Liu, B., Livingston, K., Lolos, G. J., Lorenti, L., Luckas, K., Lyubovitskij, V., Mack, D., Mahmood, A., Marukyan, H., Matveev, V., McCaughan, M., McCracken, M., Meyer, C. A., Miskimen, R., Mitchell, R. E., Mizutani, K., Neelamana, V., Nerling, F., Ng, L., Ostrovidov, A. I., Papandreou, Z., Paudel, C., Pauli, P., Pedroni, R., Pentchev, L., Peters, K. J., Reinhold, J., Ritchie, B. G., Ritman, J., Rodriguez, G., Romanov, D., Romero, C., Saldana, K., Salgado, C., Schadmand, S., Schertz, A. M., Schick, A., Schmidt, A., Schumacher, R. A., Schwiening, J., Sharp, P., Shen, X., Shepherd, M. R., Smith, A., Smith, E. S., Sober, D. I., Somov, A., Somov, S., Soto, O., Stevens, J. R., Strakovsky, I. I., Sumner, B., Suresh, K., Tarasov, V. V., Taylor, S., Teymurazyan, A., Thiel, A., Vasileiadis, G., Viducic, T., Whitlatch, T., Wickramaarachchi, N., Williams, M., Yang, Y., Yoon, S., Zarling, J., Zhang, Z., Zhao, Z., Zhou, J., Zhou, X., and Zihlmann, B.

Subjects
High Energy Physics - Experiment, Nuclear Experiment
Abstract

We present a search for axion-like particles, $a$, produced in photon-proton collisions at a center-of-mass energy of approximately 4 GeV, focusing on the scenario where the $a$-gluon coupling is dominant. The search uses $a\to\gamma\gamma$ and $a\to\pi^+\pi^-\pi^0$ decays, and a data sample corresponding to an integrated luminosity of 168 pb$^{-1}$ collected with the GlueX detector. The search for $a\to\gamma\gamma$ decays is performed in the mass range of $180 < m_a < 480$ MeV, while the search for $a\to\pi^+\pi^-\pi^0$ decays explores the $600 < m_a < 720$ MeV region. No evidence for a signal is found, and 90% confidence-level exclusion limits are placed on the $a$-gluon coupling strength. These constraints are the most stringent to date over much of the mass ranges considered., Comment: 8 pages, 4 figures, 2 tables; updated to published version

Published
2021
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33. Measurement of Spin Density Matrix Elements in $\Lambda(1520)$ Photoproduction at 8.2-8.8 GeV

Author

GlueX Collaboration, Adhikari, S., Akondi, C. S., Albrecht, M., Ali, A., Amaryan, M., Asaturyan, A., Austregesilo, A., Baldwin, Z., Barbosa, F., Barlow, J., Barriga, E., Barsotti, R., Beattie, T. D., Berdnikov, V. V., Black, T., Boeglin, W., Briscoe, W. J., Britton, T., Brooks, W. K., Chudakov, E., Cole, S., Cole, P. L., Cortes, O., Crede, V., Dalton, M. M., Daniels, T., Deur, A., Dobbs, S., Dolgolenko, A., Dotel, R., Dugger, M., Dzhygadlo, R., Egiyan, H., Erbora, T., Ernst, A., Eugenio, P., Fanelli, C., Fegan, S., Fitches, J., Foda, A. M., Furletov, S., Gan, L., Gao, H., Gasparian, A., Gleason, C., Goetzen, K., Goryachev, V. S., Guo, L., Hagen, M., Hakobyan, H., Hamdi, A., Hernandez, J., Hoffman, N. D., Hou, G., Huber, G. M., Hurley, A., Ireland, D. G., Ito, M. M., Jaegle, I., Jarvis, N. S., Jones, R. T., Kakoyan, V., Kalicy, G., Kamel, M., Khachatryan, V., Khatchatryan, M., Kourkoumelis, C., Kuleshov, S., LaDuke, A., Larin, I., Lawrence, D., Lersch, D. I., Li, H., Li, W. B., Liu, B., Livingston, K., Lolos, G. J., Luckas, K., Lyubovitskij, V., Mack, D., Mahmood, A., Marukyan, H., Matveev, V., McCaughan, M., McCracken, M., Meyer, C. A., Miskimen, R., Mitchell, R. E., Mizutani, K., Neelamana, V., Nerling, F., Ng, L., Ostrovidov, A. I., Papandreou, Z., Paudel, C., Pauli, P., Pedroni, R., Pentchev, L., Peters, K. J., Reinhold, J., Ritchie, B. G., Ritman, J., Rodriguez, G., Romanov, D., Romero, C., Saldana, K., Salgado, C., Schadmand, S., Schertz, A. M., Schick, A., Schmidt, A., Schumacher, R. A., Schwiening, J., Sharp, P., Shen, X., Shepherd, M. R., Smith, A., Smith, E. S., Sober, D. I., Somov, A., Somov, S., Soto, O., Stevens, J. R., Strakovsky, I. I., Sumner, B., Suresh, K., Tarasov, V. V., Taylor, S., Teymurazyan, A., Thiel, A., Vasileiadis, G., Viducic, T., Whitlatch, T., Wickramaarachchi, N., Williams, M., Yang, Y., Zarling, J., Zhang, Z., Zhao, Z., Zhou, J., Zhou, X., Zhou, Q., Zihlmann, B., Glazier, D. I., and Mathieu, V.

