Zobrazeno 1 - 10
of 109
pro vyhledávání: '"black hole: primordial"'
Autor:
Guillermo Ballesteros, Marcos A.G. García, Alejandro Pérez Rodríguez, Mathias Pierre, Julián Rey
Publikováno v:
Journal of cosmology and astroparticle physics 12(12), 006 (2022). doi:10.1088/1475-7516/2022/12/006
Journal of cosmology and astroparticle physics 12(12), 006 (2022). doi:10.1088/1475-7516/2022/12/006
We study the generation of a localized peak in the primordial spectrum of curvature perturbations from a transient dissipative phase during infl
We study the generation of a localized peak in the primordial spectrum of curvature perturbations from a transient dissipative phase during infl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c47411b71dbe2540dfbe2584f09bc3f0
http://arxiv.org/abs/2208.14978
http://arxiv.org/abs/2208.14978
In this letter we evaluate whether the gravitational wave background recently observed by a number of different pulsar timing arrays could be due to merging primordial supermassive black hole binaries. We find that for homogeneously distributed primo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::c989e5305362b0cec8e85390a353ed8f
In this letter we evaluate whether the gravitational wave background recently observed by a number of different pulsar timing arrays could be due to merging primordial supermassive black hole binaries. We find that for homogeneously distributed primo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ec264cca0eaf336964e2f50d1beb08c0
Autor:
Shakya, Bibhushan
The Standard Model Higgs becomes tachyonic at high energy scales according to current measurements. This unstable regime of the Higgs potential can be realized in the early Universe during high scale inflation, potentially with catastrophic consequen
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::e426c728dcd1ce7310224a2977ad1d44
Autor:
collaboration, H. E. S. S., Aharonian, F., Benkhali, F. Ait, Aschersleben, J., Boettcher, M., Backes, M., Martins, V. Barbosa, Batzo, R., Becherini, Y., Berge, D., Bi, B., Boisson, C., Bolmont, J., de Lavergne, M. de Bony, Borowska, J., Bradascio, F., Brose, R., Brun, F., Bruno, B., Bulik, T., Burger-Scheidlin, C., Caro, S., Casanova, S., Celic, J., Cerruti, M., Chand, T., Chen, A., Chibueze, O., Cotter, G., Mbarubucyeye, J. Damascene, Djannati-Atai, A., Egberts, K., van Eldik, C., Ernenwein, J. -P., Fussling, M., Fiasson, A., de Clairfontaine, G. Fichet, Fontaine, G., Gabici, S., Ghafourizadeh, S., Giavitto, G., Glawion, D., Glicenstein, J. F., Grolleron, G., Grondin, M. -H., Haerer, L., Haupt, M., Hinton, J. A., Hofmann, W., Holler, M., Horns, D., Huang, Zhiqiu, Jamrozy, M., Jankowsky, F., Joshi, V., Jung-Richardt, I., Kasai, E., Katarzynski, K., Khelifi, B., Klepser, S., Kluzniak, W., Komin, Nu., Kosack, K., Kostunin, D., Holch, T. L., Lang, R. G., Stum, S. Le, Leitl, F., Lemiere, A., Lenain, J. -P., Leuschner, F., Lohse, T., Luashvili, A., Lypova, I., Mackey, J., Malyshev, D., Marandon, V., Marchegiani, P., Marinos, P., Marti-Devesa, G., Marx, R., Mitchell, A., Moderski, R., Mohrmann, L., Montanari, A., Moulin, E., Muller, J., Nakashima, K., de Naurois, M., Niemiec, J., O'Brien, P., Ohm, S., Olivera-Nieto, L., Wilhelmi, E. de Ona, Ostrowski, M., Puehlhofer, G., Panny, S., Panter, M., Parsons, R. D., Peron, G., Noel, A. Priyana, Prokhorov, D. A., Prokoph, H., Punch, M., Quirrenbach, A., Reichherzer, P., Reimer, O., Rieger, F., Rowell, G., Rudak, B., Ricarte, H. Rueda, Sahakian, V., Salzmann, H., Sanchez, D. A., Santangelo, A., Sasaki, M., Schutte, H. M., Schwanke, U., Shapopi, J. N. S., Sol, H., Specovius, A., Spencer, S., Stawarz, L., Steenkamp, R., Steinmassl, S., Steppa, C., Sushch, I., Suzuki, H., Takahashi, T., Tanaka, T., Tavernier, T., Thorpe-Morgan, C., Tsuji, N., Uchiyama, Y., Vecchi, M., Veh, J., Venter, C., Vink, J., Wagner, S. J., White, R., Wierzcholska, A., Wong, Yu Wun, Zacharias, M., Zargaryan, D., Zdziarski, A. A., Zech, A., Zouari, S., Zywucka, N.
Publikováno v:
Journal of Cosmology and Astroparticle Physics, 2023. IOP PUBLISHING LTD
JCAP
JCAP, 2023, 04, pp.040. ⟨10.1088/1475-7516/2023/04/040⟩
JCAP
JCAP, 2023, 04, pp.040. ⟨10.1088/1475-7516/2023/04/040⟩
Primordial Black Holes (PBHs) are hypothetical black holes predicted to have been formed from density fluctuations in the early Universe. PBHs with an initial mass around $10^{14}-10^{15}$g are expected to end their evaporation at present times in a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5d5c1e13782306c62eca17fb2d43a261
International audience; This work provides, at lower order, general analytical solutions for the orbital separation, merging time, and orbital frequency of binary systems emitting gravitational waves while being submitted to mass variations. Specific
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::179fc0e6c1b38ba9f9a8cc597c9fac7a
Autor:
Yi-Peng Wu, Kin-Wang Ng
Publikováno v:
Journal of High Energy Physics, Vol 2021, Iss 11, Pp 1-26 (2021)
JHEP
JHEP, 2021, 11, pp.076. ⟨10.1007/JHEP11(2021)076⟩
Journal of High Energy Physics
JHEP
JHEP, 2021, 11, pp.076. ⟨10.1007/JHEP11(2021)076⟩
Journal of High Energy Physics
Constant-rate inflation, including ultra-slow-roll as a special case, has been widely applied to the formation of primordial black holes with significant deviation from the standard slow-roll conditions at both the growing and decaying phases of the
Autor:
Ilia Musco, Theodoros Papanikolaou
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2022, 106 (8), pp.083017. ⟨10.1103/PhysRevD.106.083017⟩
Phys.Rev.D, 2022, 106 (8), pp.083017. ⟨10.1103/PhysRevD.106.083017⟩
This work investigates the formation of primordial black holes within a radiation fluid with an anisotropic pressure. We focus our attention on the initial conditions describing cosmological perturbations in the super horizon regime, using a covarian
Publikováno v:
Physical Review
Very recently, it was suggested that combining the Swampland program with the smallness of the dark energy and confronting these ideas to experiment lead to the prediction of the existence of a single extra-dimension (dubbed the dark dimension) with
Publikováno v:
Phys.Rev.D
Phys.Rev.D, 2022, 106 (12), pp.123020. ⟨10.1103/PhysRevD.106.123020⟩
Phys.Rev.D, 2022, 106 (12), pp.123020. ⟨10.1103/PhysRevD.106.123020⟩
Ultra-light primordial black holes (PBHs) in the mass range of 10$^{16}$ - 10$^{22}$ g are allowed by current observations to constitute a significant fraction, if not all, of the dark matter in the Universe. In this work, we present limits on ultra-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a4f47ffda28769535738ee3363342d69
http://arxiv.org/abs/2208.05705
http://arxiv.org/abs/2208.05705