Energy budget of cosmological first-order phase transition in FLRWbackground
Science China: Physics, Mechanics and Astronomy, ISSN: 1869-1927, Vol: 61, Issue: 8, Page: 080411-1-080411-20
2018
- 9Citations
- 5Captures
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Example: if you select the 1-year option for an article published in 2019 and a metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019. If you select the 3-year option for the same article published in 2019 and the metric category shows 90%, that means that the article or review is performing better than 90% of the other articles/reviews published in that journal in 2019, 2018 and 2017.
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Metrics Details
- Citations9
- Citation Indexes9
- CrossRef1
- Captures5
- Readers5
Article Description
We study the hydrodynamics of bubble expansion in cosmological first-order phase transition in the Friedmann-Lemaˆıtre- Robertson-Walker (FLRW) background with probe limit. Different from previous studies for fast first-order phase transition in flat background, we find that, for slow first-order phase transition in FLRW background with a given peculiar velocity of the bubble wall, the efficiency factor of energy transfer into bulk motion of thermal fluid is significantly reduced, thus decreasing the previously-thought dominated contribution from sound wave to the stochastic gravitational-wave background.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85045971285&origin=inward; http://dx.doi.org/10.1007/s11433-018-9216-7; http://link.springer.com/10.1007/s11433-018-9216-7; http://link.springer.com/content/pdf/10.1007/s11433-018-9216-7.pdf; http://link.springer.com/article/10.1007/s11433-018-9216-7/fulltext.html; http://sciencechina.cn/gw.jsp?action=cited_outline.jsp&type=1&id=6343194&internal_id=6343194&from=elsevier; https://dx.doi.org/10.1007/s11433-018-9216-7; https://link.springer.com/article/10.1007/s11433-018-9216-7
Springer Nature
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