Lemaître Class Dark Energy Model for Relaxing Cosmological Constant
Cosmological constant corresponds to the maximally symmetric cosmological term with the equation of state p = − ρ . Introducing a cosmological term with the reduced symmetry, p r = − ρ in the spherically symmetric case, makes cosmological constant intrinsically variable component of...
| Main Authors: | , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
MDPI AG
2017-05-01
|
| Series: | Universe |
| Subjects: | |
| Online Access: | http://www.mdpi.com/2218-1997/3/2/39 |