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673 results on '"Raffelt G"'

351. New solar axion search using the CERN Axion Solar Telescope with He-4 filling

Author: Arik, M., Aune, S., Barth, K., Belov, A., Braeuninger, H., Bremer, J., Burwitz, V., Cantatore, G., Carmona, J. M., Cetin, S. A., Collar, J. I., Da Riva, E., Dafni, T., Davenport, M., Dermenev, A., Eleftheriadis, C., Elias, N., Fanourakis, G., Ferrer-Ribas, E., Galan, J., Garcia, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Georgiopoulou, E., Giomataris, I., Gninenko, S., Marzoa, M. Gomez, Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakovcic, K., Karuza, M., Kavuk, M., Krcmar, M., Kuster, M., Lakic, B., Laurent, J. M., Liolios, A., Ljubicic, A., Luzon, G., Neff, S., Niinikoski, T., Nordt, A., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Rodriguez, A., Rosu, M., Ruz, J., Savvidis, I., Shilon, I., Solanki, S. K., Stewart, L., Tomas, A., Vafeiadis, T., Villar, J., Vogel, J. K., Yildiz, S. C., Zioutas, K., and CAST Collaboration
Abstract: The CERN Axion Solar Telescope (CAST) searches for a -> gamma conversion in the 9 T magnetic field of a refurbished LHC test magnet that can be directed toward the Sun. Two parallel magnet bores can be filled with helium of adjustable pressure to match the x-ray refractive mass m(gamma) to the axion search mass m(a). After the vacuum phase (2003-2004), which is optimal for m(a) less than or similar to 0.02 eV, we used He-4 in 2005-2007 to cover the mass range of 0.02-0.39 eV and He-3 in 2009-2011 to scan from 0.39 to 1.17 eV. After improving the detectors and shielding, we returned to He-4 in 2012 to investigate a narrow m(a) range around 0.2 eV ("candidate setting" of our earlier search) and 0.39-0.42 eV, the upper axion mass range reachable with He-4, to "cross the axion line" for the KSVZ model. We have improved the limit on the axion-photon coupling to g(a gamma) < 1.47 x 10(-10) GeV-1 (95% C.L.), depending on the pressure settings. Since 2013, we have returned to the vacuum and aim for a significant increase in sensitivity.

352. Decoherence in supernova neutrino transformations suppressed by deleptonization

Author: Esteban-Pretel, A., Pastor, S., Tomas, R., Raffelt, G. G., and Sigl, G.
Subjects: 7. Clean energy, 3. Good health
Abstract: Neutrino Oscillation Workshop, Otranto, Italy, 6 Sep 2008 - 13 Sep 2008; Nuclear physics / B / Proceedings supplements 188, 3 (2009). doi:10.1016/j.nuclphysbps.2009.02.028, In the dense-neutrino region at 50–400 km above the neutrino sphere in a supernova, neutrino-neutrino interactions cause large flavor transformations. We study when the multi-angle nature of the neutrino trajectories leads to flavor decoherence between different angular modes. We consider a two-flavor mixing scenario between ν e and another flavor ν x and assume the usual hierarchy F ν e > F ν ¯ e > F ν x = F ν ¯ x for the number fluxes, Published by Elsevier, Amsterdam

353. The International Axion Observatory IAXO. Letter of Intent to the CERN SPS committee

Author: Irastorza, Igor, Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, G., Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Dael, A., Dafni, T., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Dobrich, B. D., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer-Ribas, E., Galan, J., Garcia, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gomez, H., Gonzalez-Diaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Isern, J., Imai, K., Jakobsen, A. C., Jaeckel, J., Jakovcic, K., Kaminski, J., Kawasaki, M., Karuza, M., Krcmar, M., Kousouris, K., Krieger, C., Lakic, B., Limousin, O., Lindner, A., Liolios, A., Luzon, G., Matsuki, S., Muratova, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Ten Kate, H., Tomas, A., Troitsky, S., Vafeiadis, T., Bibber, K., Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., William Wester, Yildiz, S. C., and Zioutas, K.
Subjects: Detectors and Experimental Techniques
Abstract: This Letter of Intent describes IAXO, the International Axion Observatory, a proposed 4th generation axion helioscope. As its primary physics goal, IAXO will look for axions or axion-like particles (ALPs) originating in the Sun via the Primakoff conversion of the solar plasma photons. In terms of signal to background ratio, IAXO will be about 4-5 orders of magnitude more sensitive than CAST, which means that this instrument will reach sensitivity to axion-photon couplings down to a few $\times 10^{-12}$ GeV$^{-1}$. IAXO has the potential for the discovery of axions and other ALPs, since it will deeply enter into unexplored parameter space. At the very least it will firmly exclude a large region of this space of high cosmological and astrophysical relevance. In particular it will probe a large fraction of the high mass part (1 meV to 1 eV) of the QCD axion allowed window. Additional physics cases for IAXO include the possibility of detecting solar axions produced by mechanisms mediated by the axion-electron coupling $g_{ae}$ with sensitivity $-$for the first time$-$ to values of $g_{ae}$ not previously excluded by astrophysics. IAXO follows the conceptual layout of an enhanced axion helioscope, with a purpose-built 8-coils toroidal superconducting magnet. All the eight 60-cm diameter magnet bores are equipped with focusing x-ray optics, able to focus the signal photons into $\sim$0.2 cm$^2$ spots that are imaged by ultra-low-background Micromegas x-ray detectors. The magnet is built into a structure with elevation and azimuth drives the will allow for solar tracking for $\sim$12 h each day. All the enabling technologies exists, there is no need for development. All the needed know-how is present in the proponent groups. Potential additional physics cases for IAXO to be developed in the future are the search of axionic dark radiation, relic cold dark matter axions or the realization of microwave light-shining-through wall setups, as well as the search of more specific models of weakly interacting sub-eV particles (WISPs) at the low energy frontier of particle physics. IAXO has the potential to serve as a multi-purpose facility for generic axion and ALP research in the next decade.

354. Search for Solar Axions by the CERN Axion Solar Telescope with He-3 Buffer Gas: Closing the Hot Dark Matter Gap

Author: Arik, M., Aune, S., Barth, K., Belov, A., Borghi, S., Braeuninger, H., Cantatore, G., Carmona, J. M., Cetin, S. A., Collar, J. I., Da Riva, E., Dafni, T., Davenport, M., Eleftheriadis, C., Elias, N., Fanourakis, G., Ferrer-Ribas, E., Friedrich, P., Galan, J., Garcia, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Georgiopoulou, E., Giomataris, I., Gninenko, S., Gomez, H., Marzoa, M. Gomez, Gruber, E., Guthoerl, T., Hartmann, R., Hauf, S., Haug, F., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakovcic, K., Karuza, M., Koenigsmann, K., Kotthaus, R., Krcmar, M., Kuster, M., Lakic, B., Lang, P. M., Laurent, J. M., Liolios, A., Ljubicic, A., Luzon, G., Neff, S., Niinikoski, T., Nordt, A., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Riege, H., Rodriguez, A., Rosu, M., Ruz, J., Savvidis, I., Shilon, I., Silva, P. S., Solanki, S. K., Stewart, L., Tomas, A., Tsagri, M., Van Bibber, K., Vafeiadis, T., Villar, J., Vogel, J. K., and CAST Collaboration
Subjects: Physics::Instrumentation and Detectors, Astrophysics::Earth and Planetary Astrophysics
Abstract: The CERN Axion Solar Telescope has finished its search for solar axions with He-3 buffer gas, covering the search range 0.64 eV less than or similar to ma less than or similar to 1.17 eV. This closes the gap to the cosmological hot dark matter limit and actually overlaps with it. From the absence of excess x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g(a gamma) less than or similar to 3.3 x 10(-10) GeV-1 at 95% C.L., with the exact value depending on the pressure setting. Future direct solar axion searches will focus on increasing the sensitivity to smaller values of g(a gamma), for example by the currently discussed next generation helioscope International AXion Observatory.

355. Solar axion search with the CAST experiment

Author: Borghi, S., Arik, E., Aune, S., Autiero, D., Barth, K., Belov, A., Beltrán, B., Bourlis, G., Boydag, F. S., Bräuninger, H., Cantatore, G., Carmona, J. M., Cebrián, S., Cetin, S. A., Collar, J. I., Dafni, T., Davenport, M., Di Lella, L., Dogan, O. B., Eleftheriadis, C., Elias, N., Fanourakis, G., Ferrer-Ribas, E., Fischer, H., Franz, J., Galán, J., Gazis, E., Geralis, T., Giomataris, I., Gninenko, S., Gómez, H., Hasinoff, M., Heinsius, F. H., Hikmet, I., Hoffmann, D. H. H., Irastorza, I. G., Jacoby, J., Jakovčić, K., Kang, D., Karageorgopoulou, T., Karuza, M., Königsmann, K., Kotthaus, R., Krčmar, M., Kousouris, K., Kuster, M., Lakić, B., Lasseur, C., Liolios, A., Ljubičić, A., Lozza, V., Lutz, G., Luzón, G., Miller, D., Morales, A., Morales, J., Niinikoski, T., Nordt, A., Ortiz, A., Papaevangelou, T., Michael Pivovaroff, Placci, A., Raiteri, G., Raffelt, G., Riege, H., Rodríguez, A., Ruz, J., Savvidis, I., Semertzidis, Y., Serpico, P., Solanki, S. K., Soufli, R., Stewart, L., Tsagri, M., Bibber, K., Villar, J., Vogel, J., Walckiers, L., and Zioutas, K.
Subjects: High Energy Physics::Theory, Astrophysics and Astronomy, Physics::Instrumentation and Detectors, High Energy Physics::Phenomenology
Abstract: The CAST (CERN Axion Solar Telescope) experiment is searching for solar axions by their conversion into photons inside the magnet pipe of a LHC prototype dipole. In the phase II, CAST is operating with a buffer gas inside the magnet bore apertures in order to extent the sensitivity of the experiment to larger axion masses. Preliminary results from the analysis of this second phase with He inside the magnet pipes excludes axions down to $g_{aγ}$ < 2.2 · $10^{−10}GeV^{−1}$ at 95% C.L. for 0.02 eV < $m_{\alpha}$ < 0.39 eV. The data analysis has resulted in the most restrictive experimental limit on the coupling constant of axions to photons and for the first time experimental result has entered the theory motivated axion parameter space. At the beginning of 2008, data started to be taken with He in the magnet pipes in order to extend the sensitivity to axion masses up to 1.2 eV.

356. Review of Particle Physics: Particle data group

Author: Hagiwara, K., Hikasa, K., Nakamura, K., Tanabashi, M., Aguilar-Benitez, M., Amsler, C., Barnett, R. M., Burchat, P. R., Carone, C. D., Caso, C., Conforto, G., Dahl, O., Doser, M., Eidelman, S., Feng, J. L., Gibbons, L., Goodman, M., Grab, C., Groom, D. E., Gurtu, A., Hayes, K. G., Hernández-Rey, J. J., Honscheid, K., Kolda, C., Mangano, M. L., Manley, D. M., Manohar, A. V., March-Russell, J., Masoni, A., Miquel, R., Mönig, K., Murayama, H., Navas, S., Olive, K. A., Pape, L., Patrignani, C., Piepke, A., Roos, M., Terning, J., Törnqvist, N. A., Trippe, T. G., Vogel, P., Wohl, C. G., Workman, R. L., Yao, W. -M, Armstrong, B., Gee, P. S., Lugovsky, K. S., Lugovsky, S. B., Lugovsky, V. S., Artuso, M., Asner, D., Babu, K. S., Barberio, E., Battaglia, M., Bichsel, H., Biebel, O., Bloch, P., Cahn, R. N., Cattai, A., Chivukula, R. S., Cousins, R. D., Cowan, G., Damour, T., Desler, K., Donahue, R. J., Edwards, D. A., Elvira, V. D., Erler, J., Ezhela, V. V., Fassó, A., Fetscher, W., Fields, B. D., Foster, B., Froidevaux, D., Fukugita, M., Gaisser, T. K., Garren, L., Gerber, H. J., Gilman, F. J., Haber, H. E., Hagmann, C., Hewett, J., Hinchliffe, I., Hogan, C. J., Höhler, G., Igo-Kemenes, P., Jackson, J. D., Johnson, K. F., Karlen, D., Kayser, B., Klein, S. R., Kleinknecht, K., Knowles, I. G., Kreitz, P., Kuyanov, Y. V., Landua, R., Langacker, P., Littenberg, L., Martin, A. D., Nakada, T., Narain, M., Nason, P., Peacock, J. A., Quinn, H. R., Raby, S., Raffelt, G., Razuvaev, E. A., Renk, B., Rolandi, L., Ronan, M. T., Rosenberg, L. J., Sachrajda, C. T., Sanda, A. I., Subir Sarkar, Schmitt, M., Schneider, O., Scott, D., Seligman, W. G., Shaevitz, M. H., Sjöstrand, T., Smoot, G. F., Spanier, S., Spieler, H., Spooner, N. J. C., Srednicki, M., Stahl, A., Stanev, T., Suzuki, M., Tkachenko, N. P., Valencia, G., Bibber, K., Vincter, M. G., Ward, D. R., Webber, B. R., Whalley, M., Wolfenstein, L., Womersley, J., Woody, C. L., and Zenin, O. V.

357. Cherenkov radiation by massless neutrinos in a magnetic field

Author: Ara Ioannisian and Raffelt, G. G.

358. COBRAS: Goal and Experimental Approach

Author: Mandolesi, N., Smoot, G. F., Bersanelli, M., Cesarsky, C., Lachieze-Rey, M., Danese, L., Vittorio, N., Bernardis, P., Dall Oglio, G., Sironi, G., Crane, P., Janssen, M., Partridge, B., Beckman, J., Rebolo, R., Puget, J. L., Bussoletti, E., Raffelt, G., Davies, R., Encrenaz, P., Natale, V., Tofani, G., Paola Merluzzi, Toffolatti, L., Scaramella, R., Martínez-Gonzáles, E., Sáez, D., Lasenby, A., and Efstathiou, G.

