Signal photon flux generated by high-frequency relic gravitational waves
Wen, H; Li, X; Li, X (reprint author), Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China.; Wang, S; Li, X (reprint author), Chongqing Univ, Dept Phys, Chongqing 401331, Peoples R China.
刊名CHINESE PHYSICS C
2016
卷号40期号:8页码:85101
关键词Relic Gravitational Waves High Frequency Gravitational Waves Detector Signal Photon Flux
DOIhttp://dx.doi.org/10.1088/1674-1137/40/8/085101
英文摘要The power spectrum of primordial tensor perturbations P-t increases rapidly in the high frequency region if the spectral index n(t) > 0. It is shown that the amplitude of relic gravitational waves h(t) (5 x 10(9) Hz) varies from 10(-36) to 10(-25) while n(t) varies from -6.25 x 10(-3) to 0.87. A high frequency gravitational wave detector proposed by F.-Y. Li detects gravitational waves through observing the perturbed photon flux that is generated by interaction between relic gravitational waves and electromagnetic field. It is shown that the perturbative photon flux N-x(1) (5 x 10(9) Hz) varies from 1.40 x 10(-4) s(-1) to 2.85 x 10(7) s(-1) while Tit varies from -6.25 x 10(-3) to 0.87. Correspondingly, the ratio of the transverse perturbative photon flux NI to the background photon flux varies from 10(-28) to 10(-16).
学科主题Physics
语种英语
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/21580]  
专题理论物理研究所_理论物理所1978-2010年知识产出
通讯作者Li, X (reprint author), Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, Beijing 100190, Peoples R China.; Li, X (reprint author), Chongqing Univ, Dept Phys, Chongqing 401331, Peoples R China.
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Wen, H,Li, X,Li, X ,et al. Signal photon flux generated by high-frequency relic gravitational waves[J]. CHINESE PHYSICS C,2016,40(8):85101.
APA Wen, H,Li, X,Li, X ,Wang, S,&Li, X .(2016).Signal photon flux generated by high-frequency relic gravitational waves.CHINESE PHYSICS C,40(8),85101.
MLA Wen, H,et al."Signal photon flux generated by high-frequency relic gravitational waves".CHINESE PHYSICS C 40.8(2016):85101.
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