2002
DOI: 10.1016/s0550-3213(01)00571-5
|View full text |Cite
|
Sign up to set email alerts
|

Cosmic string configuration in the supersymmetric CSKR theory

Abstract: We study a cosmic string solution of an N=1-supersymmetric version of the Cremmer-Scherk-Kalb-Ramond (CSKR) model coupled to scalars and fermions. The 2-form gauge potential is proposed to couple non-minimally to matter, here described by a chiral scalar superfield. The important outcome is that supersymmetry is kept exact in the core and it may also hold in the exterior region of the string. We contemplate the configurations of the bosonic sector and we check that the solutions saturate the Bogomolǹyi bound. … Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

0
22
0

Year Published

2002
2002
2015
2015

Publication Types

Select...
8
1

Relationship

0
9

Authors

Journals

citations
Cited by 16 publications
(22 citation statements)
references
References 35 publications
(32 reference statements)
0
22
0
Order By: Relevance
“…While in [4] only the free theory has been considered, we study here its coupling to a chiral matter. Classical aspects of this model were discussed in [5]. An alternative coupling for the linear superfield and tensor multiplet has been discussed in [6], where some of its string-related aspects were considered (for applications of this multiplet see also the references therein).…”
Section: Introductionmentioning
confidence: 99%
“…While in [4] only the free theory has been considered, we study here its coupling to a chiral matter. Classical aspects of this model were discussed in [5]. An alternative coupling for the linear superfield and tensor multiplet has been discussed in [6], where some of its string-related aspects were considered (for applications of this multiplet see also the references therein).…”
Section: Introductionmentioning
confidence: 99%
“…It is well-known, however, that the exchange of a scalar and a s = 1 boson between sources of equal charges yields attractive and repulsive interactions, respectively, therefore justifying the aforementioned sign difference between Eqs. (26) and (28).…”
Section: The Potentialsmentioning
confidence: 99%
“…3, it is important to obtain suitable spin operators in order to obtain the propagators of the model. The spin operators that act on an anti-symmetric 2-form are (15) which are anti-symmetric generalizations of the projectors θ μν and ω μν [28][29][30]. The comma indicates that we have anti-symmetry in changes μ ↔ ν or ρ ↔ σ .…”
Section: The Propagatorsmentioning
confidence: 99%
“…Then, we introduce the following gauge invariant action involving coupling of matter and gauge fields [8] studied also in [9] within the cosmic strings context:…”
Section: The Modelmentioning
confidence: 99%