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681“…We show that a subdominant component of dissipative dark matter resembling the Standard Model can form many intermediate-mass black hole seeds during the first structure formation epoch. …”
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682
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683“…Seven observations point towards the existence of primordial black holes (PBH), constituting the whole or an important fraction of the dark matter in the Universe: the mass and spin of black holes detected by Advanced LIGO/VIRGO, the detection of micro-lensing events of distant quasars and stars in M31, the non-detection of ultra-faint dwarf satellite galaxies with radius below 15 parsecs, evidences for core galactic dark matter profiles, the correlation between X-ray and infrared cosmic backgrounds, and the existence of super-massive black holes very early in the Universe's history. …”
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684“…Primordial Black Holes (PBH) arise naturally from high peaks in the curvature power spectrum of near-inflection-point single-field inflation, and could constitute today the dominant component of the dark matter in the universe. …”
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685por de Boer, Jan, Van Breukelen, Rik, Lokhande, Sagar F., Papadodimas, Kyriakos, Verlinde, Erik“…We argue that the region behind the horizon of a one-sided black hole can be probed by an analogue of the double-trace deformation protocol of Gao-Jafferis-Wall. …”
Publicado 2018
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686
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687“…We argue that the infinitely many gauge symmetries of string theory provide an infinite set of conserved (gauge) quantum numbers (W-hair) which characterise black hole states and maintain quantum coherence, even during exotic processes like black hole evaporation/decay. …”
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688
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689
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690por Somjaiuraikul, Narongrit“…The GEMs foil is thin metal-clad polymer foil chemically perforated by a high density of microscopic hole. It uses to exploit electron amplification that occurs within a gas medium inside narrow holes that perforate a thin polyimide foil in a hexagonal pattern. …”
Publicado 2018
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691“…Thus, the tantalizing prospect to test the fundamental nature of gravity with gravitational-wave observations, in a systematic way, emerges naturally. Here, we build black hole solutions in such a framework and study their main properties. …”
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692por Quintin, Jerome, Brandenberger, Robert H., Gasperini, Maurizio, Veneziano, Gabriele“…We discuss the properties of the gas of primordial “stringy” black holes possibly formed in the high-curvature phase preceding the bouncing transition to the phase of standard cosmological evolution. …”
Publicado 2018
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693“…Black holes with masses of |$\rm 10^6\text{-}10^9\,M_{\odot }$| dwell in the centres of most galaxies, but their formation mechanisms are not well known. …”
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694“…We study the sensitivity of pulsar timing arrays (PTAs) to single transiting compact objects, focusing on primordial black holes and compact subhalos in the mass range from 10-12 M⊙ to well above 100 M⊙. …”
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695
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696“…We calculate the emission of gravitational waves, gravitons, photons, and neutrinos from a perturbed Schwarzschild black hole (BH). The perturbation can be due to either classical or quantum sources and therefore the injected energy can be either positive or negative. …”
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697por Kashlinsky, A., Ali-Haimoud, Y., Clesse, S., Garcia-Bellido, J., Wyrzykowski, L., Achucarro, A., Amendola, L., Annis, J., Arbey, A., Arendt, R.G., AtrioBarandela, F., Bellomo, N., Belotsky, K., Bernal, J-L., Bird, S., Bozza, V., Byrnes, C., Calchi Novati, S., 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. …”
Publicado 2019
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698“…We study the spin of primordial black holes produced by the collapse of large inhomogeneities in the early universe. …”
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699“…We study the formation of primordial black holes when they are generated by the collapse of large overdensities in the early universe. …”
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700por Torrente-Lujan, E.“…Mass formulas for multicenter BPS 4D black holes are presented. In the case of two center BPS solutions, the ADM mass can be related to the intercenter distance r , the angular momentum J2 , the dyonic charge vectors qi and the value of the scalar moduli at infinity ( z∞ )by the Smarr-like expression MADM2=A(1+αJ2(1+2MADM/r+A/r2)) where A(Q),α(qi) are symplectic invariant quantities ( Q , the total charge vector) depending on the special geometry prepotential defining the theory. …”
Publicado 2019
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