359. The LAGUNA project - Towards the giant liquid based detectors for proton decay searches and for low energy neutrino astrophysics

Author: Kisiel, J., Angus, D., Ariga, A., Autiero, D., Apostu, A., Badertscher, A., Bennet, T., Bertola, G., Bertola, P. F., Besida, O., Bettini, A., Booth, C., Borne, J. L., Brancus, I., Bujakowski, W., Campagne, J. E., Cata-Danil, G., Chipesiu, F., Chorowski, M., Cripps, J., Curioni, A., Davidson, S., Declais, Y. R. A., Drost, U., Duliu, O., Dumarchez, J., Enqvist, T., Ereditato, A., Feilitzsch, F. V., Fynbo, H., Gamble, T., Galvanin, G., Gendotti, A., Wojciech Gizicki, Goger-Neff, M., Grasslin, U., Gurney, D., Hakala, M., Hannestad, S., Haworth, M., Jipa, A., Juget, F., Kalliokoski, T., Katsanevas, S., Keen, M., Kreslo, I., Kudryastev, V., Kuusiniemi, P., Labarga, L., Lachenmaier, T., Lanfranchi, J. C., Lazanu, I., Lewke, T., Loo, K., Lightfoot, P., Lindner, M., Lombardi, P., Longhin, A., Maalampi, J., Marafini, M., Marchionni, A., Margineanu, R. M., Markiewicz, A., Marrodan-Undagoita, T., Marteau, J. E., Matikainen, R., Meindl, Q., Messina, M., Mietelski, J. W., Mitrica, B., Mordasini, A., Mosca, L., Moser, U., Nuijten, G., Oberauer, L., Oprina, A., Paling, S., Pascoli, S., Patzak, T., Pectu, M., Pilecki, Z., Piquemal, F., Potzel, W., Pytel, W., Raczynski, M., Raffelt, G., Ranucci, G., Ristaino, G., Robinson, M., Rogers, R., Roinisto, J., Romana, M., Rondio, E., Rossi, B., Rubbia, A., Sadecki, Z., Saenz, C., Saftoiu, A., Salmelainen, J., Sima, O., Slizowski, J., Slizowski, K., Sobczyk, J., Spooner, N., Stoica, S., Suhonen, J., Sulej, R., Szarska, M., Szeglowski, T., Temussi, M., Thompson, J., Thompson, L., Trzaska, W. H., Tippmann, M., Tonazzo, A., Urbanczyk, K., Vasseur, G., Williams, A., Winter, J., Wojtuszewska, K., Wurm, M., Zalewska, A., Zampaolo, M., Zito, M., Institut de Physique Nucléaire de Lyon (IPNL), Centre National de la Recherche Scientifique (CNRS)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Neutrinos, Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), European Organization for Nuclear Research (CERN), AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, APC - Neutrinos, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC)-AstroParticule et Cosmologie (APC (UMR_7164)), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Neutrino et Faibles Radioactivités (NEMO), Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG), Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Sciences et Technologies - Bordeaux 1 (UB)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Subjects: [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]
Abstract: PoS(EPS-HEP 2009)283 - The LAGUNA design study is financed by FP7 Research Infrastructure "Design Studies" Grant Agreement No. 212343 FP7-INFRA-2007-1.; International audience; A next generation European deep underground neutrino observatory is considered within the LAGUNA design study. Three detector options are presently considered: GLACIER liquid argon Time Projection Chamber; LENA liquid scintillator and MEMPHYS water Cherenkov. It will provide both: the high statistics measurement of neutrinos from variety of sources, and high sensitivity searches for matter instability. To accommodate such giant detectors a new underground laboratory is required. The LAGUNA design study considers the following seven candidate sites in Europe: Boulby (UK), Canfranc (Spain), Fréjus (France/Italy), Pyhäsalmi (Finland), Polkowice-Sieroszowice (Poland), Slanic (Romania) and Umbria (Italy). The three detection techniques and summary of the physics potential of proposed detectors are discussed in this short paper.

360. Review of particle physics. Particle Data Group

Author: Groom, Donald E., Aguilar-Benitez, M., Amsler, Claude, Barnett, R. Michael, Burchat, P. R., Carone, C. D., Caso, C., Conforto, G., Dahl, O., Doser, M., Eidelman, S., Feng, J. L., Gibbons, L., Goodman, M., Grab, C., Gurtu, A., Hagiwara, Kaoru, Hayes, K. G., Hernandez, J. J., Hikasa, K., Honscheid, K., Kolda, Christopher F., Mangano, Michelangelo L., Manohar, A. V., Masoni, A., Monig, Klaus, Murayama, H., Nakamura, K., Sergio Navas, Olive, Keith A., Pape, L., Piepke, A., Roos, M., Tanabashi, M., Tornqvist, N. A., Trippe, T. G., Vogel, P., Wohl, C. G., Workman, R. L., Yao, W. M., Armstrong, B., Casas Serradilla, J. L., Filimonov, B. B., Gee, P. S., Lugovsky, S. B., Nicholson, F., Babu, K. S., Besson, D., Biebel, O., Bloch, P., Cahn, R. N., Cattai, A., Chivukula, R. S., Cousins, R. D., Damour, T., Desler, K., Donahue, R. J., Edwards, D. A., Erler, J., Ezhela, V. V., Fasso, A., Fetscher, W., Froidevaux, D., Fukugita, M., Gaisser, T. K., Garren, L., Geer, S., Gerber, H. -J, Gilman, F. J., Haber, H. E., Hagmann, C., Hinchliffe, I., Hogan, C. J., Hohler, G., Jackson, John David, Johnson, K. F., Karlen, D., Kayser, Boris, Klein, Spencer, Kleinknecht, K., Knowles, I. G., Kolb, Edward W., Kreitz, P. A., Landua, R., Langacker, P., Littenberg, L., Manley, D. M., March-Russell, J., Nakada, T., Quinn, Helen R., Raffelt, G., Renk, B., Rolandi, Gigi, Ronan, M. T., Rosenberg, L. J., Schmitt, M., Schneider, O., Scott, D., Seligman, W. G., Shaevitz, M. H., Sjostrand, T., Smoot, George F., Spanier, S., Spieler, H., Srednicki, M., Stahl, A., Stanev, T., Suzuki, M., Tkachenko, N. P., Turner, M. S., Valencia, G., Bibber, K., Voss, R., Wolfenstein, L., and Womersley, J.

361. White paper report on Using Nuclear Reactors to Search for a value of $\theta_{13}$

Author: Anderson, K., Anjos, J. C., Ayres, D., Beacom, J., Bediaga, I., Bellefon, A., Berger, B. E., Bilenky, S., Blucher, E., Bolton, T., Buck, C., Bugg, W., Busenitz, J., Choubey, S., Conrad, J., Cribier, M., Dadoun, O., Dalnoki-Veress, F., Decowski, M., Gouvea, Andre, Demuth, D., Dessages-Ardellier, F., Efremenko, Y., Feilitzsch, F., Finley, D., Formaggio, J. A., Freedman, S. J., Fujikawa, B. K., Garbini, M., Giusti, P., Goger-Neff, M., Goodman, M., Gray, F., Grieb, C., Grudzinski, J. J., Guarino, V. J., Hartmann, F., Hagner, C., Heeger, K. M., Hofmann, W., Horton-Smith, G., Huber, P., Inzhechik, L., Jochum, J., Jostlein, H., Kadel, R., Kamyshkov, Y., Kaplan, D., Kasper, P., Kerret, H., Kersten, J., Klein, J., Knopfle, K. T., Kopeikin, V., Kozlov, Yu, Kryn, D., Kuchler, V., Kuze, M., Lachenmaier, T., Lasserre, T., Laughton, C., Lendvai, C., Li, J., Lindner, M., Link, J., Longo, M., Lu, Y. S., Luk, K. B., Ma, Y. Q., Martemyanov, V. P., Mauger, C., Menghetti, H., Mckeown, R., Mention, G., Meyer, J. P., Mikaelyan, L., Minakata, H., Naples, D., Nunokawa, H., Oberauer, L., Obolensky, M., Parke, S., Petcov, S. T., Peres, O. L. G., Potzel, W., Pilcher, J., Plunkett, R., Raffelt, G., Rapidis, P., Reyna, D., Roe, B., Rolinec, M., Sakamoto, Y., Sartorelli, G., Schonert, S., Schwetz, T., Selvi, M., Shaevitz, M., Shellard, R., Shrock, R., Sidwell, R., Sims, J., Sinev, V., Stanton, N., Stancu, I., Stefanski, R., Suekane, F., Sugiyama, H., Sukhotin, S., Sumiyoshi, T., Svoboda, R., Talaga, R., Tamura, N., Tanimoto, M., Thron, J., Toerne, E., Vignaud, D., Wagner, C., Wang, Y. F., Wang, Z., Winter, W., Wong, H., Yakushev, E., Yang, C. G., and Osamu Yasuda
Subjects: Physics, neutrino oscillations theta13 reactor neutrino experiment Diablo Canyon Daya Bay

362. Design for a practical laboratory detector for solar axions

Author: van Bibber, K., primary, McIntyre, P. M., additional, Morris, D. E., additional, and Raffelt, G. G., additional
Published: 1989
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363. Radiative decay of keV-mass sterile neutrino in magnetized electron plasma

Author: Dobrynina Alexandra, Mikheev Nicolay, and Raffelt Georg
Subjects: Physics, QC1-999
Abstract: The radiative decay of sterile neutrinos with typical masses of 10 keV is investigated in the presence of an external magnetic field and degenerate electron plasma. Full account is taken of the modified photon dispersion relation relative to vacuum. The limiting cases of relativistic and nonrelativistic plasma are analyzed. The decay rate calculated in a strongly magnetized plasma, as a function of the electron number density, is compared with the unmagnetized plasma limit. It is found that the presence of the strong magnetic field in the electron plasma suppresses the catalyzing influence of the plasma by itself on the sterile-neutrino decay rate.
Published: 2017
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364. Self-induced neutrino flavor conversion without flavor mixing.

Author: Chakraborty, S., Hansen, R. S., Izaguirre, I., and Raffelt, G. G.
Published: 2016
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365. The galactic globular cluster M5 (NGC 5904) as a particle physics laboratory

Author: Redondo J., Raffelt G.G., Viaux N., Catelan M., and Valcarce A.A.R.
Subjects: Physics, QC1-999
Abstract: Globular clusters have been used for a long time to test stellar evolution theories, and in particular to constrain novel forms of energy loss in low-mass stars. This includes constraints on axion properties, neutrino dipole moments, milli-charged particles, Kaluza-Klein gravitons, and many other phenomena. Depending on their interaction strength, these particles can be abundantly produced in stellar interiors, escape without further interaction, and thus drain energy directly from the stellar interior. Hence, they contribute directly to the stellar energy losses, thus modifying stellar evolution. Our goal is to re-examine such constraints in the light of modern data and updated stellar evolution codes, paying particular attention to systematic and statistical errors. As a first example, we consider the case of a neutrino magnetic moment that enhances the energy loss from the plasma process. In terms of the observed color-magnitude diagrams, the tip of the red giant branch (RGB) has been identified as a sensitive observable of the effects of the energy losses due to a neutrino magnetic moment. Here we describe the consequences of adding the cooling effect due to a neutrino magnetic moment to the Princeton-Goddard-PUC (PGPUC) stellar evolution code, exploring in particular the dependence of the position of the RGB tip on the neutrino magnetic moment. As a first application, we studied the position of the observed RGB tip in the case of the Galactic globular cluster M5 (NGC 5904), using the latest, high-precision, ground-based data from the P. B. Stetson database (2012, priv. comm.). We compare the empirical results with the PGPUC model predictions, and discuss the implied constraints on the value of the neutrino magnetic moment.
Published: 2013
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366. Self-induced flavor conversion of supernova neutrinos on small scales.

Author: Chakraborty, S., Hansen, R. S., Izaguirre, I., and Raffelt, G. G.
Published: 2016
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367. Dark matter and the age of globular clusters.

Author: Dearborn, D. and Raffelt, G.
Subjects: *STARS
Abstract: Simulates, numerically, the evolution of a horizontal-branch star. Methods; Results; Discussion.
Published: 1990
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368. Isocurvature forecast in the anthropic axion window.

Author: Hamann, J., Hannestad, S., Raffelt, G. G., and Wong, Y. Y. Y.
Published: 2009
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369. Neutrino masses and mixing from the astrophysical perspective

Author: RAFFELT, G
Published: 2001
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370. Neutrinos in astrophysics and cosmology

Author: RAFFELT, G
Published: 2000
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371. General kinetic description of relativistic mixed neutrinos

Author: Sigi, G. and Raffelt, G.
Published: 1993
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372. Neutrino Masses in Astrophysics and Cosmology

Author: Raffelt, G
Published: 1999
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373. Axion hunting at the turn of the millenium

Author: Raffelt, G
Published: 1999
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374. Stellar-evolution limits on axion properties

Author: Raffelt, G
Published: 1999
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375. Review of Particle Physics

