Running vacuum model in a non-flat universe

被引：0

作者：

耿朝强 ^{[1
,2
,3
,4
]}

徐彦婷 ^{[3
]}

尹璐 ^{[1
,2
,3
]}

张开拓 ^{[5
,6
]}

机构：

[1] School of Fundamental Physics and Mathematical Sciences Hangzhou Institute for Advanced Study UCAS

[2] International Centre for Theoretical Physics Asia-Pacific

[3] Department of Physics National Tsing Hua University

[4] Department of Physics Anhui Normal University

[5] Collaborative Innovation Center of Light Manipulations and Applications Shandong Normal University

来源：

Chinese Physics C | 2020年 / 10期

基金：

中国国家自然科学基金;

关键词：

D O I：

暂无

中图分类号：

P159 [宇宙学];

学科分类号：

070401 ;

摘要：

We investigate observational constraints on the running vacuum model （RVM） ofΛ=3ν（H;+K/a;）+c;in a spatially curved universe,whereνis the model parameter,K corresponds to the spatial curvature constant,a represents the scalar factor,and c;is a constant defined by the boundary conditions.We study the CMB power spectra with several sets ofνand K in the RVM.By fitting the cosmological data,we find that the best fittedχ;value for RVM is slightly smaller than that ofΛCDM in the non-flat universe,along with the constraints of■.In particular,our results favor the open universe in bothΛCDM and RVM.In addition,we show that the cosmological constraints of ■at 95%C.L.for the neutrino mass sum are relaxed in both models in the spatially curved universe.

引用

页码：182 / 188

页数：7

共 50 条

[21] Interacting tachyon dark energy in non-flat universe
Setare, M. R.
Sadeghi, J.
Amani, A. R.
PHYSICS LETTERS B, 2009, 673 (4-5) : 241 - 246
[22] Viscous Generalized Chaplygin Gas in Non-flat Universe
H. Saadat
International Journal of Theoretical Physics, 2013, 52 : 1696 - 1700
[23] FRW Bulk Viscous Cosmology in Non-flat Universe
Hassan Saadat
International Journal of Theoretical Physics, 2012, 51 : 1317 - 1322
[24] Interacting New Agegraphic Phantom Model of Dark Energy in Non-flat Universe
Setare, M. R.
INTERNATIONAL JOURNAL OF THEORETICAL PHYSICS, 2010, 49 (04) : 759 - 765
[25] Quintessence Reconstruction of Interacting HDE in a Non-Flat Universe
A.Sheykhi
H.Alavirad
A.Bagheri
E.Ebrahimi
Communications in Theoretical Physics, 2014, 61 (06) : 773 - 780
[26] Quintessence Reconstruction of Interacting HDE in a Non-Flat Universe
Sheykhi, A.
Alavirad, H.
Bagheri, A.
Ebrahimi, E.
COMMUNICATIONS IN THEORETICAL PHYSICS, 2014, 61 (06) : 773 - 780
[27] Interacting ghost dark energy in non-flat universe
Sheykhi, A.
Movahed, M. Sadegh
GENERAL RELATIVITY AND GRAVITATION, 2012, 44 (02) : 449 - 465
[28] Interacting Holographic Modified Gravity in a Non-flat Universe
A. Banijamali
M. R. Setare
B. Fazlpour
International Journal of Theoretical Physics, 2011, 50 : 3275 - 3283
[29] AGEGRAPHIC DARK ENERGY MODEL IN THE NON-FLAT UNIVERSE: STATEFINDER DIAGNOSTIC AND ω-ω′ ANALYSIS
Malekjani, M.
Khodam-Mohammadi, A.
INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2010, 19 (11): : 1857 - 1871
[30] Reconstructing an interacting holographic polytropic gas model in a non-flat FRW universe
Karami, K.
Abdolmaleki, A.
PHYSICA SCRIPTA, 2010, 81 (05)

← 1 2 3 4 5 →