Subjects
Nuclear Experiment, High Energy Physics - Experiment
Abstract

We report on the measurement of spin density matrix elements of the $\Lambda(1520)$ in the photoproduction reaction $\gamma p\rightarrow \Lambda(1520)K^+$, via its subsequent decay to $K^{-}p$. The measurement was performed as part of the GlueX experimental program in Hall D at Jefferson Lab using a linearly polarized photon beam with $E_\gamma =$ 8.2-8.8 GeV. These are the first such measurements in this photon energy range. Results are presented in bins of momentum transfer squared, $-(t-t_\text{0})$. We compare the results with a Reggeon exchange model and determine that natural exchange amplitudes are dominant in $\Lambda(1520)$ photoproduction., Comment: 11 pages, 8 figures, accepted version

Published
2021
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34. Probing extreme environments with the Cherenkov Telescope Array

Author

Boisson, C., Brown, A. M., Burtovoi, A., Cerruti, M., Chernyakova, M., Hassan, T., Lenain, J. -P., Manganaro, M., Romano, P., Sol, H., Tavecchio, F., Vercellone, S., Zampieri, L., Zanin, R., Zech, A., Agudo, I., Batista, R. Alves, Anguner, E. O., Antonelli, L. A., Backes, M., Balazs, C., González, J. Becerra, Bigongiari, C., Bissaldi, E., Bolmont, J., Bordas, P., Bošnjak, Ž., Böttcher, M., Burton, M., Cangemi, F., Caraveo, P., Cardillo, M., Caroff, S., Carosi, A., Casanova, S., Chaty, S., Contreras, J. L., Coelho, J. G., Cotter, G., D'Aì, A., D'Ammando, F., Pino, E. M. de Gouveia Dal, de Martino, D., Delgado, C., della Volpe, D., Djannati-Ataï, A., Anjos, R. C. Dos, Wilhelmi, E. de Oña, Dwarkadas, V., Emery, G., Fedorova, E., Fegan, S., Filipovic, M. D., Galanti, G., Gasparrini, D., Ghirlanda, G., Goldoni, P., Granot, J., Green, J. G., Heller, M., Hnatyk, B., Hnatyk, R., Horan, D., Hovatta, T., Inoue, S., Jamrozy, M., Khélifi, B., Komin, N., Kohri, K., Lamastra, A., La Palombara, N., Lindfors, E., Liodakis, I., Lombardi, S., Longo, F., Lucarelli, F., Luque-Escamilla, P. L., Marti, J., Martinez, M., Mazin, D., Mbarubucyeye, J. D., Menchiari, S., Mohrmann, L., Montaruli, T., Olaizola, A. Moralejo, Morcuende, D., Morlino, G., Morselli, A., Mundell, C. G., Murach, T., Nagai, A., Nayerhoda, A., Niemiec, J., Nikolajuk, M., Olmi, B., Orienti, M., Paredes, J. M., Pareschi, G., Pe'er, A., Pühlhofer, G., Punch, M., Reimer, O., Ribó, M., Rieger, F., Rodriguez, G., Rodriguez, J., Romeo, G., Roncadelli, M., Rowell, G., Rudak, B., Sadeh, I., Greus, F. Salesa, Sawangwit, U., Schüssler, F., Sergijenko, O., Shellard, R. C., Saturni, F. G., Stamerra, A., Stolarczyk, Th., Tagliaferri, G., Testa, V., Tibaldo, L., Ventura, S., Viana, A., Vink, J., Vitale, V., Vorobiov, S., Wierzcholska, A., Zacharias, M., and Zavrtanik, D.

