2018
DOI: 10.1134/s0202289318010085
|View full text |Cite
|
Sign up to set email alerts
|

Statistical Cosmological Fermion Systems with Phantom Scalar Interaction of Particles

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

0
31
0

Year Published

2019
2019
2021
2021

Publication Types

Select...
6

Relationship

3
3

Authors

Journals

citations
Cited by 22 publications
(31 citation statements)
references
References 18 publications
0
31
0
Order By: Relevance
“…As was noted in [7][8][9], the presence of a phantom field in the cosmological model for small values of the potential of the phantom field leads to the appearance of phantom bursts of super-acceleration, characterized by large values of Ω. Figure 13 shows such bursts.…”
Section: Bursts Of Cosmological Accelerationmentioning
confidence: 61%
See 2 more Smart Citations
“…As was noted in [7][8][9], the presence of a phantom field in the cosmological model for small values of the potential of the phantom field leads to the appearance of phantom bursts of super-acceleration, characterized by large values of Ω. Figure 13 shows such bursts.…”
Section: Bursts Of Cosmological Accelerationmentioning
confidence: 61%
“…Cosmological evolution of a scalar doublet with the parameters listed in Eq. (4) and the initial conditions listed in Eq (7). in the plane of the potentials {Φ, ϕ}.…”
mentioning
confidence: 99%
See 1 more Smart Citation
“…The mathematical models of scalar fields constructed in this way were applied to a study of the cosmological evolution of systems of interacting particles and scalar fields, both of the canonical and phantom types [21][22][23]. These studies revealed unique features of the cosmological evolution of a plasma with phantom scalar particles' interaction, such as the existence of giant bursts of cosmological acceleration, the presence of a plateau with constant acceleration, and other anomalies that sharply distinguish the behavior of cosmological models with a phantom scalar field from models with a canonical scalar field.…”
Section: Introductionmentioning
confidence: 99%
“…The paper [23] analyzes the types of behavior of cosmological models based on a scalarly charged system of degenerate fermions with a quadratic interaction potential and identifies 4 main types of behavior that allow, among other things, for intermediate nonrelativistic and ultrarelativistic expansion stages. Let us note that intermediate nonrelativistic stages of cosmological expansion are a necessary condition for the emergence of a large-scale structure of the Universe as a result of the development of gravitational instability.…”
Section: Introductionmentioning
confidence: 99%