个人信息Personal Information
教授
博士生导师
硕士生导师
性别:男
毕业院校:大连理工大学
学位:博士
所在单位:物理学院
学科:理论物理
办公地点:物理学院211室
联系方式:lxxu .AT. dlut.edu.cn
Comparing the VGCG model as the unification of dark sectors with observations
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论文类型:期刊论文
发表时间:2014-04-01
发表刊物:SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
收录刊物:SCIE、EI
卷号:57
期号:4
页面范围:796-800
ISSN号:1674-7348
关键字:variable generalized Chaplygin gas (VGCG); unification of dark matter and dark energy; cosmic constraints
摘要:Current observations indicate that 95% of the energy density in the universe is the unknown dark component. The dark component is considered composed of two fluids: dark matter and dark energy. Or it is a mixture of these two dark components, i.e., one can consider it an exotic unknown dark fluid. With this consideration, the variable generalized Chaplygin gas (VGCG) model is studied with not dividing the unknown fluid into dark matter and dark energy parts in this paper. By using the Markov Chain Monte Carlo method, the VGCG model as the unification of dark sectors is constrained, and the constraint results on the VGCG model parameters are, n = 0.00057 (-0.0006-0.0006) (+0.0001+0.0009) , alpha = 0.0015 (-0.0015-0.0015) (+0.0003+0.0017) and B (s) = 0.778 (-0.016-0.035) (+0.016+0.030) , obtained by the cosmic microwave background data from the 7-year WMAP full data points, the baryon acoustic oscillation data from Sloan Digital Sky Survey (SDSS) and 2-degree Field Galaxy Redshift (2dFGRS) survey, and the Union2 type Ia supernova data with systematic errors. At last, according to the evolution of deceleration parameter it is shown that an expanded universe from deceleration to acceleration can be obtained in VGCG cosmology.