A Better Reconciliation of Hubble Tension in the Dark Energy Scalar Field

被引：0

作者：

Fu, Le ^{[1
]}

Chen, Li ^{[2
]}

Yang, Maoyou ^{[2
]}

Wang, Junmei ^{[2
]}

Zhang, Ming-Jian ^{[2
]}

机构：

[1] Qilu Univ Technol, Shandong Acad Sci, Sch Informat & Automat Engn, Jinan 250353, Peoples R China

[2] Qilu Univ Technol, Shandong Acad Sci, Int Sch Optoelect Engn, Jinan 250353, Peoples R China

来源：

RESEARCH IN ASTRONOMY AND ASTROPHYSICS | 2023年 / 23卷 / 03期

关键词：

(cosmology:)dark energy; (cosmology:) cosmological parameters; cosmology: theory; MODEL; CONSTRAINTS; COSMOLOGY; H-0;

D O I：

10.1088/1674-4527/acafc6

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Hubble tension between the local measurement and global observation has been a key problem in cosmology. In this paper, we consider the quintessence scalar field, phantom field and quintom field as the dark energy to reconcile this problem. Different from most previous work, we start from the dimensionless equation of state (w) of dark energy, not a parameterization of potential. The combined analysis shows that observational data sets favor Hubble constant H0=71.3(-0.917)(+0.854)kms(-1)Mpc(-1) b h (2) and smaller omega( c ) h (2) than the standard lambda CDM model. We finally analyze a possible reason of Hubble tension from the kinematic acceleration a'' a'' z > 0.5. However, they increase and deviate from each other at low redshift, especially in the near future. Only the a''

引用

页数：9

共 50 条

[31] Dark Sirens to Resolve the Hubble-Lemaitre Tension
Borhanian, Ssohrab
Dhani, Arnab
Gupta, Anuradha
Arun, K. G.
Sathyaprakash, B. S.
ASTROPHYSICAL JOURNAL LETTERS, 2020, 905 (02)
[32] Small scale structures in coupled scalar field dark matter
Beyer, J.
Wetterich, C.
PHYSICS LETTERS B, 2014, 738 : 418 - 423
[33] Hubble Tension as a Window on the Gravitation of the Dark Matter Sector
Pitrou, Cyril
Uzan, Jean-Philippe
PHYSICAL REVIEW LETTERS, 2024, 132 (19)
[34] Generalized holographic dark energy model in the Hubble length
Malekjani, Mohammad
ASTROPHYSICS AND SPACE SCIENCE, 2013, 347 (02) : 405 - 410
[35] A scalar field dark energy model: Noether symmetry approach
Dutta, Sourav
Panja, Madan Mohan
Chakraborty, Subenoy
GENERAL RELATIVITY AND GRAVITATION, 2016, 48 (04)
[36] Is the cosmological dark sector better modeled by a generalized Chaplygin gas or by a scalar field?
del Campo, Sergio
Fabris, Julio C.
Herrera, Ramon
Zimdahl, Winfried
EUROPEAN PHYSICAL JOURNAL C, 2017, 77 (07):
[37] Acceleration of the Universe without the Hubble tension with Kaniadakis holographic dark energy using the Hubble horizon as the IR cut-off
Fang, Wei
Chen, Guo
Feng, Chao-Jun
Du, Wei
Shu, Chenggang
MODERN PHYSICS LETTERS A, 2025, 40 (05N06)
[38] Attractive proposal for resolving the Hubble tension: Dynamical attractors that unify early and late dark energy
Ramadan, Omar F.
Karwal, Tanvi
Sakstein, Jeremy
PHYSICAL REVIEW D, 2024, 109 (06)
[39] Reconstructions of scalar field dark energy models from new holographic dark energy in Galileon universe
Debnath, Ujjal
EUROPEAN PHYSICAL JOURNAL PLUS, 2014, 129 (12):
[40] Scalar Field Dark Matter
Matos, T
Guzmán, FS
Ureña-López, LA
Núñez, D
EXACT SOLUTIONS AND SCALAR FIELDS IN GRAVITY: RECENT DEVELOPMENTS, 2001, : 165 - 184

← 1 2 3 4 5 →