Journal
PHYSICAL REVIEW D
Volume 99, Issue 9, Pages -Publisher
AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.99.095032
Keywords
-
Funding
- Agence Nationale de Recherche [ANR-15-CE31-0002]
- Labex Institut Lagrange de Paris [ANR-11-IDEX-0004-02, ANR-10-LABX-63]
- Agence Nationale de la Recherche (ANR) [ANR-15-CE31-0002] Funding Source: Agence Nationale de la Recherche (ANR)
Ask authors/readers for more resources
Stochastic gravitational waves can be produced during the preheating when out-of-equilibrium particles are produced with an anisotropic stress tensor. We discuss the case where these particles carry spin 3/2. We compute the spectrum of the gravitational waves generated by the transverse and longitudinal components. We find a different scaling of the spectrum near the peak and the longitudinal components lead to an enhancement when compared to spin-1/2 fermions with Yukawa couplings. We note, as expected, that the corresponding typical frequency is too high for the current observation and calls for ultrahigh frequency gravitational wave detectors in the future.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available