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Observational constraint on dark energy from quantum uncertainty | |
Huang, Long1,4![]() ![]() ![]() | |
2021-12-01 | |
Source Publication | CHINESE PHYSICS C
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ISSN | 1674-1137 |
Volume | 45Issue:12Pages:125102 |
Contribution Rank | 1 |
Abstract | We explore the theoretical possibility that dark energy density is derived from massless scalar bosons in vacuum and present a physical model for dark energy. By assuming massless scalar bosons fall into the horizon boundary of the cosmos with the expansion of the universe, we can deduce the uncertainty in the relative position of scalar bosons based on the quantum fluctuation of space-time and the assumption that scalar bosons satisfy P-symmetry under the parity transformation P-phi(r) = -phi(r), which can be used to estimate scalar bosons and dark energy density. Furthermore, we attempt to explain the origin of negative pressure from the increasing entropy density of the Boltzmann system and derive the equation for the state parameter, which is consistent with the specific equations of state for dark energy. Finally, we employ the SNIa Pantheon sample and Planck 2018 CMB angular power spectra to constrain the models and provide statistical results for the cosmology parameters. |
Keyword | scalar bosons P-symmetry quantum fluctuations dark energy SNIa CMB |
DOI | 10.1088/1674-1137/ac2946 |
Indexed By | SCI |
Language | 英语 |
WOS Keyword | DIGITAL SKY SURVEY ; SPACE-TIME ; MODEL ; SUPERNOVAE ; DISTANCE ; GRAVITY ; LIGHT |
Funding Project | CAS Pioneer Hundred Talents Program ; National Key R&D Program of China[2018YFA0404602] |
WOS Research Area | Physics |
WOS Subject | Physics, Nuclear ; Physics, Particles & Fields |
WOS ID | WOS:000727002800001 |
Publisher | IOP Publishing Ltd |
Funding Organization | CAS Pioneer Hundred Talents Program ; National Key R&D Program of China |
Citation statistics | |
Document Type | 期刊论文 |
Identifier | http://ir.xao.ac.cn/handle/45760611-7/4384 |
Collection | 射电天文研究室_星系宇宙学研究团组 |
Corresponding Author | Yang, Xiaofeng |
Affiliation | 1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China 2.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Peoples R China 3.Key Lab Radio Astrophys Xinjiang Prov, Urumqi 830011, Peoples R China 4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China |
First Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Corresponding Author Affilication | Xinjiang Astronomical Observatory, Chinese Academy of Sciences |
Recommended Citation GB/T 7714 | Huang, Long,Yang, Xiaofeng,Liu, Xiang. Observational constraint on dark energy from quantum uncertainty[J]. CHINESE PHYSICS C,2021,45(12):125102. |
APA | Huang, Long,Yang, Xiaofeng,&Liu, Xiang.(2021).Observational constraint on dark energy from quantum uncertainty.CHINESE PHYSICS C,45(12),125102. |
MLA | Huang, Long,et al."Observational constraint on dark energy from quantum uncertainty".CHINESE PHYSICS C 45.12(2021):125102. |
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Huang-2021-Observati(665KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text |
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