2017
DOI: 10.1016/j.jheap.2017.02.001
|View full text |Cite
|
Sign up to set email alerts
|

Dark matter candidates, helicity effects and new affine gravity with torsion

Abstract: The cross section for neutrino helicity spin-flip obtained from a new f (R, T ) model of gravitation with dynamic torsion field is phenomenologically analyzed. To this end, due to the logarithmical energy dependence of the cross section, the relation with the axion decay constant fa (Peccei-Quinn parameter) is used. Consequently the link with the phenomenological energy/mass window is found from the astrophysical and high energy viewpoints. The highest helicity spin-flip cross-sectional values presented in thi… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

0
6
0

Year Published

2017
2017
2021
2021

Publication Types

Select...
8

Relationship

2
6

Authors

Journals

citations
Cited by 13 publications
(6 citation statements)
references
References 58 publications
(87 reference statements)
0
6
0
Order By: Relevance
“…In particle physics more in general, high-energy experimental constraints on torsion have been placed, especially in [72][73][74][75][76]. Going to cosmology, dark matter has also been studied in the presence of torsion: after the already-mentioned [45], the reader may find it interesting to also have a look at [77][78][79][80][81]. As for the problem of singularity formation during the Big Bang, the following references may be of help [82][83][84][85][86].…”
Section: Discussionmentioning
confidence: 99%
“…In particle physics more in general, high-energy experimental constraints on torsion have been placed, especially in [72][73][74][75][76]. Going to cosmology, dark matter has also been studied in the presence of torsion: after the already-mentioned [45], the reader may find it interesting to also have a look at [77][78][79][80][81]. As for the problem of singularity formation during the Big Bang, the following references may be of help [82][83][84][85][86].…”
Section: Discussionmentioning
confidence: 99%
“…In [25] the cross section for neutrino helicity spin flip obtained from this type of f (R; T ) model of gravitation with dynamic torsion field introduced by us in [16], was phenomenologically analyzed using the relation with the axion decay constant f a (Peccei-Quinn parameter)…”
mentioning
confidence: 99%
“…In previous references, the authors have introduced a unified model based on a non-Riemannian geometry containing a dynamic antisymmetric torsion that admits the same results of GR and SM already proven, but also satisfactorily solves problems that GR and SM present difficulties or inconsistencies. Some of those problems that were satisfactorily treated in the context of this new formulation were the determination of the mass of the axion [12], violation of CP of the neutrino [14], primordial magnetogenesis [10], etc. In this work we calculate the equations controlling the stellar magnetospheres of compact objects in particular, in this new context.…”
Section: Introduction To the Problemmentioning
confidence: 99%
“…[10][11][12] and beyond the standard model (SM). Extending previous approaches, holding for compact objects/black hole axisymmetric geometries having into account effect of space-time curvature, the purpose of this work is the formulation of a generalized Grad-Shafranov (GGS)[2][1][3][4] equation based in a non-…”
mentioning
confidence: 99%