Effects of modified Chaplygin gas on structure formation in the universe

DOI10.1007/s10714-013-1537-6zbMath1271.83098OpenAlexW2123580394MaRDI QIDQ354726

Jian-Bo Lu, Yue-Yue Zhao, Xue Zhang, Ya-Bo Wu, Wei-Qiang Yang, Yang-Yang Su, Liang-Liang Lin

Publication date: 19 July 2013

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/s10714-013-1537-6

zbMATH Keywords

structure formationdark energydensity contrastMCGmodified Chaplygin gas

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Approximation procedures, weak fields in general relativity and gravitational theory (83C25) Astrophysical cosmology (85A40)

Related Items (3)

Toy models of universe with an effective varying \(\Lambda\)-term in Lyra manifold ⋮ THERMODYNAMICAL BEHAVIORS OF NONFLAT BRANS–DICKE GRAVITY WITH INTERACTING NEW AGEGRAPHIC DARK ENERGY ⋮ Analysis on modified Chaplygin gas as dark energy model

Cites Work

• Quinstant dark energy predictions for structure formation
• A modified Chaplygin gas model with interaction
• Structure formation and CMBR anisotropy spectrum in the inflessence model
• Role of modified Chaplygin gas in accelerated universe
• Measurements of Ω and Λ from 42 High‐Redshift Supernovae
• Cosmological Imprint of an Energy Component with General Equation of State
• An alternative to quintessence

This page was built for publication: Effects of modified Chaplygin gas on structure formation in the universe