Gauge field preheating at the end of inflation
Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN: 1550-7998, Vol: 88, Issue: 6
2013
- 46Citations
- 89Usage
- 16Captures
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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
- Citations46
- Citation Indexes46
- 46
- CrossRef18
- Usage89
- Downloads80
- Abstract Views9
- Captures16
- Readers16
- 16
Article Description
Here we consider the possibility of preheating the Universe via the parametric amplification of a massless, U(1) Abelian gauge field. We assume that the gauge field is coupled to the inflaton via a dilaton-like coupling, a conformal factor with one free parameter. We present the results of high-resolution three-dimensional simulations of this model and show that this mechanism efficiently preheats the Universe to a radiation-dominated final state. © 2013 American Physical Society.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84885067332&origin=inward; http://dx.doi.org/10.1103/physrevd.88.063530; https://link.aps.org/doi/10.1103/PhysRevD.88.063530; http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.88.063530/fulltext; http://link.aps.org/article/10.1103/PhysRevD.88.063530; https://digitalcommons.dartmouth.edu/facoa/2714; https://digitalcommons.dartmouth.edu/cgi/viewcontent.cgi?article=3728&context=facoa
American Physical Society (APS)
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