Author: J Lesgourgues, Siegfried Bethke, C. Hanhart, P Eerola, Christian W. Bauer, F Takahashi, Oleg Zenin, A. de Gouvea, C. Grojean, O Buchmuller, Masaharu Tanabashi, P. de Jong, J. Erler, R Sekhar Chivukula, M Taševský, S.I. Eidelman, C. W. Walter, D J Miller, A. Piepke, Torbjörn Sjöstrand, Y Sumino, Orin I. Dahl, Herbert K. Dreiner, A Soffer, Chi Lin, Bogdan A. Dobrescu, S. M. Spanier, R E Mitchell, Marcela Carena, Manuella Vincter, Otmar Biebel, M Karliner, V. S. Lugovsky, Ren-Yuan Zhu, J. J. Beatty, C. Patrignani, A Pomarol, U Thoma, Kurtis F Johnson, N Varelas, William J. Marciano, David Milstead, Sw. Banerjee, Michael Doser, P Urquijo, A. Gurtu, A Bettini, Aneesh V. Manohar, L. S. Littenberg, Michael Syphers, Burkert, M C Gonzalez-Garcia, Ron L. Workman, Jamie Holder, German Valencia, Subir Sarkar, M Kenzie, Charles G Wohl, W. Fetscher, J Hisano, W Vogelsang, Th. Gutsche, Zoltan Ligeti, Thibault Damour, K Rabbertz, Marumi Kado, Sharma, G. Cowan, Klaus Mönig, Fabio Maltoni, C. L. Woody, Anatoli Romaniouk, A. Stahl, Michal Kreps, J Ellis, W-M. Yao, B C Allanach, J Anderson, Ken Ichi Hikasa, Eberhard Klempt, Keith A. Olive, V I Belousov, David H. Weinberg, J.J. Hernández-Rey, Meenakshi Narain, Younghoon Kwon, Andreas Ringwald, M O Wascko, K Trabelsi, E. J. Weinberg, R Yoshida, Jonas Rademacker, D. M. Asner, R A Ryutin, Paolo Molaro, C Lourengo, Peter Skands, Vorobyev, Wolfgang Walkowiak, S. B. Lugovsky, B. K. Heltsley, K. S. Lugovsky, Uli Katz, Daniel Tovey, George F. Smoot, Stephen R. Sharpe, S Heinemeyer, Brian D. Fields, H Ramani, Y Gershtein, R S Thorne, Ofer Lahav, K M Black, T Mannel, Timothy Gershon, Yoshinari Hayato, P. Schaffner, E. Blucher, G. Venanzoni, T Skwarnicki, Giancarlo D'Ambrosio, A J Schwartz, D J Robinson, G Rybka, Joey Huston, M S Sozzi, L.J. Rosenberg, L P Lellouch, Sophia L. Stone, U G Meißner, L. R. Wiencke, L Verde, S. Rolli, G. Dissertori, Augusto Ceccucci, S. T. Petcov, Matthias Neubert, Koji Nakamura, J. Beringer, E Pianori, W Zheng, G Zanderighi, Paul William Richardson, Daniel de Florian, Maksym Titov, C Lippmann, K Terashi, Y. Sakai, A Höcker, Ezhela, L. Tiator, Manuel Drees, A Pich, S Profumo, Gavin P. Salam, R. M. Barnett, J Schwiening, E C Aschenauer, Howard Baer, O. Schneider, Tony Gherghetta, P A Zyla, Jack Laiho, T Hyodo, Jonathan L. Rosner, B. Krusche, H J Gerber, Kate Scholberg, Stefan Roesler, Shoji Hashimoto, D Wands, G Aielli, A Holtkamp, Andrei Gritsan, Arnulf Quadt, A Freitas, Alessandro Cerri, U Egede, H. R. Gallagher, G. Gerbier, V A Khoze, S. R. Klein, B. N. Ratcliff, Y Makida, S. P. Wakely, Christoph Grab, Alberto Masoni, M Mikhasenko, Tony Liss, R. N. Cahn, A A Godizov, Paolo Nason, P. Nevski, T. Sumiyoshi, M D'Onofrio, A Lusiani, B. Foster, Thomas DeGrand, N. P. Tkachenko, Martin White, Douglas Scott, M Yokoyama, G P Zeller, M Ryskin, Petr Vogel, Christian Spiering, M A Bychkov, L. Garren, R. Kowalewski, John Terning, Claude Amsler, John Matthews, Y. Nir, A Hebecker, Mario Antonelli, M Ramsey-Musolf, Andreas Vogt, S L Zhu, Andrew R. Liddle, L Baudis, Debadi Chakraborty, Kaustubh Agashe, J Tanaka, S. Sánchez Navas, Howard E. Haber, Frank Krauss, M. C. Goodman, V A Petrov, Martin Grunewald, Fabio Sauli, D A Dwyer, R. G. Van de Water, M. Silari, John A. Peacock, S Willocq, T Shutt, Frank Zimmermann, Filip Moortgat, M Moskovic, Georg G. Raffelt, D. E. Groom, T. Basaglia, The George Washington University (GW), Thomas Jefferson National Accelerator Facility (Jefferson Lab), Florida State University [Tallahassee] (FSU), Helmholtz-Institut für Strahlen- und Kernphysik (HISKP), Rheinische Friedrich-Wilhelms-Universität Bonn, Institut für Kernphysik (IKP), Forschungszentrum Jülich GmbH | Centre de recherche de Juliers, Helmholtz-Gemeinschaft = Helmholtz Association-Helmholtz-Gemeinschaft = Helmholtz Association, University of Maryland [Baltimore], Università degli Studi di Roma Tor Vergata [Roma], University of Cambridge [UK] (CAM), Austrian Academy of Sciences (OeAW), INFN Frascati, Istituto Nazionale di Fisica Nucleare (INFN), Brookhaven National Laboratory [Upton, NY] (BNL), UT-Battelle, LLC-Stony Brook University [SUNY] (SBU), State University of New York (SUNY)-State University of New York (SUNY)-U.S. Department of Energy [Washington] (DOE), University of Oklahoma (OU), University of Louisville, Lawrence Berkeley National Laboratory [Berkeley] (LBNL), Universität Zürich [Zürich] = University of Zurich (UZH), Ohio State University [Columbus] (OSU), National Research Centre Kurchatov Institute, Istituto Nazionale di Fisica Nucleare, Sezione di Padova (INFN, Sezione di Padova), Ludwig-Maximilians-Universität München (LMU), University of Wisconsin Oshkosh (UWO), University of Chicago, Imperial College London, University of Virginia, Fermi National Accelerator Laboratory (Fermilab), CERN [Genève], University of Sussex, University of California (UC), Royal Holloway [University of London] (RHUL), State University of New York (SUNY Canton), Istituto Nazionale di Fisica Nucleare, Sezione di Milano (INFN), Istituto Nazionale di Fisica Nucleare, Sezione di Napoli (INFN, Sezione di Napoli), Institut des Hautes Études Scientifiques (IHES), IHES, Universidad Nacional de San Martin (UNSAM), Northwestern University [Evanston], University of Colorado [Boulder], University of Amsterdam [Amsterdam] (UvA), Yale University [New Haven], University of Liverpool, Universitätsklinikum Bonn (UKB), TKK Helsinki University of Technology (TKK), Monash university, Budker Institute of Nuclear Physics (BINP), Siberian Branch of the Russian Academy of Sciences (SB RAS), University of Illinois [Chicago] (UIC), University of Illinois System, King‘s College London, Departement Physik [ETH Zürich] (D-PHYS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), University of Pittsburgh (PITT), Pennsylvania Commonwealth System of Higher Education (PCSHE), Tufts University [Medford], Rutgers University [Camden], Rutgers University System (Rutgers), University of Minnesota System, Stony Brook University [SUNY] (SBU), State University of New York (SUNY), Argonne National Laboratory [Lemont] (ANL), Departement Erdwissenschaften [ETH Zürich] (D-ERDW), Johns Hopkins University (JHU), Deutsches Elektronen-Synchrotron [Hamburg] (DESY), University College Dublin [Dublin] (UCD), Department of Condensed Matter Physics and Materials Science [TIFR] (CMPMS), Tata Institute for Fundamental Research (TIFR), Universitätsklinikum Tübingen - University Hospital of Tübingen, Eberhard Karls Universität Tübingen = Eberhard Karls University of Tuebingen, Laboratoire Capteurs et Architectures Electroniques (LCAE), Département Métrologie Instrumentation & Information (DM2I), Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Technologique (CEA) (DRT (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Laboratoire d'Intégration des Systèmes et des Technologies (LIST (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Forschungszentrum Jülich GmbH, KEK (High energy accelerator research organization), The University of Tokyo (UTokyo), Heidelberg University, Universidad Autónoma de Madrid (UAM), Universitat de València (UV), Tohoku University [Sendai], University of Delaware [Newark], Michigan State University System, Tokyo Metropolitan University [Tokyo] (TMU), Gran Sasso Science Institute, INFN, Università degli Studi di Roma 'La Sapienza' = Sapienza University [Rome] (UNIROMA), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), Tel Aviv University (TAU), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), University of Warwick [Coventry], Department of Physics [Durham University], Durham University, University of Ljubljana, University of Basel (Unibas), Yonsei University, University College of London [London] (UCL), Syracuse University, Centre de Physique Théorique - UMR 7332 (CPT), Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), CPT - E1 Physique des particules, Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS)-Aix Marseille Université (AMU)-Université de Toulon (UTLN)-Centre National de la Recherche Scientifique (CNRS), Rheinisch-Westfälische Technische Hochschule Aachen University (RWTH), Universidade de Lisboa, GSI Helmholtzzentrum für Schwerionenforschung (GSI), City College of New York [CUNY] (CCNY), City University of New York [New York] (CUNY), Scuola Normale Superiore di Pisa (SNS), Université Catholique de Louvain = Catholic University of Louvain (UCL), Universität Siegen [Siegen], Istituto Nazionale di Fisica Nucleare, Sezione di Cagliari (INFN, Sezione di Cagliari), Louisiana State University (LSU), University of Glasgow, Stockholms universitet, Indiana State University, INAF/OATS, Trieste, Italy, Department of Applied Physics, Ghent University, Brown University, Università degli Studi di Milano-Bicocca = University of Milano-Bicocca (UNIMIB), Johannes Gutenberg - Universität Mainz = Johannes Gutenberg University (JGU), Weizmann Institute of Science [Rehovot, Israël], University of Bologna/Università di Bologna, University of Edinburgh, Institute of Molecular Genetics of National Research Centre «Kurchatov Institute» [Moscow, Russia], Russian Academy of Sciences [Moscow] (RAS), Instituto de Fisica Corpuscular (IFIC), Consejo Superior de Investigaciones Científicas [Madrid] (CSIC)-Universitat de València (UV), University of Alabama [Tuscaloosa] (UA), Universitat Autònoma de Barcelona (UAB), Georg-August-University = Georg-August-Universität Göttingen, Karlsruhe Institute of Technology (KIT), University of Bristol [Bristol], Max-Planck-Institut für Physik (Werner-Heisenberg-Institut) (MPI-P), Tsung-Dao Lee Institute, Shanghai Jiao Tong, SLAC National Accelerator Laboratory (SLAC), Stanford University, U.S. Department of Energy [Washington] (DOE), Leopold Franzens Universität Innsbruck - University of Innsbruck, The National Research Nuclear University MEPhI (Moscow Engineering Physics Institute) [Moscow, Russia], University of Mary Washington, Petersburg Nuclear Physics Institute, University of Oxford, Ecole Polytechnique Fédérale de Lausanne (EPFL), Technische Universität München = Technical University of Munich (TUM), University of Cincinnati (UC), University of British Columbia (UBC), University of Washington [Seattle], Istituto Nazionale di Fisica Nucleare [Pisa] (INFN), Lund University [Lund], AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), University of Pisa - Università di Pisa, University of Tennessee System, Northern Illinois University, Nagoya University, Tokyo University of Science [Tokyo], Czech Academy of Sciences [Prague] (CAS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, University of Sheffield [Sheffield], University of Melbourne, Monash University [Melbourne], University of Barcelona, California Institute of Technology (CALTECH), Department of Radiology [Radiologische Universitätsklinik Eberhard-Karls-Universität Tübingen], University of Portsmouth, Columbia University [New York], Colorado School of Mines, University of Massachusetts [Amherst] (UMass Amherst), University of Massachusetts System (UMASS), Max Planck Institute for the Physics of Complex Systems (MPI-PKS), Max-Planck-Gesellschaft, Moscow Institute of Physics and Technology [Moscow] (MIPT), Peking University [Beijing], Institute of High Energy Physics [Beijing] (IHEP), Chinese Academy of Sciences [Changchun Branch] (CAS), Particle Data Group, Institut des Hautes Etudes Scientifiques (IHES), Laboratoire de Physique Théorique et Hautes Energies (LPTHE), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Université Pierre et Marie Curie - Paris 6 (UPMC)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Département de Physique des Particules (ex SPP) (DPP), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), CEA/DSM, Département de Physique des Particules (ex SPP) (DPhP), UCL - SST/IRMP - Institut de recherche en mathématique