Subjects
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract

The physics of the non-thermal Universe provides information on the acceleration mechanisms in extreme environments, such as black holes and relativistic jets, neutron stars, supernovae or clusters of galaxies. In the presence of magnetic fields, particles can be accelerated towards relativistic energies. As a consequence, radiation along the entire electromagnetic spectrum can be observed, and extreme environments are also the most likely sources of multi-messenger emission. The most energetic part of the electromagnetic spectrum corresponds to the very-high-energy (VHE, E>100 GeV) gamma-ray regime, which can be extensively studied with ground based Imaging Atmospheric Cherenkov Telescopes (IACTs). The results obtained by the current generation of IACTs, such as H.E.S.S., MAGIC, and VERITAS, demonstrate the crucial importance of the VHE band in understanding the non-thermal emission of extreme environments in our Universe. In some objects, the energy output in gamma rays can even outshine the rest of the broadband spectrum. The Cherenkov Telescope Array (CTA) is the next generation of IACTs, which, with cutting edge technology and a strategic configuration of ~100 telescopes distributed in two observing sites, in the northern and southern hemispheres, will reach better sensitivity, angular and energy resolution, and broader energy coverage than currently operational IACTs. With CTA we can probe the most extreme environments and considerably boost our knowledge of the non-thermal Universe., Comment: Submitted as input to ASTRONET Science Vision and Infrastructure roadmap on behalf of the CTA consortium

Published
2021

35. Multi-messenger and transient astrophysics with the Cherenkov Telescope Array

Author

Bošnjak, Ž., Brown, A. M., Carosi, A., Chernyakova, M., Cristofari, P., Longo, F., López-Oramas, A., Santander, M., Satalecka, K., Schüssler, F., Sergijenko, O., Stamerra, A., Agudo, I., Batista, R. Alves, Amato, E., Anguner, E. O., Antonelli, L. A., Backes, M., Balazs, Csaba, Baroncelli, L., Tjus, J. Becker, Bigongiari, C., Bissaldi, E., Boisson, C., Bolmont, J., Böttcher, M., Bordas, P., Braiding, C., Bregeon, J., Bucciantini, N., Bulgarelli, A., Burton, M., Cangemi, F., Caraveo, P., Cardillo, M., Caroff, S., Casanova, S., Chaty, S., Coelho, J. G., Cotter, G., D'Aì, A., D'Ammando, F., Pino, E. M. de Gouveia Dal, della Volpe, D., de Martino, D., Di Girolamo, T., Di Piano, A., Djannati-Ataï, A., Dwarkadas, V., Wilhelmi, E. de Ona, Anjos, R. C. Dos, Emery, G., Fedorova, E., Fegan, S., Fiasson, A., Fioretti, V., Filipovic, M. D., Gaggero, D., Galanti, G., Gasparrini, D., Ghirlanda, G., Goldoni, P., Granot, J., Green, J. G., Heller, M., Hnatyk, B., Hnatyk, R., Horan, D., Hovatta, T., Inoue, S., Jamrozy, M., Kantzas, D., Khélifi, B., Komin, N., Lamastra, A., La Palombara, N., Lenain, J. P., Lindfors, E., Liodakis, I., Lombardi, S., Lucarelli, F., Luque-Escamilla, P. L., Majumdar, P., Marcowith, A., Markoff, S., Marti, J., Martinez, M., Mazin, D., McKeague, S., Mereghetti, S., Mestre, E., Montaruli, T., Morlino, G., Morselli, A., Mundell, C., Murach, T., Nava, L., Nayerhoda, A., Nicastro, L., Niemiec, J., Nikolajuk, M., Olmi, B., Ong, R., Orienti, M., Osborne, J. P., Paredes, Josep M., Pareschi, G., Parmiggiani, N., Patricelli, B., Pe'er, A., Piano, G., Pühlhofer, G., Punch, M., Reimer, O., Ribó, M., Rodriguez, G., Rodriguez, J., Romano, P., Romeo, G., Roncadelli, M., Rowell, G., Rudak, B., Sadeh, I., Greus, F. Salesa, Saturni, F. G., Sawangwit, U., Seglar-Arroyo, M., Shellard, R. C., Sol, H., Starling, R., Stolarczyk, T., Tagliaferri, G., Tavecchio, F., Tibaldo, L., Testa, V., Vercellone, S., Viana, A., Vink, J., Vitale, V., Vergani, S. D., Vorobiov, S., Wierzcholska, A., Yang, L., Zavrtanik, D., and Zhdanov, V.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

