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Tachyonic Field Coupled with Global Monopole
by
Rahaman, F.
, Samanta, B
, Raychaudhuri, B.
, Mondal, Aditya S.
, Sarkar, Subrato
in
Einstein equations
/ Elementary Particles
/ Gravitational fields
/ Mathematical and Computational Physics
/ Orbits
/ Phase transitions
/ Physics
/ Physics and Astronomy
/ Quantum Field Theory
/ Quantum Physics
/ Relativity
/ Scalars
/ Spacetime
/ Symmetry
/ Theoretical
2024
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Tachyonic Field Coupled with Global Monopole
by
Rahaman, F.
, Samanta, B
, Raychaudhuri, B.
, Mondal, Aditya S.
, Sarkar, Subrato
in
Einstein equations
/ Elementary Particles
/ Gravitational fields
/ Mathematical and Computational Physics
/ Orbits
/ Phase transitions
/ Physics
/ Physics and Astronomy
/ Quantum Field Theory
/ Quantum Physics
/ Relativity
/ Scalars
/ Spacetime
/ Symmetry
/ Theoretical
2024
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Do you wish to request the book?
Tachyonic Field Coupled with Global Monopole
by
Rahaman, F.
, Samanta, B
, Raychaudhuri, B.
, Mondal, Aditya S.
, Sarkar, Subrato
in
Einstein equations
/ Elementary Particles
/ Gravitational fields
/ Mathematical and Computational Physics
/ Orbits
/ Phase transitions
/ Physics
/ Physics and Astronomy
/ Quantum Field Theory
/ Quantum Physics
/ Relativity
/ Scalars
/ Spacetime
/ Symmetry
/ Theoretical
2024
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Journal Article
Tachyonic Field Coupled with Global Monopole
2024
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Overview
As the early universe expanded, phase transitions occurred which resulted in the formation of different types of topological defects. Specifically, the self-coupling scalar field triplet
ϕ
a
was responsible for the creation of global monopoles, which are massive objects that arise during these phase transitions. The initial global symmetry of
O
(3) undergoes a process of spontaneous breaking, resulting in U(1) symmetry. In this paper we describe a model of global monopole consisting of the Higgs triplet of scalar fields with Tachyonic fluid described by the relativistic Lagrangian
L
Tach
=
-
V
(
ϕ
a
)
1
+
g
μ
ν
∂
μ
ϕ
a
∂
ν
ϕ
a
. In the weak field approximation, we were able to discover the solution for the scalar field and space-time produced by the global monopole and the Einstein equation that emerges from these scenario exhibits a high degree of non-linearity. Our investigation focused on determining whether the global monopole produces gravitational pull on a test particle that is in motion within its spacetime. Finally, we have calculated the bending of light due to gravitational field of this global monopole.
Publisher
Springer US,Springer Nature B.V
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