Knowledge Management System of Institute of Theoretical Physics, CAS
Cai, RG ; Liu, TB; Wang, SJ
| |
| Gravitational wave as probe of superfluid dark matter | |
| Source Publication | PHYSICAL REVIEW D
 |
| Language | 英语 |
| Keyword | NEWTONIAN DYNAMICS ACCELERATION RELATION GENERAL-RELATIVITY GALAXIES GW150914 MASS ROTATION MOND LAW |
| Abstract | In recent years, superfluid dark matter (SfDM) has become a competitive model of emergent modified Newtonian dynamics (MOND) scenario: MOND phenomenons naturally emerge as a derived concept due to an extra force mediated between baryons by phonons as a result of axionlike particles condensed as superfluid at galactic scales; Beyond galactic scales, these axionlike particles behave as normal fluid without phonon-mediated MOND-like force between baryons, therefore SfDM also maintains the usual success of ACDM at cosmological scales. In this paper, we use gravitational waves (GWs) to probe the relevant parameter space of SfDM. GWs through Bose-Einstein condensate (BEC) could propagate with a speed slightly deviation from the specd-of-light due to the change in the effective refractive index, which depends on the SfDM parameters and GW-source properties. We find that Five hundred meter Aperture Spherical Telescope (FAST), Square Kilometre Array (SKA) and International Pulsar Timing Array (IPTA) are the most promising means as GW probe of relevant parameter space of SfDM. Future space-based GW detectors are also capable of probing SfDM if a multimcssengcr approach is adopted. |
| 2018 | |
| ISSN | 2470-0010 |
| Volume | 97Issue:2Pages:23027 |
| Subject Area | Astronomy & Astrophysics ; Physics |
| MOST Discipline Catalogue | Astronomy & Astrophysics ; Physics, Particles & Fields |
| DOI | 10.1103/PhysRevD.97.023027 |
| Indexed By | SCIE |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.itp.ac.cn/handle/311006/22974 |
| Collection | SCI期刊论文 |
| Affiliation | 1.[Cai, Rong-Gen 2.Liu, Tong-Bo 3.Chinese Acad Sci, CAS Key Lab Theoret Phys, Inst Theoret Phys, Beijing 100190, Peoples R China 4.Univ Chinese Acad Sci, Sch Phys Sci, 19A Yuquan Rd, Beijing 100049, Peoples R China |
| Recommended Citation GB/T 7714 | Cai, RG,Liu, TB,Wang, SJ. Gravitational wave as probe of superfluid dark matter[J]. PHYSICAL REVIEW D,2018,97(2):23027. |
| APA | Cai, RG,Liu, TB,&Wang, SJ.(2018).Gravitational wave as probe of superfluid dark matter.PHYSICAL REVIEW D,97(2),23027. |
| MLA | Cai, RG,et al."Gravitational wave as probe of superfluid dark matter".PHYSICAL REVIEW D 97.2(2018):23027. |
| Files in This Item: | ||||||
| File Name/Size | DocType | Version | Access | License | ||
| Gravitational wave a（557KB） | 期刊论文 | 作者接受稿 | 开放获取 | CC BY-NC-SA | Application Full Text | |
Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.
Edit Comment