The discovery of gravitational waves, high-energy neutrinos or the very-high-energy counterpart of gamma-ray bursts has revolutionized the high-energy and transient astrophysics community. The development of new instruments and analysis techniques will allow the discovery and/or follow-up of new transient sources. We describe the prospects for the Cherenkov Telescope Array (CTA), the next-generation ground-based gamma-ray observatory, for multi-messenger and transient astrophysics in the decade ahead. CTA will explore the most extreme environments via very-high-energy observations of compact objects, stellar collapse events, mergers and cosmic-ray accelerators., Comment: Submitted to ASTRONET roadmap on behalf of the CTA consortium

Published
2021

36. Origin and role of relativistic cosmic particles

Author

Araudo, A., Morlino, G., Olmi, B., Acero, F., Agudo, I., Adam, R., Batista, R. Alves, Amato, E., Anguner, E. O., Antonelli, L. A., Ascasibar, Y., Balazs, C., Tjus, J. Becker, Bigongiari, C., Bissaldi, E., Bolmont, J., Boisson, C., Bordas, P., Bošnjak, Ž., Brown, A. M., Burton, M., Bucciantini, N., Cangemi, F., Caraveo, P., Cardillo, M., Caroff, S., Casanova, S., Chaty, S., Chernyakova, M., Coelho, J. G., Conte, F., Cotter, G., Crestan, S., D'Aì, A., Pino, E. M. de Gouveia Dal, Delgado, C., della Volpe, D., de Martino, D., Djannati-Ataï, A., Anjos, R. C. Dos, Dwarkadas, V., Emery, G., Fedorova, E., Filipovic, M. D., Fornieri, O., Galanti, G., Gasparrini, D., Ghirlanda, G., Giuliani, A., Goldoni, P., Granot, J., Grasso, D., Wilhelmi, E. de Oña, Khélifi, B., Heller, M., Horan, D., Hnatyk, B., Hnatyk, R., Inoue, S., Jamrozy, M., Komin, N., Lamastra, A., La Palombara, N., Lenain, J. -P., Liodakis, I., Lombardi, S., Longo, F., Lòpez-Oramas, A., Lòpez-Moya, M., Lucarelli, F., Luque-Escamilla, P. L., Majumdar, P., Marcowith, A., Martì, J., Martinez, M., Mazin, D., Menchiari, S., Mohrmann, L., Montaruli, T., Morselli, A., Mundell, C. G., Murach, T., Nagai, A., Nayerhoda, A., Niemiec, J., Nikolajuk, M., Ong, R. A., Paredes, J. M., Pareschi, G., Pohl, M., Pühlhofer, G., Punch, M., Reimer, O., Ribò, M., Rieger, F., Rodriguez, G., Rowell, G., Romano, P., Roncadelli, M., Romeo, G., Rudak, B., Greus, F. Salesa, Saturni, F. G., Sawangwit, U., Schüssler, F., Sergijenko, O., Sol, H., Stamerra, A., Stolarczyk, T., Tagliaferri, G., Tavecchio, F., Testa, V., Tibaldo, L., Viana, A., Vercellone, S., Ventura, S., Vink, J., Vorobiov, S., Vitale, V., Sadeh, I., Sharma, P., Shellard, R. C., Suomijärvi, T., and Wierzcholska, A.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

