Zobrazeno 1 - 10
of 120
pro vyhledávání: '"Macgibbon, J."'
Autor:
Ali-Haimoud, Y., Clesse, S., Garcia-Bellido, J., Kashlinsky, A., Wyrzykowski, L., Achucarro, A., Amendola, L., Annis, J., Arbey, A., Arendt, R. G., Atrio-Barandela, F., Bellomo, N., Belotsky, K., Bernal, J-L., Bird, S., Bozza, V., Byrnes, C., Novati, S. Calchi, Calore, F., Carr, B. J., Chluba, J., Cholis, I., Cieplak, A., Cole, P., Dalianis, I., Davis, A-C., Davis, T., De Luca, V., Dvorkin, I., Emparan, R., Ezquiaga, J-M., Fleury, P., Franciolini, G., Gaggero, D., Georg, J., Germani, C., Giudice, G-F., Goobar, A., Hasinger, G., Hector, A., Hundertmark, M ., Hutsi, G., Jansen, R., Kamionkowski, M., Kawasaki, M., Kazanas, D., Kehagias, A., Khlopov, M., Knebe, A., Kohri, K., Koushiappas, S., Kovetz, E., Kuhnel, F., MacGibbon, J., Marzola, L., Mediavilla, E., Meszaros, P., Mroz, P., Munoz, J., Musco, I., Nesseris, S., Ozsoy, O., Pani, P., Poulin, V., Raccanelli, A., Racco, D., Raidal, M., Ranc, C., Rattenbury, N., Rhodes, J., Ricotti, M., Riotto, A., Rubin, S., Rubio, J., Ruiz-Morales, E., Sasaki, M., Schnittman, J., Shvartzvald, Y., Street, R., Takada, M., Takhistov, V., Tashiro, H., Tasinato, G., Tringas, G., Unal, C., Tada, Y., Tsapras, Y., Vaskonen, V., Veermae, H., Vidotto, F., Watson, S., Windhorst, R., Yokoyama, S., Young, S.
The LIGO discoveries have rekindled suggestions that primordial black holes (BHs) may constitute part to all of the dark matter (DM) in the Universe. Such suggestions came from 1) the observed merger rate of the BHs, 2) their unusual masses, 3) their
Externí odkaz:
http://arxiv.org/abs/1903.04424
Autor:
Ukwatta, T. N., Hurley, K., MacGibbon, J. H, Svinkin, D. S, Aptekar, R. L, Golenetskii, S. V, Frederiks, D. D, Pal'shin, V. D, Goldsten, J., Boynton, W., Kozyrev, A. S, Rau, A., von Kienlin, A., Zhang, X., Connaughton, V., Yamaoka, K., Ohno, M., Ohmori, N., Feroci, M., Frontera, F., Guidorzi, C., Cline, T., Gehrels, N., Krimm, H. A, McTiernan, J.
The detection of a gamma-ray burst (GRB) in the solar neighborhood would have very important implications for GRB phenomenology. The leading theories for cosmological GRBs would not be able to explain such events. The final bursts of evaporating Prim
Externí odkaz:
http://arxiv.org/abs/1512.01264
Autor:
Ukwatta, T. N., Stump, D. R., Linnemann, J. T., MacGibbon, J. H., Marinelli, S. S., Yapici, T., Tollefson, K.
Many early universe theories predict the creation of Primordial Black Holes (PBHs). PBHs could have masses ranging from the Planck mass to 10^5 solar masses or higher depending on the size of the universe at formation. A Black Hole (BH) has a Hawking
Externí odkaz:
http://arxiv.org/abs/1510.04372
Autor:
Linnemann, J. T., Stump, D., Marinelli, S. S., Yapici, T., Tollefson, K., Ukwatta, T. N., MacGibbon, J. H.
