Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves
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 symmetry breaking processes during the evolution of the unive...
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Elsevier
2019-01-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269318308645 |
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doaj-993f972e2bf04bbc8c3c2555debde9c82020-11-25T00:29:28ZengElsevierPhysics Letters B0370-26932019-01-01788288294Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational wavesFa Peng Huang0Xinmin Zhang1Theoretical Physics Division, Institute of High Energy Physics, Chinese Academy of Sciences, P.O. Box 918-4, Beijing 100049, China; School of Physics Sciences, University of Chinese Academy of Sciences, Beijing 100039, China; Corresponding author.Theoretical Physics Division, Institute of High Energy Physics, Chinese Academy of Sciences, P.O. Box 918-4, Beijing 100049, China; School of Physics Sciences, University of Chinese Academy of Sciences, Beijing 100039, ChinaTaking 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 symmetry breaking processes during the evolution of the universe, which can produce detectable phase transition gravitational wave (GW) signals at future GW experiments, such as LISA, BBO, DECIGO, SKA and aLIGO. These GW signals can provide new sources of GWs with different peak frequencies, and can be used to probe the evolution history of the universe.http://www.sciencedirect.com/science/article/pii/S0370269318308645 |
| collection |
DOAJ |
| language |
English |
| format |
Article |
| sources |
DOAJ |
| author |
Fa Peng Huang Xinmin Zhang |
| spellingShingle |
Fa Peng Huang Xinmin Zhang Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves Physics Letters B |
| author_facet |
Fa Peng Huang Xinmin Zhang |
| author_sort |
Fa Peng Huang |
| title |
Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves |
| title_short |
Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves |
| title_full |
Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves |
| title_fullStr |
Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves |
| title_full_unstemmed |
Probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves |
| title_sort |
probing the gauge symmetry breaking of the early universe in 3-3-1 models and beyond by gravitational waves |
| publisher |
Elsevier |
| series |
Physics Letters B |
| issn |
0370-2693 |
| publishDate |
2019-01-01 |
| description |
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 symmetry breaking processes during the evolution of the universe, which can produce detectable phase transition gravitational wave (GW) signals at future GW experiments, such as LISA, BBO, DECIGO, SKA and aLIGO. These GW signals can provide new sources of GWs with different peak frequencies, and can be used to probe the evolution history of the universe. |
| url |
http://www.sciencedirect.com/science/article/pii/S0370269318308645 |
| work_keys_str_mv |
AT fapenghuang probingthegaugesymmetrybreakingoftheearlyuniversein331modelsandbeyondbygravitationalwaves AT xinminzhang probingthegaugesymmetrybreakingoftheearlyuniversein331modelsandbeyondbygravitationalwaves |
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