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Nonexistence of interactions between axially symmetric massive scalar field and perfect fluid distribution
General Relativity and Gravitation
◽
10.1007/bf00758974
◽
1988
◽
Vol 20
(7)
◽
pp. 711-714
Author(s):
R. K. Tarachand
◽
N. Ibotombi Singh
Keyword(s):
Scalar Field
◽
Perfect Fluid
◽
Fluid Distribution
◽
Massive Scalar
◽
Axially Symmetric
◽
Massive Scalar Field
◽
Perfect Fluid Distribution
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References
Axially symmetric Bianchi type-I cosmological model of the universe in the presence of perfect fluid and an attractive massive scalar field in Lyra manifold
Astrophysics and Space Science
◽
10.1007/s10509-020-03796-4
◽
2020
◽
Vol 365
(5)
◽
Cited By ~ 1
Author(s):
R. L. Naidu
◽
Y. Aditya
◽
G. Ramesh
◽
D. R. K. Reddy
Keyword(s):
Scalar Field
◽
Cosmological Model
◽
Perfect Fluid
◽
Bianchi Type
◽
Type I
◽
Massive Scalar
◽
Axially Symmetric
◽
Massive Scalar Field
◽
Bianchi Type I
◽
The Universe
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Dynamics of perfect fluid cosmological model in the presence of massive scalar field in f ( R , T ) $f(R,T)$ gravity
Astrophysics and Space Science
◽
10.1007/s10509-018-3491-y
◽
2019
◽
Vol 364
(1)
◽
Cited By ~ 12
Author(s):
Y. Aditya
◽
D. R. K. Reddy
Keyword(s):
Scalar Field
◽
Cosmological Model
◽
Perfect Fluid
◽
Massive Scalar
◽
Massive Scalar Field
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A class of exact solutions for axially symmetric charged perfect fluid distribution in SEN-DUNN theory of gravitation
Acta Physica Academiae Scientiarum Hungaricae
◽
10.1007/bf03159437
◽
1981
◽
Vol 50
(3)
◽
pp. 211-225
◽
Cited By ~ 1
Author(s):
B. Chatterjee
◽
A. R. Roy
Keyword(s):
Exact Solutions
◽
Perfect Fluid
◽
Fluid Distribution
◽
Axially Symmetric
◽
Perfect Fluid Distribution
◽
Theory Of Gravitation
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Slowly rotating universes with radiating perfect fluid distribution coupled with a scalar field in general relativity
General Relativity and Gravitation
◽
10.1007/bf02108230
◽
1995
◽
Vol 27
(11)
◽
pp. 1145-1165
◽
Cited By ~ 2
Author(s):
Kj. Maniharsingh
Keyword(s):
General Relativity
◽
Scalar Field
◽
Perfect Fluid
◽
Fluid Distribution
◽
Perfect Fluid Distribution
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Isotropization of the minimally coupled scalar–tensor theory with a massive scalar field and a perfect fluid in the Bianchi type I model
Classical and Quantum Gravity
◽
10.1088/0264-9381/19/2/307
◽
2002
◽
Vol 19
(2)
◽
pp. 269-278
◽
Cited By ~ 4
Author(s):
Stéphane Fay
Keyword(s):
Scalar Field
◽
Perfect Fluid
◽
Bianchi Type
◽
Type I
◽
Scalar Tensor Theory
◽
Massive Scalar
◽
Massive Scalar Field
◽
Bianchi Type I
◽
Tensor Theory
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Massive scalar field interacting with viscous fluid distribution in cosmological models
Astrophysics and Space Science
◽
10.1007/bf00714154
◽
1988
◽
Vol 150
(1)
◽
pp. 65-74
◽
Cited By ~ 1
Author(s):
R. K. Tarachand Singh
◽
N. Ibotombi Singh
Keyword(s):
Scalar Field
◽
Viscous Fluid
◽
Cosmological Models
◽
Fluid Distribution
◽
Massive Scalar
◽
Massive Scalar Field
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On new symmetries and exact solutions of Einstein’s field equation for perfect fluid distribution
Pramana
◽
10.1007/s12043-021-02162-5
◽
2021
◽
Vol 95
(3)
◽
Author(s):
R K Gupta
◽
Radhika Jain
◽
Sachin Kumar
◽
Divya Jyoti
Keyword(s):
Field Equation
◽
Exact Solutions
◽
Perfect Fluid
◽
Fluid Distribution
◽
Perfect Fluid Distribution
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Log to log-log crossover of entanglement in a (1+1) -dimensional massive scalar field
Physical Review D
◽
10.1103/physrevd.103.125008
◽
2021
◽
Vol 103
(12)
◽
Author(s):
Parul Jain
◽
S. Mahesh Chandran
◽
S. Shankaranarayanan
Keyword(s):
Scalar Field
◽
Massive Scalar
◽
Massive Scalar Field
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Casimir effect for a massive scalar field under mixed boundary conditions
Brazilian Journal of Physics
◽
10.1590/s0103-97332003000400042
◽
2003
◽
Vol 33
(4)
◽
pp. 860-866
◽
Cited By ~ 9
Author(s):
A.C. Aguiar Pinto
◽
T.M. Britto
◽
R. Bunchaft
◽
F. Pascoal
◽
F.S.S. da Rosa
Keyword(s):
Scalar Field
◽
Boundary Conditions
◽
Mixed Boundary
◽
Casimir Effect
◽
Mixed Boundary Conditions
◽
Massive Scalar
◽
Massive Scalar Field
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Charged Black Holes with Massive Scalar Field
10.1063/1.3265326
◽
2009
◽
Author(s):
D. Georgieva
◽
I. Stefanov
◽
M. Todorov
◽
S. Yazadjiev
◽
Michail D. Todorov
◽
...
Keyword(s):
Black Holes
◽
Scalar Field
◽
Massive Scalar
◽
Massive Scalar Field
◽
Charged Black Holes
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