This white paper briefly summarizes the importance of the study of relativistic cosmic rays, both as a constituent of our Universe, and through their impact on stellar and galactic evolution. The focus is on what can be learned over the coming decade through ground-based gamma-ray observations over the 20 GeV to 300 TeV range. The majority of the material is drawn directly from "Science with the Cherenkov Telescope Array", which describes the overall science case for CTA. We request that authors wishing to cite results contained in this white paper cite the original work., Comment: Submitted as input to ASTRONET Science Vision and Infrastructure roadmap on behalf of the CTA consortium. arXiv admin note: text overlap with arXiv:1709.07997

Published
2021

37. Development and evaluation of the use of a virtual health filter survey in a private primary education system in Baja California Mexico during the SARS-CoV-2 contingency (COVID-19)

Author

Romo-Cárdenas, G. S., Cosío-León, M. A., Avilés-Rodriguez, G. J., Isiodoro-Carballo, N., Zuñiga-Violante, E., Sánchez-López, J. dD., and Nieto-Hipólito, J. I.

Subjects
Computer Science - Computers and Society, 03B05, J.1, J.4, J.3
Abstract

This work reports on the design, implementation and evaluation of a survey used as a remote sanitary filter, which was applied in the Adventist Educational System of Baja California. During the SARS-CoV-2 sanitary contingency. This with the intention of acquiring information safely and in real time. Allowing to safeguard the integrity of the educational community as a whole. Accessible and easily distributed digital resources were used in order to meet the necessary requirements of distribution, acquisition and management of the information. These were adapted to the previously established communication dynamic of the educational system. The use of the survey as a sanitary filter allowed to acquire relevant health information from the student community and facilitated decision-making regarding class attendance by their tutors.These in consideration to the conditions established by educational and health authorities. Despite the short time during the design and implementation, the communication of the educational system allowed the effective distribution, application and monitoring of the digital survey. Similar strategies can be used in the follow-up during the reactivation after lockdown and to analyze social components that may be involved in these scenarios, Comment: Spanish, 9 pages, 3 tables, 3 figures

Published
2020

38. Effect of Self-Lubricating Carbon Materials on the Tribological Performance of Ultra-High-Molecular-Weight Polyethylene

Author

Camacho, N., Escobedo-Rodríguez, J. D., Alvarado-Orozco, J. M., and Mondragón-Rodríguez, G. C.

Subjects
Condensed Matter - Materials Science
Abstract

Ultra-high-molecular-weight polyethylene (UHMWPE) has been the gold standard for total knee replacements. Due to the knee's natural movements, UHMWPE wear debris production is inevitable. The debris, at the micron and submicron level, results in the joint's mechanical instability, reduced mobility, increased pain, and implant loosening. Wear debris production has been linked to UHMWPE mechanical properties; therefore, improvements to increase the UHMWPE mechanical properties will impact the component's longevity. Here, TiC coating and multiwalled carbon nanotubes (MWCNTs) were used to decrease the UHMWPE wear. After 400,000 cycles, the UHMWPE-MWCNT diminishes the mass loss compared to UHMWPE, and the combination with TiC decreased the material loss by ~ 43.7 % compared to the reference pair. Cold-flow and burnishing were the predominant wear modes., Comment: 9 p\'aginas

