Results 11 to 20 of about 3,021 (33)
Gamma Ray Constraints on Flavor Violating Asymmetric Dark Matter
, 2012 We show how cosmic gamma rays can be used to constrain models of asymmetric
Dark Matter decaying into lepton pairs by violating flavor. First of all we
require the models to explain the anomalies in the charged cosmic rays measured
by PAMELA, FERMI and ..., , A. Ibarra, A. Ibarra, C.-R. Chen, E. Nardi, Fermi-LAT collaboration, Fermi-LAT collaboration, Francesco Sannino, G. Bertone, I. Masina, I.V. Moskalenko, Isabella Masina, M. Ackermann, M. Cirelli ., M. Papucci, MAGIC collaboration, P. Ciafaloni ., Paolo Panci, see also: I. Masina, X. Huang +20 morecore +1 more sourceIceCube-Gen2: A Vision for the Future of Neutrino Astronomy in
Antarctica [PDF]
, 2014 The recent observation by the IceCube neutrino observatory of an
astrophysical flux of neutrinos represents the "first light" in the nascent
field of neutrino astronomy.:, Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., Altmann, D., andaz-Vélez, J. C. Dí, Anderson, T., andić, andl, A. Stöß, Anton, G., Arguelles, C., Arlen, T. C., Auffenberg, J., Axani, S., Bai, X., Bartos, I., Barwick, S. W., Baum, V., Bay, R., Beatty, J. J., Becker, K. -H., BenZvi, S., Berghaus, P., Berley, D., Bernardini, E., Bernhard, A., Besson, D. Z., Binder, G., Bindig, D., Bissok, M., Blaufuss, E., Blumenthal, J., Boersma, D. J., Bohm, C., Bos, F., Bose, D., Botner, O., Brayeur, L., Bretz, H. -P., Brown, A. M., Buzinsky, N., Böser, S., Casey, J., Casier, M., Cheung, E., Chirkin, D., Christov, A., Christy, B., Clark, K., Classen, L., Clevermann, F., Coenders, S., Collaboration, IceCube-Gen2, Collin, G. H., Conrad, J. M., Cowen, D. F., Daughhetee, J., Davis, J. C., Day, M., de André, J. P. A. M., De Clercq, C., De Ridder, S., de Vries, K. D., de With, M., Desiati, P., DeYoung, T., Dunkman, M., Eagan, R., Eberhardt, B., Ehrhardt, T., Eichmann, B., Eisch, J., Euler, S., Evans, J. J., Evenson, P. A., Fadiran, O., Fazely, A. R., Fedynitch, A., Feintzeig, J., Felde, J., Filimonov, K., Finley, C., Fischer-Wasels, T., Flis, S., Frantzen, K., Fuchs, T., Gaior, R., Gaisser, T. K., Gallagher, J., Gerhardt, L., Gier, D., Gladstone, L., Glüsenkamp, T., Goldschmidt, A., Golup, G., Gonzalez, J. G., Goodman, J. A., Grant, D., Gretskov, P., Groh, J. C., Groß, A., Góra, D., Ha, C., Haack, C., Hallen, P., Hallgren, A., Halzen, F., Hanson, K., Haugen, J., Hebecker, D., Heereman, D., Heinen, D., Helbing, K., Hellauer, R., Hellwig, D., Heros, C. Pérez de los, Hickford, S., Hignight, J., Hill, G. C., Hoffman, K. D., Hoffmann, R., Homeier, A., Hoshina, K., Huang, F., Huelsnitz, W., Hulth, P. O., Hultqvist, K., Ishihara, A., Ismail, A. Haj, Jacobi, E., Jacobsen, J., Japaridze, G. S., Jero, K., Jlelati, O., Jones, B. J. P., Jurkovic, M., Kalekin, O., Kappes, A., Karg, T., Karle, A., Katori, T., Katz, U. F., Kauer, M., Keivani, A., Kelley, J. L., Kheirandish, A., Kiryluk, J., Klein, S. R., Kläs, J., Kohnen, G., Kolanoski, H., Koob, A., Kopper, C., Kopper, S., Koskinen, D. J., Kowalski, M., Krauss, C. B., Kriesten, A., Krings, K., Kroll, G., Kroll, M., Kunnen, J., Kurahashi, N., Kuwabara, T., Köhne, J. -H., Köpke, L., Labare, M., Lanfranchi, J. L., Larsen, D. T., Larson, M. J., Lesiak-Bzdak, M., Leuermann, M., LoSecco, J., Lünemann, J., Madsen, J., Maggi, G., Mahn, K. B. M., Marka, S., Marka, Z., Maruyama, R., Mase, K., Matis, H. S., Maunu, R., McNally, F., Meagher, K., Medici, M., Meli, A., Meures, T., Miarecki, S., Middell, E., Middlemas, E., Milke, N., Miller, J., Mohrmann, L., Montaruli, T., Moore, R. W., Morse, R., Nahnhauer, R., Naumann, U., Niederhausen, H., Nowicki, S. C., Nygren, D. R., O'Murchadha, A., Obertacke, A., Odrowski, S., Olivas, A., Omairat, A., Palczewski, T., Paul, L., Penek, Ö., Pepper, J. A., Pfendner, C., Pieloth, D., Pinat, E., Pinfold, J. L., Posselt, J., Price, P. B., Przybylski, G. T., Pütz, J., Quinnan, M., Rameez, M., Rawlins, K., Redl, P., Rees, I., Reimann, R., Relich, M., Resconi, E., Rhode, W., Richman, M., Riedel, B., Robertson, S., Rodrigues, J. P., Rongen, M., Rott, C., Ruhe, T., Ruzybayev, B., Ryckbosch, D., Rädel, L., Saba, S. M., Sander, H. -G., Sandroos, J., Sandstrom, P., Santander, M., Sarkar, S., Schatto, K., Scheriau, F., Schmidt, T., Schmitz, M., Schoenen, S., Schukraft, A., Schulte, L., Schulz, O., Schöneberg, S., Schönwald, A., Seckel, D., Sestayo, Y., Seunarine, S., Shaevitz, M. H., Shanidze, R., Silva, A. H. Cruz, Smith, M. W. E., Soldin, D., Spiczak, G. M., Spiering, C., Stamatikos, M., Stanev, T., Stanisha, N. A., Stasik, A., Stezelberger, T., Stokstad, R. G., Strahler, E. A., Strotjohann, N. L., Ström, R., Sullivan, G. W., Söldner-Rembold, S., Taavola, H., Taboada, I., Taketa, A., Tamburro, A., Tanaka, H. K. M., Tepe, A., Ter-Antonyan, S., Terliuk, A., Teš, G., Tilav, S., Tjus, J. Becker, Toale, P. A., Tobin, M. N., Tosi, D., Tselengidou, M., Unger, E., Usner, M., Vallecorsa, S., van Eijndhoven, N., van Santen, J., Vandenbroucke, J., Vanheule, S., Vehring, M., Voge, M., Vraeghe, M., Walck, C., Wallraff, M., Weaver, Ch., Wellons, M., Wendt, C., Westerhoff, S., Whelan, B. J., Whitehorn, N., Wichary, C., Wiebe, K., Wiebusch, C. H., Williams, D. R., Wissing, H., Wolf, M., Wood, T. R., Woschnagg, K., Wren, S., Xu, D. L., Xu, X. W., Xu, Y., Yanez, J. P., Yodh, G., Yoshida, S., Zarzhitsky, P., Ziemann, J., Zoll, M. +328 morecore +1 more sourceMeasuring the neutron star equation of state using X-ray timing [PDF]
, 2016 One of the primary science goals of the next generation of hard X-ray timing
instruments is to determine the equation of state of the matter at supranuclear
densities inside neutron stars, by measuring the radius of neutron stars with
different masses to Andersson, Nils, Chakrabarty, Deepto, Feroci, Marco, Hebeler, Kai, Israel, Gianluca, Lamb, Frederick K., Miller, M. Coleman, Morsink, Sharon, Patruno, Alessandro, Poutanen, Juri, Psaltis, Dimitrios, Schwenk, Achim, Steiner, Andrew W., Stella, Luigi, Tolos, Laura, van der Klis, Michiel, Watts, Anna L., Özel, Feryal +17 morecore +6 more sourcesGalaxy Clusters as Reservoirs of Heavy Dark Matter and High-Energy
Cosmic Rays: Constraints from Neutrino Observations
, 2013 Galaxy Clusters (GCs) are the largest reservoirs of both dark matter and
cosmic rays (CRs). Dark matter self-annihilation can lead to a high luminosity
in gamma rays and neutrinos, enhanced by a strong degree of clustering in dark
matter substructures ...A. Hektor, A. Strumia, A. Vladimirov, A.M. Green, A.V. Kravtsov, B. Wolfe, C. Weniger, D. Kushnir, D. Kushnir, D. Ryu, E. Tempel, F. Miniati ., F. Zwicky, Fermi-LAT collaboration, Fermi-LAT collaboration, G. Brunetti ., H. Kang, H. Kang, H. Takami, HESS collaboration, IceCube collaboration, IceCube collaboration, IceCube collaboration, J. Diemand, J. Einasto, J. Han, J.D. Finke, J.F. Beacom, J.F. Navarro, J.F. Navarro, John F Beacom, K. Kotera ., K. Murase, K. Murase, K. Murase, K. Murase, K.N. Abazajian, Kohta Murase, L. Bergstrom, L. Silva, LAT collaboration, M. Ackermann ., M. Kuhlen, M. Su, M.A. Sanchez-Conde, MAGIC collaboration, O. Reimer, O.Y. Gnedin, O.Y. Gnedin ., P. Ciafaloni ., P. Ciafaloni ., P. Martini, P. Sutter, P. Sutter, R. Berrington, S. Ando, S. Gabici, S. Inoue, S. Inoue, S.W. Skillman, T. Bringmann, T. Bringmann, T. Sjöstrand, T. Totani, T.E. Jeltema, U. Keshet, U. Keshet, U. Keshet, V. Berezinsky, Veritas collaboration, X. Huang, Y. Fujita, Y. Fujita +72 morecore +1 more source
