ITP OpenIR  > SCI期刊论文
Li, FY; Wen, H; Fang, ZY; Wei, LF; Wang, YW; Zhang, M; Li, FY (reprint author), Chongqing Univ, Inst Gravitat Phys, Dept Phys, Chongqing 400044, Peoples R China.
Quasi-B-mode generated by high-frequency gravitational waves and corresponding perturbative photon fluxes
Source PublicationNUCLEAR PHYSICS B
Language英语
AbstractInteraction of very low-frequency primordial (relic) gravitational waves (GWs) to cosmic microwave background (CMB) can generate B-mode polarization. Here, for the first time we point out that the electromagnetic (EM) response to high-frequency GWs (HFGWs) would produce quasi-B-mode distribution of the perturbative photon fluxes. We study the duality and high complementarity between such two B-modes, and it is shown that such two effects are from the same physical origin: the tensor perturbation of the GWs and not the density perturbation. Based on this quasi-B-mode in HFGWs and related numerical calculation, it is shown that the distinguishing and observing of HFGWs from the braneworld would be quite possible due to their large amplitude, higher frequency and very different physical behaviors between the perturbative photon fluxes and background photons, and the measurement of relic HFGWs may also be possible though face to enormous challenge. (C) 2016 The Author(s). Published by Elsevier B.V.
2016
Volume911Pages:500-516
Subject AreaPhysics
DOIhttp://dx.doi.org/10.1016/j.nuclphysb.2016.08.009
Indexed BySCI
Funding OrganizationNational Natural Science Foundation of China [11375279, 11605015, 11205254] ; National Natural Science Foundation of China [11375279, 11605015, 11205254] ; National Natural Science Foundation of China [11375279, 11605015, 11205254] ; National Natural Science Foundation of China [11375279, 11605015, 11205254] ; Foundation of China Academy of Engineering Physics [2008 T0401, T0402] ; Foundation of China Academy of Engineering Physics [2008 T0401, T0402] ; Foundation of China Academy of Engineering Physics [2008 T0401, T0402] ; Foundation of China Academy of Engineering Physics [2008 T0401, T0402] ; Fundamental Research Funds for the Central Universities [106112016CDJXY300002, 106112015CDJRC131216] ; Fundamental Research Funds for the Central Universities [106112016CDJXY300002, 106112015CDJRC131216] ; Fundamental Research Funds for the Central Universities [106112016CDJXY300002, 106112015CDJRC131216] ; Fundamental Research Funds for the Central Universities [106112016CDJXY300002, 106112015CDJRC131216] ; Open Project Program of State Key Laboratory of Theoretical Physics Institute of Theoretical Physics, Chinese Academy of Sciences, China [Y5KF181CJ1] ; Open Project Program of State Key Laboratory of Theoretical Physics Institute of Theoretical Physics, Chinese Academy of Sciences, China [Y5KF181CJ1] ; Open Project Program of State Key Laboratory of Theoretical Physics Institute of Theoretical Physics, Chinese Academy of Sciences, China [Y5KF181CJ1] ; Open Project Program of State Key Laboratory of Theoretical Physics Institute of Theoretical Physics, Chinese Academy of Sciences, China [Y5KF181CJ1]
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Document Type期刊论文
Identifierhttp://ir.itp.ac.cn/handle/311006/21518
CollectionSCI期刊论文
Corresponding AuthorLi, FY (reprint author), Chongqing Univ, Inst Gravitat Phys, Dept Phys, Chongqing 400044, Peoples R China.
Recommended Citation
GB/T 7714
Li, FY,Wen, H,Fang, ZY,et al. Quasi-B-mode generated by high-frequency gravitational waves and corresponding perturbative photon fluxes[J]. NUCLEAR PHYSICS B,2016,911:500-516.
APA Li, FY.,Wen, H.,Fang, ZY.,Wei, LF.,Wang, YW.,...&Li, FY .(2016).Quasi-B-mode generated by high-frequency gravitational waves and corresponding perturbative photon fluxes.NUCLEAR PHYSICS B,911,500-516.
MLA Li, FY,et al."Quasi-B-mode generated by high-frequency gravitational waves and corresponding perturbative photon fluxes".NUCLEAR PHYSICS B 911(2016):500-516.
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