Many early universe theories predict the creation of Primordial Black Holes (PBHs). The PBHs could have masses ranging from the Planck mass to 10^5 solar masses or higher depending on the formation scenario. Hawking showed that any Black Hole (BH) ha
Externí odkaz:
http://arxiv.org/abs/1507.01648
Autor:
Abdo, A. A., Abeysekara, A. U., Alfaro, R., Allen, B. T., Alvarez, C., Álvarez, J. D., Arceo, R., Arteaga-Velázquez, J. C., Aune, T., Solares, H. A. Ayala, Barber, A. S., Baughman, B. M., Bautista-Elivar, N., Gonzalez, J. Becerra, Belmont, E., BenZvi, S. Y., Berley, D., Rosales, M. Bonilla, Braun, J., Caballero-Lopez, R. A., Caballero-Mora, K. S., Carramiñana, A., Castillo, M., Chen, C., Christopher, G. E., Cotti, U., Cotzomi, J., de la Fuente, E., De León, C., DeYoung, T., Hernandez, R. Diaz, Diaz-Cruz, L., Díaz-Vélez, J. C., Dingus, B. L., DuVernois, M. A., Ellsworth, R. W., Fiorino, D. W., Fraija, N., Galindo, A., Garfias, F., González, M. M., Goodman, J. A., Grabski, V., Gussert, M., Hampel-Arias, Z., Harding, J. P., Hays, E., Hoffman, C. M., Hui, C. M., Hüntemeyer, P., Imran, A., Iriarte, A., Karn, P., Kieda, D., Kolterman, B. E., Kunde, G. J., Lara, A., Lauer, R. J., Lee, W. H., Lennarz, D., Vargas, H. León, Linares, E. C., Linnemann, J. T., Longo, M., Luna-GarcIa, R., MacGibbon, J. H., Marinelli, A., Marinelli, S. S., Martinez, H., Martinez, O., Martínez-Castro, J., Matthews, J. A. J., McEnery, J., Torres, E. Mendoza, Mincer, A. I., Miranda-Romagnoli, P., Moreno, E., Morgan, T., Mostafá, M., Nellen, L., Nemethy, P., Newbold, M., Noriega-Papaqui, R., Oceguera-Becerra, T., Patricelli, B., Pelayo, R., Pérez-Pérez, E. G., Pretz, J., Rivière, C., Rosa-González, D., Ryan, J., Salazar, H., Salesa, F., Sandoval, A., Parkinson, P. M. Saz, Schneider, M., Shoup, A., Silich, S., Sinnis, G., Smith, A. J., Stump, D., Woodle, K. Sparks, Springer, R. W., Taboada, I., Toale, P. A., Tollefson, K., Torres, I., Ukwatta, T. N., Vasileiou, V., Villaseñor, L., Walker, G. P., Weisgarber, T., Westerhoff, S., Williams, D. A., Wisher, I. G., Wood, J., Yodh, G. B., Younk, P. W., Zaborov, D., Zepeda, A., Zhou, H.
Publikováno v:
Astroparticle Physics, Volume 64, p. 4-12. 2015
Primordial Black Holes (PBHs) are gravitationally collapsed objects that may have been created by density fluctuations in the early universe and could have arbitrarily small masses down to the Planck scale. Hawking showed that due to quantum effects,
Externí odkaz:
http://arxiv.org/abs/1407.1686
Autor:
Beatty, J. J., Nelson, A. E., Olinto, A., Sinnis, G., Abeysekara, A. U., Anchordoqui, L. A., Aramaki, T., Belz, J., Buckley, J. H., Byrum, K., Cameron, R., Chen, M-C., Clark, K., Connolly, A., Cowen, D., DeYoung, T., Dumm, P. von Doetinchem J., Errando, M., Farrar, G., Ferrer, F., Fortson, L., Funk, S., Grant, D., Griffiths, S., Groß, A., Hailey, C., Hogan, C., Holder, J., Humensky, B., Kaaret, P., Klein, S. R., Krawczynski, H., Krennrich, F., Krings, K., Krizmanic, J., Kusenko, A., Linnemann, J. T., MacGibbon, J. H., Matthews, J., McCann, A., Mitchell, J., Mukherjee, R., Nitz, D., Ong, R. A., Orr, M., Otte, N., Paul, T., Resconi, E., Sanchez-Conde, M. A., Sokolsky, P., Stecker, F., Stump, D., Taboada, I., Thomson, G. B., Tollefson, K., von Doetinchem, P., Ukwatta, T., Vandenbroucke, J., Vasileiou, V., Vassileiv, V. V., Weiler, T. J., Williams, D. A., Weinstein, A., Wood, M., Zitzer, B.
Report of the CF6 Working Group at Snowmass 2013. Topics addressed include ultra-high energy cosmic rays, neutrinos, gamma rays, baryogenesis, and experiments probing the fundamental nature of spacetime.
Comment: Snowmass 2013 CF6 Working Group
Comment: Snowmass 2013 CF6 Working Group
Externí odkaz:
http://arxiv.org/abs/1310.5662
Autor:
Ukwatta, T. U., Stump, D., Linnemann, J. T., Tollefson, K., Vasileiou, V., Sinnis, G., MacGibbon, J. H.
Primordial Black Holes (PBHs) created early in the universe are dark matter candidates. One method of detecting these PBHs is through their Hawking radiation. PBHs created with an initial mass of 5.0 x 10^14 g should be evaporating today with bursts
Externí odkaz:
http://arxiv.org/abs/1308.4912
Autor:
Ukwatta, T. N., MacGibbon, J. H., Parke, W. C., Dhuga, K. S., Eskandarian, A., Gehrels, N., Maximon, L., Morris, D. C.
Publikováno v:
AIP Conf.Proc.1133:440-442,2009
Primordial Black Holes (PBHs), which may have been created in the early Universe, are predicted to be detectable by their Hawking radiation. PBHs with an initial mass of 5.0 * 10^14 g should be expiring today with a burst of high energy particles. Ev
Externí odkaz:
http://arxiv.org/abs/0901.0542
Topological defects, particularly cosmic strings, can provide a mechanism to produce particles with energies of the order 10^21 eV and higher. Here, we report on order of magnitude calculations of fluxes from a cosmic string network which evolves acc
Externí odkaz:
http://arxiv.org/abs/hep-ph/9903545
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