Zobrazeno 1 - 10
of 48
pro vyhledávání: '"Fa Peng Huang"'
Publikováno v:
Journal of High Energy Physics, Vol 2024, Iss 7, Pp 1-40 (2024)
Abstract As a new type of dynamical dark matter mechanism, we discuss the stability of the gauged Q-ball dark matter and its production mechanism through a cosmological first-order phase transition. This work delves into the study of gauged Q-ball da
Externí odkaz:
https://doaj.org/article/b4cfacd273fb4cff970bcfe670bf2d17
Autor:
Fa Peng Huang, Xinmin Zhang
Publikováno v:
Physics Letters B, Vol 788, Iss , Pp 288-294 (2019)
Taking the 3-3-1 models (with SU(3)c⊗SU(3)L⊗U(1)Y gauge group) as examples, we study that a class of new physics models with extended gauge group could undergo one or several first-order phase transitions associated with the spontaneously symmetr
Externí odkaz:
https://doaj.org/article/993f972e2bf04bbc8c3c2555debde9c8
Autor:
Fa Peng Huang
Publikováno v:
Nuclear and Particle Physics Proceedings. :21-26
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ff1e618e0f1d754d7340f3a48919ba48
https://doi.org/10.1016/j.nuclphysbps.2023.04.013
https://doi.org/10.1016/j.nuclphysbps.2023.04.013
Publikováno v:
Physical Review
The bubble wall velocity is essential for the spectra of phase-transition gravitational waves, electroweak baryogenesis and the dynamical dark matter mechanism. We perform detailed calculations of the bubble wall velocity in the well-motivated inert
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ff8041cc888b68a7c997d892362d8b9f
https://doi.org/10.1103/physrevd.107.095005
https://doi.org/10.1103/physrevd.107.095005
Publikováno v:
Physical Review D. 105
We quantitatively study how the primordial density fluctuations are imprinted on the anisotropy of the phase transition gravitational wave (PTGW). Generated long before recombination and free from Silk damping, the anisotropic PTGW might reveal the d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d02a5473ff8796b91bb7cc0b4f082b43
https://doi.org/10.1103/physrevd.105.083527
https://doi.org/10.1103/physrevd.105.083527
A cosmological first-order phase transition gravitational wave could provide a novel approach to studying the early Universe. In most cases, the acoustic gravitational wave from the sound wave mechanism is dominant. Considering different sound veloci
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::75a6f4169cdcc532d3d7127479432e1c
Publikováno v:
Physical Review
We study how to unravel the dark matter blind spots by phase transition gravitational waves in synergy with collider signatures at electroweak one-loop level taking the inert doublet model as an example. We perform a detailed Monte Carlo study at the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cb882d944da59d4e5bd212cce49e939d
http://arxiv.org/abs/2012.03920
http://arxiv.org/abs/2012.03920
Publikováno v:
Physical Review Letters
Dark photon as an ultralight dark matter candidate can interact with the Standard Model particles via kinetic mixing. We propose to search for the ultralight dark photon dark matter using radio telescopes with solar observations. The dark photon dark
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6d201f52ed30a30054035aa0c41567a4
http://arxiv.org/abs/2010.15836
http://arxiv.org/abs/2010.15836
The energy budget of cosmological first-order phase transition is essential for the gravitational wave spectra. Most of the previous studies are based on the bag model with same sound velocity in the symmetric and broken phase. We study the energy bu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb6c7d6d3defd9ae9d656d93dc35900f
http://arxiv.org/abs/2010.13770
http://arxiv.org/abs/2010.13770
We study the radio signals generated when an axion star enters the magnetosphere of a neutron star. As the axion star moves through the resonant region where the plasma-induced photon mass becomes equal to the axion mass, the axions can efficiently c
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::115749d5c14193f62107a0e09786728b
http://arxiv.org/abs/2004.06486
http://arxiv.org/abs/2004.06486