Quasi-B-mode generated by high-frequency gravitational waves and corresponding perturbative photon fluxes

DOI10.1016/j.nuclphysb.2016.08.009zbMath1346.83027arXiv1505.06546OpenAlexW1517275096MaRDI QIDQ318788

Miao Zhang, Hao Wen, Zhen-Yun Fang, Lian-Fu Wei, Yi Wen Wang, Fang-Yu Li

Publication date: 5 October 2016

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1505.06546

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Quantum optics (81V80) Electromagnetic fields in general relativity and gravitational theory (83C50) Gravitational waves (83C35)

Related Items (1)

Characteristic electromagnetic waves caused by tensorial and possible nontensorial thermal high-frequency gravitational waves from magnetars

Cites Work

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• Very high frequency gravitational wave background in the universe
• A gravitational wave window on extra dimensions
• The thermal history of the plasma and high-frequency gravitons
• Detecting the cosmic gravitational wave background with the Big Bang Observer

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