et physique, Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), ITA, Department of Energy (US), Japan Society for the Promotion of Science, European Commission, Ministry of Education, Culture, Sports, Science and Technology (Japan), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Science and Technology Facilities Council (STFC), Tanabashi, M, Grp, P, Hagiwara, K, Hikasa, K, Nakamura, K, Sumino, Y, Takahashi, F, Tanaka, J, Agashe, K, Aielli, G, Amsler, C, Antonelli, M, Asner, D, Baer, H, Banerjee, S, Barnett, R, Basaglia, T, Bauer, C, Beatty, J, Belousov, V, Beringer, J, Bethke, S, Bettini, A, Bichsel, H, Biebel, O, Black, K, Blucher, E, Buchmuller, O, Burkert, V, Bychkov, M, Cahn, R, Carena, M, Ceccucci, A, Cerri, A, Chakraborty, D, Chen, M, Chivukula, R, Cowan, G, Dahl, O, D'Ambrosio, G, Damour, T, de Florian, D, de Gouvea, A, Degrand, T, de Jong, P, Dissertori, G, Dobrescu, B, D'Onofrio, M, Doser, M, Drees, M, Dreiner, H, Dwyer, D, Eerola, P, Eidelman, S, Ellis, J, Erler, J, Ezhela, V, Fetscher, W, Fields, B, Firestone, R, Foster, B, Freitas, A, Gallagher, H, Garren, L, Gerber, H, Gerbier, G, Gershon, T, Gershtein, Y, Gherghetta, T, Godizov, A, Goodman, M, Grab, C, Gritsan, A, Grojean, C, Groom, D, Grunewald, M, Gurtu, A, Gutsche, T, Haber, H, Hanhart, C, Hashimoto, S, Hayato, Y, Hayes, K, Hebecker, A, Heinemeyer, S, Heltsley, B, Hernandez-Rey, J, Hisano, J, Hocker, A, Holder, J, Holtkamp, A, Hyodo, T, Irwin, K, Johnson, K, Kado, M, Karliner, M, Katz, U, Klein, S, Klempt, E, Kowalewski, R, Krauss, F, Kreps, M, Krusche, B, Kuyanov, Y, Kwon, Y, Lahav, O, Laiho, J, Lesgourgues, J, Liddle, A, Ligeti, Z, Lin, C, Lippmann, C, Liss, T, Littenberg, L, Lugovsky, K, Lugovsky, S, Lusiani, A, Makida, Y, Maltoni, F, Mannel, T, Manohar, A, Marciano, W, Martin, A, Masoni, A, Matthews, J, Meissner, U, Milstead, D, Mitche, R, Moenig, K, Molaro, P, Moortgat, F, Moskovic, M, Murayama, H, Narain, M, Nason, P, Navas, S, Neubert, M, Nevski, P, Nir, Y, Olive, K, Griso, S, Parsons, J, Patrignani, C, Peacock, J, Pennington, M, Petcov, S, Petrov, V, Pianori, E, Piepke, A, Pomarol, A, Quadt, A, Rademacker, J, Raffelt, G, Ratcliff, B, Richardson, P, Ringwald, A, Roesler, S, Rolli, S, Romaniouk, A, Rosenberg, L, Rosner, J, Rybka, G, Ryutin, R, Sachrajda, C, Sakai, Y, Salam, G, Sarkar, S, Sauli, F, Schneider, O, Scholberg, K, Schwartz, A, Scott, D, Sharma, V, Sharpe, S, Shutt, T, Silari, M, Sjostrand, T, Skands, P, Skwarnicki, T, Smith, J, Smoot, G, Spanier, S, Spieler, H, Spiering, C, Stah, A, Stone, S, Sumiyoshi, T, Syphers, M, Terashi, K, Terning, J, Thoma, U, Thorne, R, Tiator, L, Titov, M, Tkachenko, N, Tornqvist, N, Tovey, D, Valencia, G, Van de Water, R, Varelas, N, Venanzoni, G, Verde, L, Vincter, M, Voge, P, Vogt, A, Wakely, S, Walkowiak, W, Walter, C, Wands, D, Ward, D, Wascko, M, Weiglein, G, Weinberg, D, Weinberg, E, White, M, Wiencke, L, Willocq, S, Woh, C, Womersley, J, Woody, C, Workman, R, Yao, W, Zeller, G, Zenin, O, Zhu, R, Zhu, S, Zimmermann, F, Zyla, P, Anderson, J, Fuller, L, Lugovsky, V, Schaffner, P, Tanabashi, M., Grp, Particle Data, Hagiwara, K., Hikasa, K., Nakamura, K., Sumino, Y., Takahashi, F., Tanaka, J., Agashe, K., Aielli, G., Amsler, C., Antonelli, M., Asner, D. M., Baer, H., Banerjee, Sw., Barnett, R. M., Basaglia, T., Bauer, C. W., Beatty, J. J., Belousov, V. I., Beringer, J., Bethke, S., Bettini, A., Bichsel, H., Biebel, O., Black, K. M., Blucher, E., Buchmuller, O., Burkert, V., Bychkov, M. A., Cahn, R. N., Carena, M., Ceccucci, A., Cerri, A., Chakraborty, D., Chen, M. -C., Chivukula, R. S., Cowan, G., Dahl, O., D'Ambrosio, G., Damour, T., de Florian, D., de Gouvea, A., Degrand, T., de Jong, P., Dissertori, G., Dobrescu, B. A., D'Onofrio, M., Doser, M., Drees, M., Dreiner, H. K., Dwyer, D. A., Eerola, P., Eidelman, S., Ellis, J., Erler, J., Ezhela, V. V., Fetscher, W., Fields, B. D., Firestone, R., Foster, B., Freitas, A., Gallagher, H., Garren, L., Gerber, H. -J., Gerbier, G., Gershon, T., Gershtein, Y., Gherghetta, T., Godizov, A. A., Goodman, M., Grab, C., Gritsan, A. V., Grojean, C., Groom, D. E., Grunewald, M., Gurtu, A., Gutsche, T., Haber, H. E., Hanhart, C., Hashimoto, S., Hayato, Y., Hayes, K. G., Hebecker, A., Heinemeyer, S., Heltsley, B., Hernandez-Rey, J. J., Hisano, J., Hocker, A., Holder, J., Holtkamp, A., Hyodo, T., Irwin, K. D., Johnson, K. F., Kado, M., Karliner, M., Katz, U. F., Klein, S. R., Klempt, E., Kowalewski, R. V., Krauss, F., Kreps, M., Krusche, B., Kuyanov, Yu. V., Kwon, Y., Lahav, O., Laiho, J., Lesgourgues, J., Liddle, A., Ligeti, Z., Lin, C. -J., Lippmann, C., Liss, T. M., Littenberg, L., Lugovsky, K. S., Lugovsky, S. B., Lusiani, A., Makida, Y., Maltoni, F., Mannel, T., Manohar, A. V., Marciano, W. J., Martin, A. D., Masoni, A., Matthews, J., Meissner, U. -G., Milstead, D., Mitche, R. E., Moenig, K., Molaro, P., Moortgat, F., Moskovic, M., Murayama, H., Narain, M., Nason, P., Navas, S., Neubert, M., Nevski, P., Nir, Y., Olive, K. A., Griso, S. Pagan, Parsons, J., Patrignani, C., Peacock, J. A., Pennington, M., Petcov, S. T., Petrov, V. A., Pianori, E., Piepke, A., Pomarol, A., Quadt, A., Rademacker, J., Raffelt, G., Ratcliff, B. N., Richardson, P., Ringwald, A., Roesler, S., Rolli, S., Romaniouk, A., Rosenberg, L. J., Rosner, J. L., Rybka, G., Ryutin, R. A., Sachrajda, C. T., Sakai, Y., Salam, G. P., Sarkar, S., Sauli, F., Schneider, O., Scholberg, K., Schwartz, A. J., Scott, D., Sharma, V., Sharpe, S. R., Shutt, T., Silari, M., Sjostrand, T., Skands, P., Skwarnicki, T., Smith, J. G., Smoot, G. F., Spanier, S., Spieler, H., Spiering, C., Stah, A., Stone, S. L., Sumiyoshi, T., Syphers, M. J., Terashi, K., Terning, J., Thoma, U., Thorne, R. S., Tiator, L., Titov, M., Tkachenko, N. P., Tornqvist, N. A., Tovey, D. R., Valencia, G., Van de Water, R., Varelas, N., Venanzoni, G., Verde, L., Vincter, M. G., Voge, P., Vogt, A., Wakely, S. P., Walkowiak, W., Walter, C. W., Wands, D., Ward, D. R., Wascko, M. O., Weiglein, G., Weinberg, D. H., Weinberg, E. J., White, M., Wiencke, L. R., Willocq, S., Woh, C. C., Womersley, J., Woody, C. L., Workman, R. L., Yao, W. -M., Zeller, G. P., Zenin, O. V., Zhu, R. -Y., Zhu, S. -L., Zimmermann, F., Zyla, P. A., Anderson, J., Fuller, L., Lugovsky, V. S., Schaffner, P., Robinson, D. J., Wohl, C. G., Allanach, B. C., Aschenauer, E. C., Baudis, L., Sekhar Chivukula, R., Egede, U., Gonzalez-Garcia, M. C., Huston, J., Kenzie, M., Khoze, V. A., Lellouch, L. P., Liddle, A. R., Lourenco, C., Mikhasenko, M., Miller, D. J., Mitchell, R. E., Monig, K., Pich, A., Profumo, S., Rabbertz, K., Ramani, H., Ramsey-Musolf, M., Ryskin, M., Schwiening, J., Soffer, A., Sozzi, M. S., Stahl, A., Tasevsky, M., Trabelsi, K., Urquijo, P., van de Water, R., Vogel, P., Vogelsang, W., Vorobyev, V., Yokoyama, M., Yoshida, R., Zanderighi, G., Zheng, W., and Department of Physics
Subjects: high energy, lepton, mixing [neutrino], High Energy Physics::Lattice, Cosmic microwave background, diffraction, Technicolor, Astrophysics, Omega, 01 natural sciences, Physics, Particles & Fields, higgs-boson production, Big Bang nucleosynthesis, cosmological model: parameter space, tau, dark energy, Monte Carlo, fields, pentaquark, instrumentation, Settore FIS/01, gauge boson, Anomalous magnetic dipole moment, deep-inelastic scattering, new physics, Physics, DOUBLE-BETA-DECAY, Electroweak interaction, density [dark matter], HEAVY FLAVOUR, Quarkonium, review, particle, physics, SUPERSYMMETRIC STANDARD MODEL, square-root-s, Physics, Nuclear, grand unified theory, boson: heavy, statistics, Physical Sciences, Higgs boson, axion: mass, flavor: violation, Neutrino, ELECTROWEAK SYMMETRY-BREAKING, numerical calculations: Monte Carlo, on-line, S013EPH, Quark, heavy [boson], [PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th], Physics, Multidisciplinary, anomalous magnetic-moment, electroweak radiative-corrections, dark matter: density, Higgs particle, meson, neutrino masses, neutrino mixing, neutrino oscillations, 114 Physical sciences, CHIRAL PERTURBATION-THEORY, neutrino mixing, Standard Model, quark, 0202 Atomic, Molecular, Nuclear, Particle And Plasma Physics, Nucleosynthesis, quantum chromodynamics, CP: violation, Dark matter, ddc:530, particle physics, Strong Interactions, 010306 general physics, sparticle, S013DF, grand unified theories, PRODUCTION, Gauge boson, Science & Technology, neutrino masses, 010308 nuclear & particles physics, C50 Other topics in experimental particle physics, Particle Data Group, Astronomy and Astrophysics, Deep inelastic scattering, to-leading-order, Automatic Keywords, heavy boson, axion, tables (particle physics), Tetraquark, proton-proton collisions, Supersymmetry, hadron, neutrino: mixing, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], cosmology, Volume (compression), HIGGS-BOSON, UB-VERTICAL-BAR, cosmological model, dark energy density, experimental methods, ddc:539.72021, Physics beyond the Standard Model, standard model, group theory, General Physics and Astronomy, tables, particle physics, high energy physics, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Quantum chromodynamics, energy: high, E Rev 2016, [PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th], Settore FIS/01 - Fisica Sperimentale, photon, Nuclear & Particles Physics, parameter space [cosmological model], dark energy: density, high [energy], M013WX, fermion-pair production, Nuclear and High Energy Physics, Particle physics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astronomy & Astrophysics, dark matter, statistical analysis, Double beta decay, 0103 physical sciences, conservation law, cold dark-matter, TAU LEPTONS, Astrophysics::Galaxy Astrophysics, tables, DEEP-INELASTIC-SCATTERING, electroweak interaction, High Energy Physics::Phenomenology, 750 GeV diphoton excess, PRODUCTION CROSS-SECTION, baryon, density [dark energy], Physics and Astronomy, gravitation, CKM matrix, [PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph], High Energy Physics::Experiment, supersymmetry, Minimal Supersymmetric Standard Model
Abstract: The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 2,143 new measurements from 709 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as supersymmetric particles, heavy bosons, axions, dark photons, etc. Particle properties and search limits are listed in Summary Tables. We give numerous tables, figures, formulae, and reviews of topics such as Higgs Boson Physics, Supersymmetry, Grand Unified Theories, Neutrino Mixing, Dark Energy, Dark Matter, Cosmology, Particle Detectors, Colliders, Probability and Statistics. Among the 120 reviews are many that are new or heavily revised, including a new review on Machine Learning, and one on Spectroscopy of Light Meson Resonances. The Review is divided into two volumes. Volume 1 includes the Summary Tables and 97 review articles. Volume 2 consists of the Particle Listings and contains also 23 reviews that address specific aspects of the data presented in the Listings. The complete Review (both volumes) is published online on the website of the Particle Data Group (pdg.lbl.gov) and in a journal. Volume 1 is available in print as the PDG Book. A Particle Physics Booklet with the Summary Tables and essential tables, figures, and equations from selected review articles is available in print, as a web version optimized for use on phones, and as an Android app., United States Department of Energy (DOE) DE-AC02-05CH11231, government of Japan (Ministry of Education, Culture, Sports, Science and Technology), Istituto Nazionale di Fisica Nucleare (INFN), Physical Society of Japan (JPS), European Laboratory for Particle Physics (CERN), United States Department of Energy (DOE)
Published: 2018
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376. Self-induced flavor conversion of supernova neutrinos on small scales