Published
2020

39. Measurement of beam asymmetry for $\pi^-\Delta^{++}$ photoproduction on the proton at $E_\gamma$=8.5 GeV

Author

GlueX Collaboration, Adhikari, S., Akondi, C. S., Ali, A., Amaryan, M., Asaturyan, A., Austregesilo, A., Baldwin, Z., Barbosa, F., Barlow, J., Barriga, E., Barsotti, R., Beattie, T. D., Berdnikov, V. V., Black, T., Boeglin, W., Briscoe, W. J., Britton, T., Brooks, W. K., Cannon, B. E., Chudakov, E., Cole, S., Cortes, O., Crede, V., Dalton, M. M., Daniels, T., Deur, A., Dobbs, S., Dolgolenko, A., Dotel, R., Dugger, M., Dzhygadlo, R., Egiyan, H., Erbora, T., Ernst, A., Eugenio, P., Fanelli, C., Fegan, S., Fitches, J., Foda, A. M., Furletov, S., Gan, L., Gao, H., Gasparian, A., Gleason, C., Goetzen, K., Goryachev, V. S., Guo, L., Hakobyan, H., Hamdi, A., Huber, G. M., Hurley, A., Ireland, D. G., Ito, M. M., Jaegle, I., Jarvis, N. S., Jones, R. T., Kakoyan, V., Kalicy, G., Kamel, M., Khachatryan, V., Khatchatryan, M., Kourkoumelis, C., Kuleshov, S., LaDuke, A., Larin, I., Lawrence, D., Lersch, D. I., Li, H., Li, W. B., Liu, B., Livingston, K., Lolos, G. J., Luckas, K., Lyubovitskij, V., Mack, D., Marukyan, H., Matveev, V., McCaughan, M., McCracken, M., McGinley, W., Meyer, C. A., Miskimen, R., Mitchell, R. E., Mizutani, K., Neelamana, V., Nerling, F., Ng, L., Ostrovidov, A. I., Papandreou, Z., Paudel, C., Pauli, P., Pedroni, R., Pentchev, L., Peters, K. J., Phelps, W., Pooser, E., Reinhold, J., Ritchie, B. G., Ritman, J., Rodriguez, G., Romanov, D., Romero, C., Salgado, C., Schadmand, S., Schertz, A. M., Schick, A., Schumacher, R. A., Schwiening, J., Shen, X., Shepherd, M. R., Smith, A., Smith, E. S., Sober, D. I., Somov, A., Somov, S., Soto, O., Stevens, J. R., Strakovsky, I. I., Sumner, B., Suresh, K., Tarasov, V. V., Taylor, S., Teymurazyan, A., Thiel, A., Vasileiadis, G., Whitlatch, T., Wickramaarachchi, N., Williams, M., Yang, Y., Zarling, J., Zhang, Z., Zhao, Z., Zhou, J., Zhou, Q., Zhou, X., and Zihlmann, B.

Subjects
Nuclear Experiment, High Energy Physics - Experiment
Abstract

We report a measurement of the $\pi^-$ photoproduction beam asymmetry for the reaction $\vec{\gamma} p \rightarrow \pi^- \Delta^{++}$ using data from the GlueX experiment in the photon beam energy range 8.2--8.8 GeV. The asymmetry $\Sigma$ is measured as a function of four-momentum transfer $t$ to the $\Delta^{++}$ and compared to phenomenological models. We find that $\Sigma$ varies as a function of $t$: negative at smaller values and positive at higher values of $|t|$. The reaction can be described theoretically by $t$-channel particle exchange requiring pseudoscalar, vector, and tensor intermediaries. In particular, this reaction requires charge exchange, allowing us to probe pion exchange and the significance of higher-order corrections to one-pion exchange at low momentum transfer. Constraining production mechanisms of conventional mesons may aid in the search for and study of unconventional mesons. This is the first measurement of the process at this energy., Comment: 7 pages, 5 figures

Published
2020
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40. LabOSat as a versatile payload for small satellites: first 100days in LEO orbit

Author

Sanca, G. A., Barella, M., Marlasca, F. Gomez, Rodríguez, G., Martelliti, D., Patrone, L., Levy, P., and Golmar, F.

Subjects
Physics - Instrumentation and Detectors, Physics - Applied Physics, Physics - Space Physics
Abstract

In this work the first results obtained by LabOSat-01 platform are presented. This platform was designed for testing custom devices on board of small satellites. Two LabOSat-01 type boards were launched and placed into Low Earth Orbit (LEO) on May 30, 2016. We present here an analysis of data collected by one of these boards during the first days of mission. Total Ionization Dose results are compared with data acquired by LabOSat-01`s predecessor board, MeMOSat-01, launched in 2014.

Published
2020

41. Associations between food portion sizes, insulin resistance, VO2 max and metabolic syndrome in European adolescents: The HELENA study

