2020
DOI: 10.1016/j.physletb.2020.135960
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An interacting fermion-antifermion pair in the spacetime background generated by static cosmic string

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Cited by 42 publications
(54 citation statements)
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“…Even though these spacetime backgrounds are locally flat [9][10][11] out of the intersection point, they are not flat when viewed globally [9][10][11]. Because of this feature, the cosmic strings can be responsible for several physical events in the universe [12][13][14][15]. The spacetime background of the cosmic string is characterized by parameter, which is angular deficit parameter depending on the linear mass density ( ) of the cosmic string [12][13][14][15].…”
Section: Introductionmentioning
confidence: 99%
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“…Even though these spacetime backgrounds are locally flat [9][10][11] out of the intersection point, they are not flat when viewed globally [9][10][11]. Because of this feature, the cosmic strings can be responsible for several physical events in the universe [12][13][14][15]. The spacetime background of the cosmic string is characterized by parameter, which is angular deficit parameter depending on the linear mass density ( ) of the cosmic string [12][13][14][15].…”
Section: Introductionmentioning
confidence: 99%
“…Because of this feature, the cosmic strings can be responsible for several physical events in the universe [12][13][14][15]. The spacetime background of the cosmic string is characterized by parameter, which is angular deficit parameter depending on the linear mass density ( ) of the cosmic string [12][13][14][15]. The gravitational [9][10][11][12][13][14] and electrostatic effects [12,15] of these topological defects on the dynamics of physical systems depend on the parameter .…”
Section: Introductionmentioning
confidence: 99%
See 3 more Smart Citations