Author: Raffelt, G. [Max-Planck-Institut für Physik (Werner-Heisenberg-Institut),Föhringer Ring 6, 80805 München (Germany)]
Published: 2016
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377. Erratum: Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling [Phys. Rev. Lett. 104, 251101 (2010)]

Author: Raffelt, G
Published: 2010
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378. Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling

Author: Raffelt, G [Max-Planck-Institut fuer Physik, Werner-Heisenberg-Institut, Foehringer Ring 6, D-80802 Muenchen (Germany)]
Published: 2010
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379. Neutrino dispersion in external magnetic fields

Author: Raffelt, G [Max-Planck-Institut fuer Physik (Werner-Heisenberg-Institut), Foehringer Ring 6, 80805 Munich (Germany)]
Published: 2006
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380. Pulsar bound on the photon electric charge reexamined

Author: Raffelt, G [Center for Particle Astrophysics, University of California, Berkeley, California 94720 (United States)]
Published: 1994
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381. An update on the Axion Helioscopes front: current activities at CAST and the IAXO project

Author: Joachim Jacoby, J. I. Collar, H. Ten Kate, Fritz Caspers, Julia Vogel, J. Kaminski, H. Silva, Giovanni Cantatore, Benito Gimeno, S. C. Yildiz, M. Betz, Alexey Dudarev, Georg G. Raffelt, A. Belov, F.J. Iguaz, Rainer Kotthaus, Javier Redondo, F. Haug, K. Barth, G. Luzón, Klaus Kurt Desch, C. Eleftheriadis, S. Caspi, P. Brax, Georgios Fanourakis, W. C. Wester, Hector Gomez, J. M. Laurent, N. Breijnholt, I. Dratchnev, Toyokazu Sekiguchi, S. Neff, L. Stewart, Joerg Jaeckel, Amanda Weltman, Marin Karuza, C. Krieger, Pierre Sikivie, A. Tomás, S. Aune, C. Nones, Heinrich Bräuninger, Serkant Ali Cetin, M. Rosu, I. G. Irastorza, J. M. Carmona, Babette Döbrich, Krešimir Jakovčić, Steffen Hauf, Takashi Hiramatsu, Biljana Lakić, Milica Krčmar, Evangelos Gazis, M. Davenport, Dieter H. H. Hoffmann, T. Papaevangelou, J.A. Villar, A. V. Derbin, Ante Ljubičić, Dieter Horns, S. N. Gninenko, A. Diago, I. Ortega, S. Matsuki, E. Gruber, Sergey Troitsky, T. Dafni, J. G. Garza, I. Savvidis, Andreas Ringwald, A. Lindner, Jordi Isern, M. Arik, Javier Galan, Ken'ichi Saikawa, E. Georgiopoulou, T. Guthörl, Eduardo Guendelman, Adriane De Assis Lawisch Rodriguez, I. Shilon, D. Chelouche, S. Russenschuck, Kenichi Imai, V. N. Muratova, P. Vedrine, F.E. Christensen, T. O. Niinikoski, E. Ferrer-Ribas, F. T. Avignone, Charles J. Hailey, M. D. Hasinoff, Peter Friedrich, M. J. Pivovaroff, Konstantin Zioutas, Sami K. Solanki, Louis Walckiers, H. Riege, Pierre Brun, Konstantinos Kousouris, Markus Kuster, A. Dael, T. Geralis, Gianpaolo Carosi, J. A. Garcia, A. Gardikiotis, Yannis K. Semertzidis, Eric Armengaud, Raimo Hartmann, Theodoros Vafeiadis, J. Ruz, K. Königsmann, Masahiro Kawasaki, D. González-Díaz, I. Giomataris, K. van Bibber, Olivier Limousin, A.C. Jakobsen, A. Liolios, Dafni, T, Arik, M., Armengaud, E., Aune, S., Avignone, F. T., Barth, K., Belov, A., Betz, M., Bräuninger, H., Brax, P., Breijnholt, N., Brun, P., Cantatore, Giovanni, Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Collar, J. I., Dael, A., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Friedrich, P., Galán, J., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Georgiopoulou, E., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., González Díaz, D., Gruber, E., Guendelman, E., Guthörl, T., Hailey, C. J., Hartmann, R., Hauf, S., Haug, F., Hasinoff, M. D., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G., Isern, J., Imai, K., Jacoby, J., Jaeckel, J., Jakobsen, A. C., Jakovcić, K., Kaminski, J., Kawasaki, M., Karuza, M., Königsmann, K., Kotthaus, R., Krcmar, M., Kousouris, K., Krieger, C., Kuster, M., Lakić, B., Laurent, J. M., Limousin, O., Lindner, A., Liolios, A., Ljubicić, A., Luzón, G., Matsuki, S., Muratova, V. N., Neff, S., Niinikoski, T., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Riege, H., Ringwald, A., Rodríguez, A., Rosu, M., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Solanki, S. K., Stewart, L., ten Kate, H. H. J., Tomas, A., Troitsky, S., Vafeiadis, T., van Bibber, K., Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., Zioutas, K., Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Arık, Metin, and Yıldız, Süleyman Cenk
Subjects: X-Ray Focusing Devices, X-ray detector, Particle physics, Nuclear and High Energy Physics, X-ray focusing device, Axions, Dark matter, Magnet Development, Micromegas detector, axions, dark matter, x-ray, detectors, micromegas detectors, x-ray focusing devices, magnet development, CAST, IAXO, 01 natural sciences, Axion, Primary (astronomy), Observatory, 0103 physical sciences, Dark Matter, X-Ray Detectors, 010306 general physics, Physics, Helioscope, Micromegas Detectors, 010308 nuclear & particles physics, Magnet development, Micromegas detectors, X-ray detectors, X-ray focusing devices, Orders of magnitude (time), Experimental methods, CERN Axion Solar Telescope
Abstract: Çetin, Serkant Ali (Dogus Author) -- Arık, Metin (Dogus Author) -- Yıldız, Süleyman Cenk (Dogus Author) Although they have not yet been detected, axions and axion-like particles (ALPs) continue to maintain the interest (even increasingly so) of the rare-event searches community as viable candidates for the Dark Matter of the Universe but also as a solution for several other puzzles of astrophysics. Their property of coupling to photons has inspired different experimental methods for their detection, one of which is the helioscope technique. The CERN Axion Solar Telescope (CAST) is the most sensitive helioscope built up to date and has recently published part of the latest data taken with the magnet bores gradually filled with He-3, probing the mass range up to 1.17 eV. The International AXion Observatory (IAXO) is being proposed as a facility where different axion studies can be performed, with the primary goal to study axions coming from the Sun. Designed to maximize sensitivity, it will improve the levels reached by CAST by almost 5 orders of magnitude in signal detection, that is more than one order of magnitude in terms of gay. Here we will summarize the most important aspects of the helioscopes, and focus mainly on IAXO, based on the recent papers [1, 2].
Published: 2016
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382. New bound on neutrino dipole moments from globular-cluster stars

Author: Raffelt, G [Max-Planck-Institut fuer Physik, Postfach 401212, 8000 Muenchen 40 (West Germany)]
Published: 1990
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383. Axion bremsstrahlung in red giants

Author: Raffelt, G [Astronomy Department Center for Particle Astrophysics, University of California, Berkeley, California 94720 (US)]
Published: 1990
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384. The Next Generation of Axion Helioscopes: The International Axion Observatory (IAXO)

Author: Javier Redondo, Biljana Lakić, Eduardo Guendelman, K. van Bibber, A. Diago, S. Matsuki, Hector Gomez, Marin Karuza, C. Eleftheriadis, Olivier Limousin, H. H. J. ten Kate, Eric Armengaud, T. Dafni, Finn Erland Christensen, I. Ortega, Pierre Sikivie, Anders Clemen Jakobsen, F.J. Iguaz, Charles J. Hailey, Diego González-Díaz, Theodoros Vafeiadis, Milica Krčmar, Takashi Hiramatsu, V. N. Muratova, Dieter H. H. Hoffmann, J.A. Villar, S. C. Yildiz, Klaus Kurt Desch, I. Shilon, B. Döbrich, Javier Galan, J. G. Garza, Pierre Brun, A. Dael, S. Gninenko, F. T. Avignone, A. Tomás, W. C. Wester, C. Krieger, I. G. Irastorza, Masahiro Kawasaki, A. Lindner, A. Dudarev, Andreas Ringwald, Michael J. Pivovaroff, M. Betz, A. V. Derbin, P. Brax, C. Nones, D. Chelouche, Ioannis Giomataris, I. Savvidis, Yannis K. Semertzidis, S. Russenschuck, Kenichi Imai, Konstantin Zioutas, Theodoros Geralis, Serkant Ali Cetin, Giovanni Cantatore, Julia Vogel, Jordi Isern, H. Silva, E. Ferrer-Ribas, Ken'ichi Saikawa, G. Luzón, Dieter Horns, P. Vedrine, G. Fanourakis, Toyokazu Sekiguchi, Fritz Caspers, J. A. Garcia, Joerg Jaeckel, Amanda Weltman, J. Ruz, M. Davenport, J. Kaminski, L. Walckiers, Krešimir Jakovčić, Gianpaolo Carosi, A. Liolios, B. Gimeno, Georg G. Raffelt, T. Papaevangelou, J. M. Carmona, S. Caspi, Konstantinos Kousouris, I. Dratchnev, Sergey Troitsky, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Vogel, J. K., Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, Giovanni, Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Dael, A., Dafni, T., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Galán, J., García, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., González Díaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G., Isern, J., Imai, K., Jakobsen, A. C., Jaeckel, J., Jakovčić, K., Kaminski, J., Kawasaki, M., Karuza, M., Krčmar, M., Kousouris, K., Krieger, C., Lakić, B., Limousin, O., Lindner, A., Liolios, A., Luzón, G., Matsuki, S., Muratova, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., ten Kate, H., Tomas, A., Troitsky, S., Vafeiadis, T., van Bibber, K., Vedrine, P., Villar, J. A., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., and Zioutas, K.
Subjects: QCD axion, Particle physics, Physics::Instrumentation and Detectors, Dark matter, Physics and Astronomy(all), 01 natural sciences, 7. Clean energy, magnetic helioscope, High Energy Physics::Theory, QCD axions, Astroparticle Physics, Axion, Observatory, 0103 physical sciences, dark matter, Dark Matter, ddc:530, Detectors and Experimental Techniques, 010306 general physics, Astroparticle physics, Physics, Helioscope, 010308 nuclear & particles physics, Axion Dark Matter Experiment, High Energy Physics::Phenomenology, Strong CP problem, IAXO, Strong CP Problem, ALP, CERN Axion Solar Telescope, Particle Physics - Experiment, Helioscopes
Abstract: Çetin, Serkant Ali (Dogus Author) -- Conference full title: 13th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2013; Asilomar Conference Grounds Monterey Peninsula; United States; 8 September 2013 through 13 September 2013. The International Axion Observatory (IAXO) is a proposed 4th-generation axion helioscope with the primary physics research goal to search for solar axions via their Primakoff conversion into photons of 1 - 10 keV energies in a strong magnetic field. IAXO will achieve a sensitivity to the axion-photon coupling gaγ down to a few ×10-12 GeV-1 for a wide range of axion masses up to ∼ 0.25 eV. This is an improvement over the currently best (3rd generation) axion helioscope, the CERN Axion Solar Telescope (CAST), of about 5 orders of magnitude in signal strength, corresponding to a factor ∼ 20 in the axion photon coupling. IAXO's sensitivity relies on the construction of a large superconducting 8-coil toroidal magnet of 20 m length optimized for axion research. Each of the eight 60 cm diameter magnet bores is equipped with x-ray optics focusing the signal photons into ∼ 0.2 cm2 spots that are imaged by very low background x-ray detectors. The magnet will be built into a structure with elevation and azimuth drives that will allow solar tracking for 12 hours each day. This contribution is a summary of our papers [1-3] and we refer to these for further details.
Published: 2015
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385. Neutrino Physics with JUNO