Author

Coordinator, Moreno, L.A., Core Group members, Gottrand, F., De Henauw, S., González-Gross, M., Gilbert, C., Steering Committee, Kafatos, A., Libersa, C., Castelló, S., Kersting, M., Sjöstrom, M., Molnár, D., Dallongeville, J., Hall, G., Maes, L., Scalfi, L., Project Manager, Meléndez, P., Casajús, J.A., Fleta, J., Rodríguez, G., Tomás, C., Mesana, M.I., Vicente-Rodríguez, G., Villarroya, A., Gil, C.M., Ara, I., Alvira, J.F., Bueno, G., Bueno, O., León, J.F., Garagorri, J.Ma, Labayen, I., Iglesia, I., Bel, S., Gracia Marco, L.A., Mouratidou, T., Santaliestra-Pasías, A., González-Gil, E., De Miguel-Etayo, P., Miguel-Berges, M., Iguacel, I., Rupérez, A., Marcos, A., Wärnberg, J., Nova, E., Gómez, S., Díaz, L.E., Romeo, J., Veses, A., Zapatera, B., Pozo, T., Martínez, D., Beghin, L., Iliescu, C., Von Berlepsch, J., Sichert-Hellert, W., Koeppen, E., Molnar, D., Erhardt, E., Csernus, K., Török, K., Bokor, S., Angster, M., Nagy, E.ö, Kovács, O., Répasi, J., Codrington, C., Plada, M., Papadaki, A., Sarri, K., Viskadourou, A., Hatzis, C., Kiriakakis, M., Tsibinos, G., Vardavas, C., Sbokos, M., Protoyeraki, E., Fasoulaki, M., Stehle, P., Pietrzik, K., Breidenassel, C., Spinneker, A., Al-Tahan, J., Segoviano, M., Berchtold, A., Bierschbach, C., Blatzheim, E., Schuch, A., Pickert, P., Castillo, M.J., Gutiérrez, Á., Ortega, F.B., Ruiz, J.R., Artero, E.G., España, V., Jiménez-Pavón, D., Chillón, P., Sánchez-Muñoz, C., Cuenca, M., former INRAN, Arcella, D., Azzini, E., Barrison, E., Bevilacqua, N., Buonocore, P., Catasta, G., Censi, L., Ciarapica, D., D'Acapito, P., Ferrari, M., Galfo, M., Le Donne, C., Leclercq, C., Maiani, G., Mauro, B., Mistura, L., Pasquali, A., Piccinelli, R., Polito, A., Roccaldo, R., Spada, R., Sette, S., Zaccaria, M., Vitaglione, P., Montagnese, C., De Bourdeaudhuij, I., De Vriendt, T., Matthys, C., Vereecken, C., de Maeyer, M., Ottevaere, C., Huybrechts, I., Widhalm, K., Phillipp, K., Dietrich, S., Kubelka, B., Boriss-Riedl, M., Manios, Y., Grammatikaki, E., Bouloubasi, Z., Cook, T.L., Eleutheriou, S., Consta, O., Moschonis, G., Katsaroli, I., Kraniou, G., Papoutsou, S., Keke, D., Petraki, I., Bellou, E., Tanagra, S., Kallianoti, K., Argyropoulou, D., Tsikrika, S., Karaiskos, C., Meirhaeghe, A., Hagströmer, M., Wennlöf, A.H., Hallström, L., Patterson, E., Kwak, L., Rizzo, N., Sánchez-Molero, J., Picó, E., Navarro, M., Viadel, B., Carreres, J.E., Merino, G., Sanjuán, R., Lorente, M., Sánchez, M.J., Thoma-IRs, S., Allchurch, E., Burgess, P., Astrom, A., Sverkén, A., Broberg, A., Masson, A., Lehoux, C., Brabant, P., Pate, P., Fontaine, L., Sebok, A., Kuti, T., Hegyi, A., Maldonado, C., Llorente, A., García, E., von Fircks, H., Hallberg, M.L., Messerer, M., Larsson, M., Fredriksson, H., Adamsson, V., Börjesson, I., Fernández, L., Smillie, L., Wills, J., Pedrero-Chamizo, R., Meléndez, A., Valtueña, J., Albers, U., Benito, P.J., Gómez Lorente, J.J., Cañada, D., Urzanqui, A., Torres, R.M., Navarro, P., Flieh, S.M., Miguel-Berges, M.L., Gonzalez-Gross, M., Gesteiro, E., Abbeddou, S., and González-Gil, E.M.

