Gravitational radiation background from boson star binaries
Croon, D; Mohapatra, S1; Gleiser, M; Sun, C3
刊名PHYSICS LETTERS B
2018
卷号783页码:158-162
关键词GALAXY CLUSTER 1E-0657-56 INTERACTION CROSS-SECTION DARK-MATTER BLACK-HOLES SIMULATIONS CONSTRAINTS STABILITY EVOLUTION REDSHIFT UNIVERSE
ISSN号0370-2693
DOI10.1016/j.physletb.2018.03.055
英文摘要We calculate the gravitational radiation background generated from boson star binaries formed in locally dense clusters with formation rate tracked by the regular star formation rate. We compute how the frequency window in gravitational waves is affected by the boson field mass and repulsive self-coupling, anticipating constraints from EPTA and LISA. We also comment on the possible detectability of these binaries. (c) 2018 The Authors. Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). Funded by SCOAP(3).
学科主题Astronomy & Astrophysics ; Physics
语种英语
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/22838]  
专题理论物理研究所_理论物理所1978-2010年知识产出
作者单位1.Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
2.Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
3.Univ Sussex, Dept Phys & Astron, Brighton BN1 9QH, E Sussex, England
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GB/T 7714
Croon, D,Mohapatra, S,Gleiser, M,et al. Gravitational radiation background from boson star binaries[J]. PHYSICS LETTERS B,2018,783:158-162.
APA Croon, D,Mohapatra, S,Gleiser, M,&Sun, C.(2018).Gravitational radiation background from boson star binaries.PHYSICS LETTERS B,783,158-162.
MLA Croon, D,et al."Gravitational radiation background from boson star binaries".PHYSICS LETTERS B 783(2018):158-162.
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