Author: Jilei Xu, Andre Kruth, Yuguang Xie, Wei Wang, S. M. Chen, Janet Conrad, Xingtao Huang, V. Vorobel, Jose Busto, Qi An, Alexander Olshevskiy, Jiaxing Li, Cécile Jollet, Xiangdong Ji, Ran Han, Sandra Zavatarelli, Dmitriy Taichenachev, F. Yermia, Georg G. Raffelt, R. Möllenberg, Yong Zhong Qian, Ugur Yegin, Yu Yao, Wenxiong Zhou, Siguang Wang, Zheng Wang, Zhenyu Zhang, Rupert Leitner, M. Göger-Neff, Lino Miramonti, Qun Wu, O. Drapier, Donghua Fan, Jen-Chieh Peng, D. W. Liu, Stephen T. Dye, Hao Cai, John F. Beacom, Lucia Votano, Massimiliano Clemenza, Juan Pedro Ochoa-Ricoux, Davide Chiesa, Tao Hu, Igor Tkachev, Fabio Mantovani, Hongbang Liu, Jiawen Zhang, J. G. Lu, Shulin Liu, Baojun Yan, Weili Zhong, Changgen Yang, A. Garfagnini, Antonio Cammi, Liangjian Wen, Guofu Cao, Christopher Wiebusch, Michael Wurm, Anselmo Meregaglia, Xubo Ma, Boxiang Yu, G. Meng, Damien Dornic, Vladimir Lyashuk, Björn Wonsak, Anatael Cabrera, Y. H. Zhou, Jochen Steinmann, M. Soiron, S. Dusini, Xiaomei Li, Honghao Zhang, Yajun Mao, Gang Guo, Y. B. Hsiung, Z. V. Krumshteyn, Marco Grassi, Guanghua Gong, Guang Yang, Zhi Deng, Laurent Favart, Shaomin Chen, Jun Cao, Lothar Oberauer, Xilei Sun, Herve De Kerret, Hao Liang, Ara Ioannisian, Yufei Xi, Monica Sisti, Chao Li, Yuekun Heng, Yifang Wang, Alessandro Paoloni, Stefan van Waasen, Qingmin Zhang, Meng Wang, Shouyang Hu, Jing Zhou, Dongmei Xia, Yongjie Sun, G. Salamanna, Ezio Previtali, Mengyun Guan, Thomas Mueller, Bayarto Lubsandorzhiev, Xin Heng Guo, Guorong Zhou, Xiao Cai, Guey-Lin Lin, Zhimin Wang, Margherita Buizza Avanzini, Mauro Mezzetto, Barbara Ricci, Hu Liu, Chiara Sirignano, William F. McDonough, Xichao Ruan, Dmitry V. Naumov, Jiajie Ling, Ziyan Deng, Haoqi Lu, Jianglai Liu, Paolo Lombardi, Xiang Zhou, Manfred Jeitler, Weiguo Li, Christian Grewing, Barbara Clerbaux, Jianli Liu, Jian Fang, Yi Chen, Ming Qi, Oleg Smirnov, L. B. Bezrukov, Narine Kazarian, Yangheng Zheng, Wanlei Guo, Marcos Dracos, Jinchang Liu, Hui Gong, Ivano Lippi, Michael Karagounis, Stefano Maria Mari, Vito Antonelli, Miao He, Zhengyun You, Yayun Ding, Richard Ford, Zelimir Djurcic, Qian Liu, Zhonghua Qin, Jian Tang, E. Meroni, Shubin Liu, Ruiguang Wang, Jingbo Zhang, Rong Zhou, Timo Enqvist, Zhe Wang, V. V. Sinev, Simon Blyth, Zhenghua Zhao, Yi Wang, Yumei Zhang, Yi Li, Zeyuan Yu, Tobias Lachenmaier, Marco Giammarchi, Yongbing Long, Maxim Gonchar, Wei Wei, D. D'Angelo, Sen Qian, Shu Luo, Caren Hagner, Claudia-Elisabeth Wulz, H. Peng, Jiaheng Zou, Liang Zhan, Yifan Yang, Chunxu Yu, Wei Li, Markus Robens, Fengpeng An, Xiaoshan Jiang, Yen-Hsun Lin, Pasi Kuusiniemi, Zhibing Li, Luca Stanco, Fausto Ortica, Chao Zhang, Guangpeng An, Xiangdong Ruan, R. Brugnera, Achim Stahl, Eric Baussan, Yufeng Li, Livia Ludhova, Chung Hsiang Wang, Lei Huo, Vic Guarino, Tao Lin, X. N. Li, Haonan Gan, Lei Yang, Hao Wang, M. Gonin, Ye-Ling Zhou, Yun Chang, M. H. Shaevitz, Xin Qian, Wladyslaw Henryk Trzaska, Li Zhou, C. G. Yang, Zhi-zhong Xing, Jingbin Lu, Aldo Romani, Shun Zhou, Cristina Volpe, Li Kang, Junguang Lu, Gioacchino Ranucci, Hanxiong Huang, Guo-Li Wang, Jun Hu, Institut Pluridisciplinaire Hubert Curien (IPHC), Université de Strasbourg (UNISTRA)-Université de Haute-Alsace (UHA) Mulhouse - Colmar (Université de Haute-Alsace (UHA))-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Leprince-Ringuet (LLR), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), JUNO, An, F, An, G, An, Q, Antonelli, V, Baussan, E, Beacom, J, Bezrukov, L, Blyth, S, Brugnera, R, Avanzini, M, Busto, J, Cabrera, A, Cai, H, Cai, X, Cammi, A, Cao, G, Cao, J, Chang, Y, Chen, S, Chen, Y, Chiesa, D, Clemenza, M, Clerbaux, B, Conrad, J, D'Angelo, D, De Kerret, H, Deng, Z, Ding, Y, Djurcic, Z, Dornic, D, Dracos, M, Drapier, O, Dusini, S, Dye, S, Enqvist, T, Fan, D, Fang, J, Favart, L, Ford, R, Göger Neff, M, Gan, H, Garfagnini, A, Giammarchi, M, Gonchar, M, Gong, G, Gong, H, Gonin, M, Grassi, M, Grewing, C, Guan, M, Guarino, V, Guo, G, Guo, W, Guo, X, Hagner, C, Han, R, He, M, Heng, Y, Hsiung, Y, Hu, J, Hu, S, Hu, T, Huang, H, Huang, X, Huo, L, Ioannisian, A, Jeitler, M, Ji, X, Jiang, X, Jollet, C, Kang, L, Karagounis, M, Kazarian, N, Krumshteyn, Z, Kruth, A, Kuusiniemi, P, Lachenmaier, T, Leitner, R, Li, C, Li, J, Li, W, Li, X, Li, Y, Li, Z, Liang, H, Lin, G, Lin, T, Lin, Y, Ling, J, Lippi, I, Liu, D, Liu, H, Liu, J, Liu, Q, Liu, S, Lombardi, P, Long, Y, Lu, H, Lu, J, Lubsandorzhiev, B, Ludhova, L, Luo, S, Lyashuk, V, Möllenberg, R, Ma, X, Mantovani, F, Mao, Y, Mari, S, Mcdonough, W, Meng, G, Meregaglia, A, Meroni, E, Mezzetto, M, Miramonti, L, Mueller, T, Naumov, D, Oberauer, L, Ochoa Ricoux, J, Olshevskiy, A, Ortica, F, Paoloni, A, Peng, H, Peng, J, Previtali, E, Qi, M, Qian, S, Qian, X, Qian, Y, Qin, Z, Raffelt, G, Ranucci, G, Ricci, B, Robens, M, Romani, A, Ruan, X, Salamanna, G, Shaevitz, M, Sinev, V, Sirignano, C, Sisti, M, Smirnov, O, Soiron, M, Stahl, A, Stanco, L, Steinmann, J, Sun, X, Sun, Y, Taichenachev, D, Tang, J, Tkachev, I, Trzaska, W, Van Waasen, S, Volpe, C, Vorobel, V, Votano, L, Wang, C, Wang, G, Wang, H, Wang, M, Wang, R, Wang, S, Wang, W, Wang, Y, Wang, Z, Wei, W, Wen, L, Wiebusch, C, Wonsak, B, Wu, Q, Wulz, C, Wurm, M, Xi, Y, Xia, D, Xie, Y, Xing, Z, Xu, J, Yan, B, Yang, C, Yang, G, Yang, L, Yang, Y, Yao, Y, Yegin, U, Yermia, F, You, Z, Yu, B, Yu, C, Yu, Z, Zavatarelli, S, Zhan, L, Zhang, C, Zhang, H, Zhang, J, Zhang, Q, Zhang, Y, Zhang, Z, Zhao, Z, Zheng, Y, Zhong, W, Zhou, G, Zhou, J, Zhou, L, Zhou, R, Zhou, S, Zhou, W, Zhou, X, Zhou, Y, Zou, J, Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), An, Fengpeng, An, Guangpeng, An, Qi, Antonelli, Vito, Baussan, Eric, Beacom, John, Bezrukov, Leonid, Blyth, Simon, Brugnera, Riccardo, Avanzini, Margherita Buizza, Busto, Jose, Cabrera, Anatael, Cai, Hao, Cai, Xiao, Cammi, Antonio, Cao, Guofu, Cao, Jun, Chang, Yun, Chen, Shaomin, Chen, Shenjian, Chen, Yixue, Chiesa, Davide, Clemenza, Massimiliano, Clerbaux, Barbara, Conrad, Janet, D’Angelo, Davide, Kerret, Hervé De, Deng, Zhi, Deng, Ziyan, Ding, Yayun, Djurcic, Zelimir, Dornic, Damien, Dracos, Marco, Drapier, Olivier, Dusini, Stefano, Dye, Stephen, Enqvist, Timo, Fan, Donghua, Fang, Jian, Favart, Laurent, Ford, Richard, Göger Neff, Marianne, Gan, Haonan, Garfagnini, Alberto, Giammarchi, Marco, Gonchar, Maxim, Gong, Guanghua, Gong, Hui, Gonin, Michel, Grassi, Marco, Grewing, Christian, Guan, Mengyun, Guarino, Vic, Guo, Gang, Guo, Wanlei, Guo, Xin Heng, Hagner, Caren, Han, Ran, He, Miao, Heng, Yuekun, Hsiung, Yee, Hu, Jun, Hu, Shouyang, Hu, Tao, Huang, Hanxiong, Huang, Xingtao, Huo, Lei, Ioannisian, Ara, Jeitler, Manfred, Ji, Xiangdong, Jiang, Xiaoshan, Jollet, Cécile, Kang, Li, Karagounis, Michael, Kazarian, Narine, Krumshteyn, Zinovy, Kruth, Andre, Kuusiniemi, Pasi, Lachenmaier, Tobia, Leitner, Rupert, Li, Chao, Li, Jiaxing, Li, Weidong, Li, Weiguo, Li, Xiaomei, Li, Xiaonan, Li, Yi, Li, Yufeng, Li, Zhi Bing, Liang, Hao, Lin, Guey Lin, Lin, Tao, Lin, Yen Hsun, Ling, Jiajie, Lippi, Ivano, Liu, Dawei, Liu, Hongbang, Liu, Hu, Liu, Jianglai, Liu, Jianli, Liu, Jinchang, Liu, Qian, Liu, Shubin, Liu, Shulin, Lombardi, Paolo, Long, Yongbing, Lu, Haoqi, Lu, Jiashu, Lu, Jingbin, Lu, Junguang, Lubsandorzhiev, Bayarto, Ludhova, Livia, Luo, Shu, Vladimir Lyashuk, Null, Möllenberg, Randolph, Ma, Xubo, Mantovani, Fabio, Mao, Yajun, Mari, Stefano Maria, Mcdonough, William F, Meng, Guang, Meregaglia, Anselmo, Meroni, Emanuela, Mezzetto, Mauro, Miramonti, Lino, Thomas Mueller, Null, Naumov, Dmitry, Oberauer, Lothar, Ochoa Ricoux, Juan Pedro, Olshevskiy, Alexander, Ortica, Fausto, Paoloni, Alessandro, Peng, Haiping, Jen Chieh Peng, Null, Previtali, Ezio, Qi, Ming, Qian, Sen, Qian, Xin, Qian, Yongzhong, Qin, Zhonghua, Raffelt, Georg, Ranucci, Gioacchino, Ricci, Barbara, Robens, Marku, Romani, Aldo, Ruan, Xiangdong, Ruan, Xichao, Salamanna, Giuseppe, Shaevitz, Mike, Valery Sinev, Null, Sirignano, Chiara, Sisti, Monica, Smirnov, Oleg, Soiron, Michael, Stahl, Achim, Stanco, Luca, Steinmann, Jochen, Sun, Xilei, Sun, Yongjie, Taichenachev, Dmitriy, Tang, Jian, Tkachev, Igor, Trzaska, Wladyslaw, Waasen, Stefan van, Volpe, Cristina, Vorobel, Vit, Votano, Lucia, Wang, Chung Hsiang, Wang, Guoli, Wang, Hao, Wang, Meng, Wang, Ruiguang, Wang, Siguang, Wang, Wei, Wang, Yi, Wang, Yifang, Wang, Zhe, Wang, Zheng, Wang, Zhigang, Wang, Zhimin, Wei, Wei, Wen, Liangjian, Wiebusch, Christopher, Wonsak, Björn, Wu, Qun, Wulz, Claudia Elisabeth, Wurm, Michael, Xi, Yufei, Xia, Dongmei, Xie, Yuguang, Zhi zhong Xing, Null, Xu, Jilei, Yan, Baojun, Yang, Changgen, Yang, Chaowen, Yang, Guang, Yang, Lei, Yang, Yifan, Yao, Yu, Yegin, Ugur, Yermia, Frédéric, You, Zhengyun, Yu, Boxiang, Yu, Chunxu, Yu, Zeyuan, Zavatarelli, Sandra, Zhan, Liang, Zhang, Chao, Zhang, Hong Hao, Zhang, Jiawen, Zhang, Jingbo, Zhang, Qingmin, Zhang, Yu Mei, Zhang, Zhenyu, Zhao, Zhenghua, Zheng, Yangheng, Zhong, Weili, Zhou, Guorong, Zhou, Jing, Zhou, Li, Zhou, Rong, Zhou, Shun, Zhou, Wenxiong, Zhou, Xiang, Zhou, Yeling, Zhou, Yufeng, Zou, Jiaheng, Université de Strasbourg (UNISTRA)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Aix Marseille Université (AMU), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), Massachusetts Institute of Technology. Department of Physics, and Conrad, Janet Marie
Subjects: Particle physics, Sterile neutrino, Nuclear and High Energy Physics, Physics - Instrumentation and Detectors, Geoneutrino, reactor neutrino experiment, Physics::Instrumentation and Detectors, Solar neutrino, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, FOS: Physical sciences, 7. Clean energy, 01 natural sciences, NO, High Energy Physics - Experiment, neutrino astronomy, High Energy Physics - Experiment (hep-ex), neutrino physics, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], ddc:530, neutrino, mass hierarchy, reactor, liquid scintillator, 010306 general physics, Jiangmen Underground Neutrino Observatory, media_common, Physics, 010308 nuclear & particles physics, High Energy Physics::Phenomenology, neutrino physic, Instrumentation and Detectors (physics.ins-det), Universe, reactor neutrino experiments, large scintillator detectors, Supernova, 13. Climate action, Physics::Space Physics, large scintillator detector, High Energy Physics::Experiment, Neutrino
Abstract: The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hierarchy as a primary physics goal. It is also capable of observing neutrinos from terrestrial and extra-terrestrial sources, including supernova burst neutrinos, diffuse supernova neutrino background, geoneutrinos, atmospheric neutrinos, solar neutrinos, as well as exotic searches such as nucleon decays, dark matter, sterile neutrinos, etc. We present the physics motivations and the anticipated performance of the JUNO detector for various proposed measurements. By detecting reactor antineutrinos from two power plants at 53-km distance, JUNO will determine the neutrino mass hierarchy at a 3-4 sigma significance with six years of running. The measurement of antineutrino spectrum will also lead to the precise determination of three out of the six oscillation parameters to an accuracy of better than 1\%. Neutrino burst from a typical core-collapse supernova at 10 kpc would lead to ~5000 inverse-beta-decay events and ~2000 all-flavor neutrino-proton elastic scattering events in JUNO. Detection of DSNB would provide valuable information on the cosmic star-formation rate and the average core-collapsed neutrino energy spectrum. Geo-neutrinos can be detected in JUNO with a rate of ~400 events per year, significantly improving the statistics of existing geoneutrino samples. The JUNO detector is sensitive to several exotic searches, e.g. proton decay via the $p\to K^++\bar\nu$ decay channel. The JUNO detector will provide a unique facility to address many outstanding crucial questions in particle and astrophysics. It holds the great potential for further advancing our quest to understanding the fundamental properties of neutrinos, one of the building blocks of our Universe., Comment: Version submitted to Journal of Physics G, with minor typo corrections. 222 Pages, 147 figures
Published: 2016
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386. Diffuse cosmic neutrino background from population III stars

Author: Pasquale D. Serpico, Gianpiero Mangano, Gennaro Miele, Georg G. Raffelt, Fabio Iocco, Iocco, F., Mangano, G., Miele, Gennaro, Raffelt, G. G., and Serpico, P. D.
Subjects: Physics, education.field_of_study, Astrophysics::High Energy Astrophysical Phenomena, Metallicity, Solar neutrino, Astrophysics (astro-ph), Population, FOS: Physical sciences, Astronomy, Astronomy and Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Solar neutrino problem, Redshift, Cosmic neutrino background, High Energy Physics - Phenomenology, Stars, High Energy Physics - Phenomenology (hep-ph), Astrophysics::Solar and Stellar Astrophysics, Neutrino, education
Abstract: We study the expected diffuse cosmic neutrino flux produced by Population III (PopIII) stars during their nuclear burning phases as well as from their final stages of evolution (core collapse). Assuming a fraction f_III=10^(-3) of all baryons forms PopIII stars, our flux estimate is comparable to the diffuse neutrino flux produced by the ordinary stars and by the ordinary core-collapse supernovae in the universe, i.e. of order 1-10 cm^(-2) s^(-1). Due to the large cosmic redshift, however, the typical energies are in the MeV and sub-MeV range where the solar and geophysical neutrino fluxes are much larger. A direct detection of the diffuse cosmic flux is out of the question with presently known experimental techniques., 17 pages, 7 figures
Published: 2005
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387. Search for chameleons with CAST

