Fully self-consistent cosmological simulation pipeline for interacting dark energy models-Reference-Cited by-同舟云学术

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Fully self-consistent cosmological simulation pipeline for interacting dark energy models

Published:2018-11-27 Issue:10 Volume:98 Page:
ISSN:2470-0010
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Zhang Jiajun,An Rui,Liao Shihong,Luo Wentao,Li Zhaozhou,Wang Bin

Funder

China Postdoctoral Science Foundation

National Natural Science Foundation of China

Shanghai Jiao Tong University and University of Michigan

World Premier International Research Center Initiative

Publisher

American Physical Society (APS)

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.98.103530/fulltext

Reference35 articles.

1. The cosmological constant problem

2. Quintessence, Cosmic Coincidence, and the Cosmological Constant

3. A 3% SOLUTION: DETERMINATION OF THE HUBBLE CONSTANT WITH THEHUBBLE SPACE TELESCOPEAND WIDE FIELD CAMERA 3

4. A 2.4% DETERMINATION OF THE LOCAL VALUE OF THE HUBBLE CONSTANT

5. Baryon acoustic oscillations in the Lyαforest of BOSS DR11 quasars

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1. Tightening the reins on nonminimal dark sector physics: Interacting dark energy with dynamical and nondynamical equation of state;Physical Review D;2024-09-11

2. Further understanding the interaction between dark energy and dark matter: current status and future directions;Reports on Progress in Physics;2024-02-23

3. Cosmological simulations of a momentum coupling between dark matter and quintessence;Monthly Notices of the Royal Astronomical Society;2023-09-12

4. Void Lensing in Cubic Galileon Gravity;The Astrophysical Journal;2023-07-01

5. Constraining interacting dark energy models with the halo concentration–mass relation;Monthly Notices of the Royal Astronomical Society;2023-06-19

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