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Detection of Early-Universe Gravitational Wave Signatures and Fundamental Physics / Caldwell, Robert (Dartmouth Coll.) ; Cui, Yanou (UC, Riverside) ; Guo, Huai-Ke (U. Utah, Salt Lake City) ; Mandic, Vuk (Minnesota U.) ; Mariotti, Alberto (Brussels U., IIHE) ; No, Jose Miguel (Madrid, IFT) ; Ramsey-Musolf, Michael J. (Shanghai Jiao Tong U.) ; Sakellariadou, Mairi (King's Coll. London) ; Sinha, Kuver (U. Oklahoma, Norman) ; Wang, Lian-Tao (Chicago U.) et al.
Detection of a gravitational-wave signal of non-astrophysical origin would be a landmark discovery, potentially providing a significant clue to some of our most basic, big-picture scientific questions about the Universe. In this white paper, we survey the leading early-Universe mechanisms that may produce a detectable signal -- including inflation, phase transitions, topological defects, as well as primordial black holes -- and highlight the connections to fundamental physics. [...]
arXiv:2203.07972.- 2022-11-30 - 67 p. Fulltext: 2203.07972 - PDF; document - PDF; External link: eConf
In : 2021 Snowmass Summer Study, Seattle, WA, United States, 11 - 20 July 2021, pp.

Detaljnije - Slični zapisi

Implications for First-Order Cosmological Phase Transitions from the Third LIGO-Virgo Observing Run / Romero, Alba (Barcelona, IFAE) ; Martinovic, Katarina (King's Coll. London) ; Callister, Thomas A. (Flatiron Inst., New York) ; Guo, Huai-Ke (Oklahoma U.) ; Martínez, Mario (Barcelona, IFAE ; ICREA, Barcelona) ; Sakellariadou, Mairi (King's Coll. London ; CERN) ; Yang, Feng-Wei (Utah U.) ; Zhao, Yue (Utah U.)
We place constrains on the normalised energy density in gravitational waves from first-order strong phase transitions using data from Advanced LIGO and Virgo's first, second and third observing runs. First, adopting a broken power law model, we place $95 \%$ confidence level upper limits simultaneously on the gravitational-wave energy density at 25 Hz from unresolved compact binary mergers, $\Omega_{\rm cbc} < 5.9 \times 10^{-9}$, and strong first-order phase transitions, $\Omega_{\rm bpl} < 2.8 \times 10^{-9}$. [...]
arXiv:2102.01714.- 2021-04-17 - 7 p. - Published in : Phys. Rev. Lett. 126 (2021) 151301 Article from SCOAP3: PDF; Fulltext: PDF; Fulltext from publisher: PDF;

Detaljnije - Slični zapisi

Također vidi: slična imena autora
117	Guo, H
3	Guo, H C
2	Guo, H F
1	Guo, H J
2	Guo, H M
2	Guo, H R
19	Guo, H W
140	Guo, H Y
7	Guo, H.
8	Guo, H.-K.
1	Guo, Hai-Chuan
1	Guo, Hai-Feng
1	Guo, Haibiao
13	Guo, Hairun
1	Guo, Han
10	Guo, Han-Ying
3	Guo, Hanliang
5	Guo, Hao
21	Guo, Heng
4	Guo, Hengxiao
76	Guo, Hong
1	Guo, Hong-Li
1	Guo, Hong-gang
1	Guo, Hongbo
5	Guo, Hongli
1	Guo, Hongwen
2	Guo, Hongzhi
6	Guo, Hua
2	Guo, Huadong
6	Guo, Huai-ke
1	Guo, Huan
1	Guo, Hui
1	Guo, Huicheng
1	Guo, Huidong
1	Guo, Hun

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