Author: J. I. Collar, M. Arik, F.J. Iguaz, Milica Krčmar, Javier Galan, Philippe Brax, José Villar, S. C. Yildiz, Marin Karuza, Julia Vogel, K. Barth, G. Luzón, Biljana Lakić, M. Davenport, M. Kavuk, I. Ortega, Joachim Jacoby, Heinrich Bräuninger, Serkant Ali Cetin, T. Geralis, Georg G. Raffelt, E. Ferrer-Ribas, M. Rosu, H. Riege, T. Papaevangelou, J. G. Garza, Theodoros Vafeiadis, A. Belov, I. G. Irastorza, S. Aune, A. Gardikiotis, Krešimir Jakovčić, F. Haug, I. Savvidis, J. M. Laurent, Dieter H. H. Hoffmann, Peter Friedrich, S. Neff, Charles J. Hailey, M. J. Pivovaroff, Konstantin Zioutas, T. Dafni, Vassilis Anastassopoulos, J. Ruz, I. Giomataris, Klaus Kurt Desch, I. Lavrentyev, Finn Erland Christensen, C. Eleftheriadis, Ante Ljubičić, A. V. Dermenev, A. Upadhye, C. Krieger, Sami K. Solanki, J. M. Carmona, M. D. Hasinoff, Georgios Fanourakis, G. Cantatore, Evangelos Gazis, Jochen Kaminski, Anders Clemen Jakobsen, A. Krüger, A. Liolios, J. A. Garcia, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Anastassopoulos, V, Arik, M., Aune, S., Barth, K., Belov, A., Bräuninger, H., Cantatore, Giovanni, Carmona, J. M., Cetin, S. A., Christensen, F., Collar, J. I., Dafni, T., Davenport, M., Desch, K., Dermenev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Friedrich, P., Galán, J., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Giomataris, I., Hailey, C., Haug, F., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakobsen, A., Jakovčić, K., Kaminski, J., Karuza, M., Kavuk, M., Krčmar, M., Krieger, C., Krüger, A., Lakić, B., Laurent, J. M., Liolios, A., Ljubičić, A., Luzón, G., Neff, S., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Riege, H., Rosu, M., Ruz, J., Savvidis, I., Solanki, S. K., Vafeiadis, T., Villar, J. A., Vogel, J. K., Yildiz, S. C., Zioutas, K., Brax, P., Lavrentyev, I., and Upadhye, A.
Subjects: Nuclear and High Energy Physics, Astrophysics and Astronomy, Photon, Physics - Instrumentation and Detectors, Physics::Instrumentation and Detectors, FOS: Physical sciences, Tachocline, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, 01 natural sciences, SDD, X-ray, High Energy Physics - Phenomenology (hep-ph), 0103 physical sciences, Chameleon, Dark energy, 010306 general physics, Axion, Solar and Stellar Astrophysics (astro-ph.SR), Primakoff effect, Coupling constant, Coupling, Physics, CAST, 010308 nuclear & particles physics, Instrumentation and Detectors (physics.ins-det), lcsh:QC1-999, High Energy Physics - Phenomenology, Astrophysics - Solar and Stellar Astrophysics, CERN Axion Solar Telescope, lcsh:Physics
Abstract: In this work we present a search for (solar) chameleons with the CERN Axion Solar Telescope (CAST). This novel experimental technique, in the field of dark energy research, exploits both the chameleon coupling to matter ($\beta_{\rm m}$) and to photons ($\beta_{\gamma}$) via the Primakoff effect. By reducing the X-ray detection energy threshold used for axions from 1$\,$keV to 400$\,$eV CAST became sensitive to the converted solar chameleon spectrum which peaks around 600$\,$eV. Even though we have not observed any excess above background, we can provide a 95% C.L. limit for the coupling strength of chameleons to photons of $\beta_{\gamma}\!\lesssim\!10^{11}$ for $1, Comment: 8 pages, 12 figures
Published: 2015
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388. The IAXO Helioscope

Author: I. Savvidis, I. G. Irastorza, I. Ortega, Toyokazu Sekiguchi, K Saikawa, M. Davenport, Serkant Ali Cetin, C. Eleftheriadis, C. Krieger, D. Chelouche, O. Limousin, Charles J. Hailey, P. Vedrine, G. Fanourakis, S. Caspi, Gianpaolo Carosi, Javier Redondo, A. Tomás, Ioannis Giomataris, Javier Galan, Hector Gomez, Pierre Sikivie, A.C. Jakobsen, S. Russenschuck, J. G. Garza, F.J. Iguaz, Kenichi Imai, K. van Bibber, Pierre Brun, Marin Karuza, A. Dael, Takashi Hiramatsu, S. Gninenko, A. Lindner, M. Betz, Dieter H. H. Hoffmann, A. Liolios, Jochen Kaminski, E. Ferrer Ribas, Theodoros Geralis, V. N. Muratova, Julia Vogel, Yannis K. Semertzidis, Theodoros Vafeiadis, Babette Döbrich, Sergey Troitsky, G. Luzón, A. V. Derbin, D. González-Díaz, Michael J. Pivovaroff, F. T. Avignone, J. A. Garcia, Joerg Jaeckel, Amanda Weltman, W. C. Wester, Georg G. Raffelt, Masahiro Kawasaki, A. Dudarev, Andreas Ringwald, Krešimir Jakovčić, T. Dafni, Milica Krčmar, J.A. Villar, A. Diago, Eduardo Guendelman, Konstantin Zioutas, Dieter Horns, Klaus Kurt Desch, J. Ruz, J. M. Carmona, Giovanni Cantatore, Benito Gimeno, F.E. Christensen, P. Brax, T. Papaevangelou, L. Walckiers, Jordi Isern, Konstantinos Kousouris, I. Dratchnev, I. Shilon, Fritz Caspers, C. Nones, S. Matsuki, S. C. Yildiz, Biljana Lakić, H. H. J. ten Kate, E. Armengaud, H. Silva, Ribas, E. Ferrer, Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, Giovanni, Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Dael, A., Dafni, T., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Galán, J., García, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., González Diaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G., Isern, J., Imai, K., Jaeckel, J., Jakobsen, A. C., Jakovčić, K., Kaminski, J., Kawasaki, M., Karuza, M., Krčmar, M., Kousouris, K., Krieger, C., Lakić, B., Limousin, O., Lindner, A., Liolios, A., Luzón, G., Matsuki, S., Muratova, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Ten Kate, H. H. J., Tomas, A., Troitsky, S., Vafeiadis, T., Van Bibber, K., Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., Zioutas, K., Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, and Çetin, Serkant Ali
Subjects: History, Particle physics, QCD axion, Dark matter, X-ray optics, Detectable Signal, 7. Clean energy, magnetic helioscope, dark matter, Education, Solar tracker, Optics, QCD axions, ddc:530, Detectors and Experimental Techniques, Axion, Physics, Helioscope, Fourth Generation, business.industry, Technical Design, Detector, MicroMegas detector, Toroidal Magnets, Low Background Detectors, Computer Science Applications, Magnet, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Feasibility Studies, X-ray Focusing Optics, business
Abstract: Çetin, Serkant Ali (Dogus Author) -- Conference full title: 7th International Symposium on Large TPCs for Low-Energy Rare Event Detection; Institute of Astroparticle Physics (APC) Campus - Paris Diderot UniversityParis; France; 15 December 2014 through 17 December 2014 The IAXO (International Axion Experiment) is a fourth generation helioscope with a sensitivity, in terms of detectable signal counts, at least 104 better than CAST phase-I, resulting in sensitivity on gaγ one order of magnitude better. To achieve this performance IAXO will count on a 8-coil toroidal magnet with 60 cm diameter bores and equipped with X-ray focusing optics into 0.20 cm2 spots coupled to ultra-low background Micromegas X-ray detectors. The magnet will be on a platform that will allow solar tracking for 12 hours per day. The next short term objectives are to prepare a Technical Design Report and to construct the first prototypes of the hardware main ingredients: demonstration coil, X-ray optics and low background detector while refining the physics case and studying the feasibility studies for Dark Matter axions.
Published: 2015
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389. Conceptual design of the International Axion Observatory (IAXO)

Author: A. Liolios, P. Vedrine, G. Fanourakis, Doron Chelouche, Klaus Kurt Desch, Serkant Ali Cetin, I. G. Irastorza, Konstantin Zioutas, Gianpaolo Carosi, Javier Redondo, I. Dratchnev, Ken'ichi Saikawa, Ioannis Giomataris, B. Gimeno, Pierre Brun, Eduardo Guendelman, A. Dael, B. Döbrich, S. Gninenko, E. Ferrer-Ribas, C. Krieger, L. Walckiers, J. Ruz, J. A. García, S. Matsuki, Milica Krčmar, I. Shilon, S. Russenschuck, Kenichi Imai, J.A. Villar, I. Ortega, A. Diago, J. Galán, Sergey Troitsky, V. N. Muratova, Joerg Jaeckel, I. Savvidis, Ph. Brax, Amanda Weltman, H. Silva, C. Nones, Charles J. Hailey, Haley Louise Gomez, Dieter Horns, K. van Bibber, Krešimir Jakovčić, S. C. Yildiz, Olivier Limousin, Jordi Isern, Finn Erland Christensen, T. Vafeiadis, William Wester, C. Eleftheriadis, Michael J. Pivovaroff, Theodoros Geralis, Biljana Lakić, Julia Vogel, A. Dudarev, Andreas Ringwald, Fritz Caspers, A. V. Derbin, K. Kousouris, G. Luzón, T. Papaevangelou, J. M. Carmona, J. Kaminski, Anders Clemen Jakobsen, H. H. J. ten Kate, T. Dafni, A. Lindner, M. Betz, Georg G. Raffelt, Marin Karuza, S. Caspi, Masahiro Kawasaki, Giovanni Cantatore, Eric Armengaud, J. G. Garza, F.J. Iguaz, F. T. Avignone, A. Tomás, T. Sekiguchi, M. Davenport, Pierre Sikivie, Takashi Hiramatsu, Dieter H. H. Hoffmann, Diego González-Díaz, Yannis K. Semertzidis, Doğuş Üniversitesi, Fen Edebiyat Fakültesi, Fizik Bölümü, TR3959, Çetin, Serkant Ali, Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, Giovanni, Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Dael, A., Dafni, T., Davenport, M., Derbin, A. V., Desch, K., Diago, A., Döbrich, B., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer Ribas, E., Galán, J., García, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gómez, H., Gonźlez Díaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Irastorza, I. G, Isern, J., Imai, K., Jakobsen, A. C., Jaeckel, J., Jakovčić, K., Kaminski, J., Kawasaki, M., Karuza, M., Krčmar, M., Kousouris, K., Krieger, C., Lakić, B., Limousin, O., Lindner, A., Liolios, A., Luzón, G., Matsuki, S., Muratova, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Kate, H. Ten, Tomas, A., Troitsky, S., Vafeiadis, T., Bibber, K. Van, Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., and Zioutas, K.
Subjects: MICROPIC, Physics - Instrumentation and Detectors, Photon, axions, Parameter space, 7. Clean energy, High Energy Physics - Experiment, Dark Matter detectors (WIMPs, axions, etc.), High Energy Physics - Experiment (hep-ex), Observatory, etc.), Micropattern gaseous detectors (MSGC, GEM, THGEM, RETHGEM, MHSP, MICROPIC, MICROMEGAS, InGrid, etc), Detectors and Experimental Techniques, Instrumentation, Mathematical Physics, Physics, GEM, solar [axion], Dark Matter Detectors (Wimps, Axions, etc.), MicroMegas detector, X-ray detectors, Instrumentation and Detectors (physics.ins-det), Large detector systems for particle and astroparticle physics, solar, observatory, MICROMEGAS, MHSP, axion-like particles, proposed experiment, dark matter detectors, x-ray detectors, Micropattern gaseous detectors, large detector systems for particle and astroparticle physics, Micromegas, X-ray detector, Particle physics, optics [X-ray], FOS: Physical sciences, Superconducting magnet, Micropattern gaseous detectors (MSGC, ddc:610, Axion, activity report, Dark Matter detectors (WIMPs, superconductivity [magnet], etc), Helioscope, sensitivity, InGrid, RETHGEM, Orders of magnitude (time), axion, Large detector systems for particle and astroparticle physic, THGEM, Micropattern Gaseous Detectors (MSGC, Gem, THGEM, Rethgem, MHSP, Micropic, Micromegas, In Grid
Abstract: The International Axion Observatory (IAXO) will be a forth generation axion helioscope. As its primary physics goal, IAXO will look for axions or axion-like particles (ALPs) originating in the Sun via the Primakoff conversion of the solar plasma photons. In terms of signal-to-noise ratio, IAXO will be about 4-5 orders of magnitude more sensitive than CAST, currently the most powerful axion helioscope, reaching sensitivity to axion-photon couplings down to a few $\times 10^{-12}$ GeV$^{-1}$ and thus probing a large fraction of the currently unexplored axion and ALP parameter space. IAXO will also be sensitive to solar axions produced by mechanisms mediated by the axion-electron coupling $g_{ae}$ with sensitivity $-$for the first time$-$ to values of $g_{ae}$ not previously excluded by astrophysics. With several other possible physics cases, IAXO has the potential to serve as a multi-purpose facility for generic axion and ALP research in the next decade. In this paper we present the conceptual design of IAXO, which follows the layout of an enhanced axion helioscope, based on a purpose-built 20m-long 8-coils toroidal superconducting magnet. All the eight 60cm-diameter magnet bores are equipped with focusing x-ray optics, able to focus the signal photons into $\sim 0.2$ cm$^2$ spots that are imaged by ultra-low-background Micromegas x-ray detectors. The magnet is built into a structure with elevation and azimuth drives that will allow for solar tracking for $\sim$12 h each day., Comment: 47 pages, submitted to JINST
Published: 2014
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390. Search for Sub-eV Mass Solar Axions by the CERN Axion Solar Telescope with (3)He Buffer Gas