Published
2022
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43. Adult T-cell leukemia/lymphoma in HTLV-1 non-endemic regions

Author

Calderón, E., Rodríguez-Iglesias, M., Montiel, N., Trujillo, T., Viciana, I., Cabezas, T., Lozano, A., Fernández-Fuertes, E., Fernández, J.M., García, F., Benito, R., Algarate, S., Ducons, M., Roc, L., Cifuentes, C., Fernández-Baca, V., Fernández-Montero, J.V, Maciá, MD., Hernández-Betancor, A., Martín, A.M., Pena, M.J., Hernández, M., López-Lirola, A.M., Gómez-Sirvent, J.L., Copado, R., Cano, M.E., Rojo, S., Eirós, J.M., Rodríguez, M., Gómez-Hernando, C., González-Praetorius, A., Rando, A., Force, L., Miró, E., Cebollero, A., Delgado, J.F., Rodríguez, G., Fernández-Pereira, L., Aguilera, A., Pereira, S., García, J., Trigo, M., Diz, J., García-Campello, M., Cortizo, S., Pérez, S., Morano, L., Reina, G., Arazamendi, M., Salicio, Y., Ugalde, E., Nieto, M.C., Liendo, P., Goikoetxea, A.J., Ocete, M.D., Ramos, J.M., Escribano, I., Sauleda, S., Pirón, M., González, R., Richart, A., Barea, L., Jiménez, A., Blanco, L., Navarro, L., Ayerdi, O., Baza, B., Rodriguez, C., del Romero, J., Galar, A., Aldamiz, T., Valeiro, M., Pérez, L., Rodríguez-Avial, I., Martín-Carbonero, L., Fernández-Ruiz, M., Parra, P., Redondo, N., Ruiz-Merlo, T., Pozuelo, M.J., Barreiro, P., Treviño, A., Corral, O., Soriano, V., Pintos, I., Moreno-Torres, V., Carrizo, P., Huertas, A., Vargas-Núñez, J.A., de Mendoza, C., de Mendoza, Carmen, Rando, Ariadna, Miró, Elisenda, Pena, María José, Rodríguez-Avial, Iciar, Ortega, Diego, González-Praetorius, Alejandro, Reina, Gabriel, Pintos, Ilduara, Pozuelo, María José, and Soriano, Vicente

Published
2023
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49. The multi-outburst activity of the magnetar in Westerlund I

Author

Borghese, A., Rea, N., Turolla, R., Pons, J. A., Esposito, P., Zelati, F. Coti, Savchenko, V., Bozzo, E., Perna, R., Zane, S., Mereghetti, S., Campana, S., Mignani, R. P., Bachetti, M., Rodriguez, G., Pintore, F., Tiengo, A., Gotz, D., Israel, G. L., and Stella, L.

Subjects
Astrophysics - High Energy Astrophysical Phenomena
Abstract

After two major outbursts in 2006 and 2011, on 2017 May 16 the magnetar CXOU J164710.2-455216, hosted within the massive star cluster Westerlund I, emitted a short (20 ms) burst, which marked the onset of a new active phase. We started a long-term monitoring campaign with Swift (45 observations), Chandra (5 observations) and NuSTAR (4 observations) from the activation until 2018 April. During the campaign, Swift BAT registered the occurrence of multiple bursts, accompanied by two other enhancements of the X-ray persistent flux. The long time span covered by our observations allowed us to study the spectral as well as the timing evolution of the source. After 11 months since the 2017 May outburst onset, the observed flux was about 15 times higher than its historical minimum level and a factor of 3 higher than the level reached after the 2006 outburst. This suggests that the crust has not fully relaxed to the quiescent level, or that the source quiescent level has changed following the multiple outburst activities in the past 10 years or so. This is another case of multiple outbursts from the same source on a yearly time scale, a somehow recently discovered behaviour in magnetars., Comment: Accepted for publication in MNRAS, 14 pages, 7 figures

Published
2019
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50. A Robot for Facade Cleaning Based on a Cartesian Configuration: Kinematic Analysis and Prototype Construction

Author

García-Rodríguez, G. M., Castillo-Castañeda, E., Ceccarelli, Marco, Series Editor, Agrawal, Sunil K., Advisory Editor, Corves, Burkhard, Advisory Editor, Glazunov, Victor, Advisory Editor, Hernández, Alfonso, Advisory Editor, Huang, Tian, Advisory Editor, Jauregui Correa, Juan Carlos, Advisory Editor, Takeda, Yukio, Advisory Editor, Müller, Andreas, editor, and Brandstötter, Mathias, editor

Published
2022
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