Corrigendum: Scalar radiation emitted from a source rotating around a black hole (2000
                    <i>Class. Quantum Grav.</i>
                    <b>17</b>
                    19)

Crispino, Luís C. B.; Higuchi, Atsushi; Matsas, George E. A.

doi:10.1088/0264-9381/33/20/209502

Search citation statements

Order By: Relevance

Paper Sections

Select...

Introduction1

Citation Types

Supporting

Mentioning

Contrasting

Year Published

2017

2024

Publication Types

Select...

Article6

Relationship

Self Cite0

Independent6

Authors

Journals

Cited by 9 publications

(1 citation statement)

References 6 publications

(6 reference statements)

Supporting

Mentioning

Contrasting

Order By: Relevance

“…Recently, the framework of semiclassical gravity has been used at tree level to compute the (massless) scalar radiation of a point source in circular orbit around Reissner-Nordström [31], Schwarzschild [32][33][34] and Kerr black holes [35].…”

Section: Introductionmentioning

confidence: 99%

Scalar field radiation emitted by an accelerated scalar point source: A classical field theory approach

et al. 2019

View full text Add to dashboard Cite

In this paper we will use classical field theory to address the interaction of an accelerated point source with a non-massive Klein-Gordon-Fock (KGF) field in Minkowski spacetime. For this, initially, we obtain the KGF equation for the non-massive scalar field via lagrangian formalism and the scalar potential through Green's function formalism. Finally, we reach the expression of the power radiated by a point scalar source under the influence of this field and its covariant generalization.

show abstract

Section: Introductionmentioning

confidence: 99%

Scalar field radiation emitted by an accelerated scalar point source: A classical field theory approach

et al. 2019

View full text Add to dashboard Cite

show abstract

Geodesic synchrotron radiation in black hole spacetimes: Analytical investigation

2021

View full text Add to dashboard Cite

Scalar radiation from a source rotating around a regular black hole

Bernar

Crispino

2019

Phys. Rev. D

View full text Add to dashboard Cite

The scalar radiation emitted by a source in geodesic circular orbit around a regular Bardeen black hole is analyzed. We use the quantum field theory in curved spacetime framework to obtain the emitted power of radiation by computing the one-particle emission amplitude of scalar particles in the curved background. We compare our results to a similar setting in the spacetime of a Reissner-Nordström black hole.

show abstract

Corrigendum: Scalar radiation emitted from a source rotating around a black hole (2000 Class. Quantum Grav. 17 19)

Cited by 9 publications

References 6 publications

Scalar field radiation emitted by an accelerated scalar point source: A classical field theory approach

Scalar field radiation emitted by an accelerated scalar point source: A classical field theory approach

Geodesic synchrotron radiation in black hole spacetimes: Analytical investigation

Scalar radiation from a source rotating around a regular black hole

Contact Info

Product

Resources

About