Author: M, Arik, S, Aune, K, Barth, A, Belov, S, Borghi, H, Bräuninger, G, Cantatore, J M, Carmona, S A, Cetin, J I, Collar, T, Dafni, M, Davenport, C, Eleftheriadis, N, Elias, C, Ezer, G, Fanourakis, E, Ferrer-Ribas, P, Friedrich, J, Galán, J A, García, A, Gardikiotis, E N, Gazis, T, Geralis, I, Giomataris, S, Gninenko, H, Gómez, E, Gruber, T, Guthörl, R, Hartmann, F, Haug, M D, Hasinoff, D H H, Hoffmann, F J, Iguaz, I G, Irastorza, J, Jacoby, K, Jakovčić, M, Karuza, K, Königsmann, R, Kotthaus, M, Krčmar, M, Kuster, B, Lakić, J M, Laurent, A, Liolios, A, Ljubičić, V, Lozza, G, Lutz, G, Luzón, J, Morales, T, Niinikoski, A, Nordt, T, Papaevangelou, M J, Pivovaroff, G, Raffelt, T, Rashba, H, Riege, A, Rodríguez, M, Rosu, J, Ruz, I, Savvidis, P S, Silva, S K, Solanki, L, Stewart, A, Tomás, M, Tsagri, K, van Bibber, T, Vafeiadis, J A, Villar, J K, Vogel, S C, Yildiz, K, Zioutas, Arik, M., Aune, S., Barth, K., Belov, A., Borghi, S., Brauninger, H., Cantatore, Giovanni, Carmona, J. M., Cetin, S. A., Collar, J. I., Dafni, T., Davenport, M., Eleftheriadis, C., Elias, N., Ezer, C., Fanourakis, G., Ferrer Ribas, E., Friedrich, P., Galan, J., Garcia, J. A., Gardikiotis, A., Gazis, E. N., Geralis, T., Giomataris, I., Gninenko, S., Gomez, H., Gruber, E., Guthorl, T., Hartmann, R., Haug, F., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jacoby, J., Jakovcic, K., Karuza, M., Konigsmann, K., Kotthaus, R., Krcmar, M., Kuster, M., Lakic, B., Laurent, J. M., Liolios, A., Ljubicic, A., Lozza, Valentina, Lutz, G., Luzon, G., Morales, J., Niinikoski, T., Nordt, A., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Rashba, T., Riege, H., Rodriguez, A., Rosu, M., Ruz, J., Savvidis, I., Silva, P. S., Solanki, S. K., Stewart, L., Tomas, A., Tsagri, M., van Bibber, K., Vafeiadis, T., Villar, J. A., Vogel, J. K., Yildiz, S. C., and Zioutas, K.
Subjects: solar axion, low background detectors, solar axions, photons, dark matter
Abstract: The CERN Axion Solar Telescope (CAST) has extended its search for solar axions by using (3)He as a buffer gas. At T=1.8 K this allows for larger pressure settings and hence sensitivity to higher axion masses than our previous measurements with (4)He. With about 1 h of data taking at each of 252 different pressure settings we have scanned the axion mass range 0.39 eV≲m(a)≲0.64 eV. From the absence of excess x rays when the magnet was pointing to the Sun we set a typical upper limit on the axion-photon coupling of g(aγ)≲2.3×10(-10) GeV(-1) at 95% C.L., the exact value depending on the pressure setting. Kim-Shifman-Vainshtein-Zakharov axions are excluded at the upper end of our mass range, the first time ever for any solar axion search. In the future we will extend our search to m(a)≲1.15 eV, comfortably overlapping with cosmological hot dark matter bounds.
Published: 2011

391. Indirect Searches for Gravitino Dark Matter

Author: Michael Grefe, Grefe, M., Oberauer, L., Raffelt, G., Wagner, R., and UAM. Departamento de Física Teórica
Subjects: History, Particle physics, Astrophysics::High Energy Astrophysical Phenomena, Dark matter, FOS: Physical sciences, Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, Education, General Relativity and Quantum Cosmology, Positron, High Energy Physics - Phenomenology (hep-ph), Big Bang nucleosynthesis, 0103 physical sciences, ddc:530, 010303 astronomy & astrophysics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, High Energy Physics::Phenomenology, Gamma ray, Física, Computer Science Applications, High Energy Physics - Phenomenology, 13. Climate action, Antiproton, Leptogenesis, Gravitino, High Energy Physics::Experiment, Neutrino, Astrophysics - High Energy Astrophysical Phenomena
Abstract: The gravitino in models with a small violation of R-parity is a well-motivated decaying dark matter candidate that leads to a cosmological scenario that is consistent with big bang nucleosynthesis and thermal leptogenesis. The gravitino lifetime is cosmologically long-lived since its decays are suppressed by the Planck-scale as well as the small R-parity violating parameter. We discuss the signals in different cosmic-ray species coming from the decay of gravitino dark matter, namely gamma rays, positrons, antiprotons, antideuterons and neutrinos. Comparison to cosmic-ray data can be used to constrain the parameters of the model., Comment: 4 pages, 15 figures; to appear in the proceedings of the 12th International Conference on Topics in Astroparticle and Underground Physics (TAUP 2011), Munich, Germany, 5-9 September 2011
Published: 2011
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392. Comment on axion emission rates in stars

Author: Raffelt, G
Published: 1986
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393. Horizontal branch stars and the neutrino signal from SN 1987A

Author: Raffelt, G
Published: 1988
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394. Astrophysical axion bounds diminished by screening effects

Author: Raffelt, G
Published: 1986
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395. Design for a practical laboratory detector for solar axions

Author: Raffelt, G
Published: 1989
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396. Neutrino oscillation experiments at accelerators and reactors

Author: Jürgen Brunner, Centre de Physique des Particules de Marseille (CPPM), Aix Marseille Université (AMU)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Berezinsky V. Raffelt G. Valle J.W.F., ANTARES, and Damoiseaux, Magali
Subjects: Physics, Nuclear and High Energy Physics, Particle physics, [PHYS.HEXP] Physics [physics]/High Energy Physics - Experiment [hep-ex], 010308 nuclear & particles physics, Solar neutrino problem, CHOOZ, 01 natural sciences, Atomic and Molecular Physics, and Optics, Nuclear physics, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Neutrino, 010306 general physics, Baseline (configuration management), Neutrino oscillation, KARMEN
Abstract: A whole generation of neutrino experiments at artificial neutrino sources has recently finished data taking. CHORUS and NOMAD took their last data in 1997 and 1998 respectively. LSND and Chooz stopped running in 1998 and Palo Verde will switch off in 1999. Only Karmen will continue to take data until 2001. Final or preliminary results of all these experiments will be reviewed. Two future short baseline accelerator projects - Boone and I216 - will be presented which address the verification of the LSND result. The Kamland project - a very long baseline reactor experiment - will be described as well.
Published: 1999

397. Electroweak lights from Dark Matter annihilations

Author: Andrea De Simone, Oberauer, L, Raffelt, G, and Wagner, R
Subjects: Physics, History, Gauge boson, Particle physics, Annihilation, High Energy Physics::Phenomenology, Electroweak interaction, Dark matter, FOS: Physical sciences, Fermion, Computer Science Applications, Education, Standard Model, High Energy Physics - Phenomenology, MAJORANA, High Energy Physics - Phenomenology (hep-ph), Particle
Abstract: The energy spectra of Standard Model particles originated from Dark Matter annihilations can be significantly altered by the inclusion of electroweak gauge boson radiation from the final state. A situation where this effect is particularly important is when a Majorana Dark Matter particle annihilates into two light fermions. This process is in p-wave and hence suppressed by the small value of the relative velocity of the annihilating particles. The inclusion of electroweak radiation eludes this suppression and opens up a potentially sizeable s-wave contribution to the annihilation cross section. I will discuss the impact of this effect on the fluxes of stable particles resulting from the Dark Matter annihilations, which are relevant for Dark Matter indirect searches., 4 pages, 2 figures. Contribution to the conference proceedings of TAUP 2011, Munich - Germany (5-9 September 2011)
Published: 2012
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398. Improved search for solar chameleons with a GridPix detector at CAST

Author: Wolfgang Funk, Milica Krčmar, T. Geralis, M. Maroudas, S. C. Yildiz, I. G. Irastorza, Joachim Jacoby, Sofia Kostoglou, Babette Döbrich, Sergei Gninenko, Giovanni Cantatore, C. Krieger, Søren Schmidt, M. Davenport, Marin Karuza, I. Ortega, M. J. Pivovaroff, Konstantin Zioutas, C. J. Hailey, J. Ruz, S. Neff, L. Miceli, T. Papaevangelou, S. Aune, Georg G. Raffelt, T. Dafni, I. Savvidis, M. Vretenar, Klaus Kurt Desch, Biljana Lakić, A. Liolios, Georgios Fanourakis, Nenad Kralj, Alexander Dermenev, J. F. Castel, A. Belov, Krešimir Jakovčić, L. Stewart, Dieter Hoffmann, Sami K. Solanki, Heinrich Bräuninger, Serkant Ali Cetin, E. Ruiz Chóliz, F.J. Iguaz, Vassilis Anastassopoulos, H. Fischer, A. Gardikiotis, Yannis K. Semertzidis, M. D. Hasinoff, C. Eleftheriadis, Jochen Kaminski, Anders Clemen Jakobsen, K. Paraschou, E. Ferrer-Ribas, J. M. Carmona, Julia Vogel, Theodoros Vafeiadis, J. G. Garza, K. Barth, G. Luzón, Walter Wuensch, I. Giomataris, M. Rosu, P. Brax, Ante Ljubičić, J. M. Laurent, J. A. Garcia, Evangelos Gazis, Finn Erland Christensen, Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Institut de Physique Théorique - UMR CNRS 3681 (IPHT), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), CAST, Anastassopoulos, V., Aune, S., Barth, K., Belov, A., Bräuninger, H., Cantatore, G., Carmona, J. M., Castel, J. F., Cetin, S. A., Christensen, F., Dafni, T., Davenport, M., Dermenev, A., Desch, K., Döbrich, B., Eleftheriadis, C., Fanourakis, G., Ferrer-Ribas, E., Fischer, H., Funk, W., García, J. A., Gardikiotis, A., Garza, J. G., Gazis, E. N., Geralis, T., Giomataris, I., Gninenko, S., Hailey, C. J., Hasinoff, M. D., Hoffmann, D. H. H., Iguaz, F. J., Irastorza, I. G., Jakobsen, A., Jacoby, J., Jakovčić, K., Kaminski, J., Karuza, M., Kostoglou, S., Kralj, N., Krčmar, M., Krieger, C., Lakić, B., Laurent, J. M., Liolios, A., Ljubičić, A., Luzón, G., Maroudas, M., Miceli, L., Neff, S., Ortega, I., Papaevangelou, T., Paraschou, K., Pivovaroff, M. J., Raffelt, G., Rosu, M., Ruz, J., Chóliz, E. Ruiz, Savvidis, I., Schmidt, S., Semertzidis, Y. K., Solanki, S. K., Stewart, L., Vafeiadis, T., Vogel, J. K., Vretenar, M., Wuensch, W., Yildiz, S. C., Zioutas, K., and Brax, P.
Subjects: Physics - Instrumentation and Detectors, Photon, Physics::Instrumentation and Detectors, Solar luminosity, magnetic field, Astrophysics, 01 natural sciences, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), photon: coupling, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Astrophysics::Solar and Stellar Astrophysics, Detectors and Experimental Techniques, GridPix, dark energy, modified gravity, physics.ins-det, Solar physics, Physics, dark energy experiments, particle physics - cosmology connection, solar physics, Astronomy and Astrophysics, chameleon: solar, solar physic, Instrumentation and Detectors (physics.ins-det), Coupling (probability), transition: (axion photon), dark energy experiment, Beta (plasma physics), Physics::Space Physics, CAST, Astrophysics::Earth and Planetary Astrophysics, CERN Axion Solar Telescope, Particle Physics - Experiment, chameleon, Modified gravity, Particle physics, CERN Lab, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, photon: spectrum, coupling constant: upper limit, Tachocline, Astrophysics::Cosmology and Extragalactic Astrophysics, X-ray, Dark energy experiments, 0103 physical sciences, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Sensitivity (control systems), hep-ex, background, 010308 nuclear & particles physics, magnet, coupling: (axion 2photon), Particle physics - cosmology connection, axion: solar, tachocline, Energy (signal processing), experimental results
Abstract: We report on a new search for solar chameleons with the CERN Axion Solar Telescope (CAST). A GridPix detector was used to search for soft X-ray photons in the energy range from 200 eV to 10 keV from converted solar chameleons. No signiffcant excess over the expected background has been observed in the data taken in 2014 and 2015. We set an improved limit on the chameleon photon coupling, $\beta_\gamma < 5.7\times10^{10}$ for $1, Comment: 19 pages, 12 figures, 3 tables
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399. Fast Neutrino Flavor Conversions Can Help and Hinder Neutrino-Driven Explosions.

Author: Ehring J, Abbar S, Janka HT, Raffelt G, and Tamborra I
Abstract: We present the first simulations of core-collapse supernovae in axial symmetry with feedback from fast neutrino flavor conversion (FFC). Our schematic treatment of FFCs assumes instantaneous flavor equilibration under the constraint of lepton-number conservation individually for each flavor. Systematically varying the spatial domain where FFCs are assumed to occur, we find that they facilitate SN explosions in low-mass (9-12M_{⊙}) progenitors that otherwise explode with longer time delays, whereas FFCs weaken the tendency to explode of higher-mass (around 20M_{⊙}) progenitors.
Published: 2023
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400. Low-Energy Supernovae Severely Constrain Radiative Particle Decays.

Author: Caputo A, Janka HT, Raffelt G, and Vitagliano E
Abstract: The hot and dense core formed in the collapse of a massive star is a powerful source of hypothetical feebly interacting particles such as sterile neutrinos, dark photons, axionlike particles (ALPs), and others. Radiative decays such as a→2γ deposit this energy in the surrounding material if the mean free path is less than the radius of the progenitor star. For the first time, we use a supernova (SN) population with particularly low explosion energies as the most sensitive calorimeters to constrain this possibility. These SNe are observationally identified as low-luminosity events with low ejecta velocities and low masses of ejected ^{56}Ni. Their low energies limit the energy deposition from particle decays to less than about 0.1 B, where 1 B(bethe)=10^{51} erg. For 1-500 MeV-mass ALPs, this generic argument excludes ALP-photon couplings G_{aγγ} in the 10^{-10}-10^{-8} GeV^{-1} range.
Published: 2022
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