Scattering of charged massive scalar waves by Kerr-Newman black holes Article Swipe
The scattering of charged massive scalar waves by Kerr-Newman black holes, with incidence along the equatorial plane, is investigated in this work. The differential scattering cross section is computed using the partial wave method, with the forward divergence handled via the series reduction technique. For the first time, we systematically examine the influence of the black hole charge, electromagnetic interactions, and field mass on the equatorial cross section. Our results reveal that regardless of whether the electromagnetic interaction is present or not, the frame-dragging effect shifts the glory away from the exact backward direction and can place interference minima there, contrasting with the on-axis scattering case. The average scattered flux intensity at the medium to large scattering angles exhibits a large enhancement as the Lorentz attraction or field mass increases, particularly in the slowly rotating regime, with the enhancement being frequency-dependent. When superradiance occurs, we observe that the cross section in the prograde scattering angles ($\sim 135^{\circ} < ϕ< 270^{\circ}$) increases as the black hole spin increases, due to enhanced prograde partial wave contributions. Meanwhile, the superradiant scattering cross section increases in all (except the forward) directions when the Lorentz force becomes more repulsive. These findings highlight unique equatorial-plane signatures of charged, rotating spacetimes, distinguishing them from prior on-axis analyses.
Related Topics
Concepts
Physics
Scattering
Quantum electrodynamics
Superradiance
Black hole (networking)
Scalar field
Scattering length
Electromagnetic radiation
Scattering theory
Scattering amplitude
Classical mechanics
Scalar (mathematics)
Rayleigh scattering
Lorentz transformation
Electromagnetic field
Field (mathematics)
Forward scatter
Light scattering
Optical theorem
Computational physics
Mott scattering
Cross section (physics)
Scattering cross-section
Quantum mechanics
Anomalous scattering
Hawking radiation
Rainbow
Spin-flip
Metadata
- Type
- article
- Landing Page
- http://arxiv.org/abs/2511.21318
- https://arxiv.org/pdf/2511.21318
- OA Status
- green
- OpenAlex ID
- https://openalex.org/W7106861354
All OpenAlex metadata
Raw OpenAlex JSON
- OpenAlex ID
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https://openalex.org/W7106861354Canonical identifier for this work in OpenAlex
- Title
-
Scattering of charged massive scalar waves by Kerr-Newman black holesWork title
- Type
-
articleOpenAlex work type
- Publication year
-
2025Year of publication
- Publication date
-
2025-11-26Full publication date if available
- Authors
-
Li Qian, Wang Qianchuan, Jia Jun-jiList of authors in order
- Landing page
-
https://arxiv.org/abs/2511.21318Publisher landing page
- PDF URL
-
https://arxiv.org/pdf/2511.21318Direct link to full text PDF
- Open access
-
YesWhether a free full text is available
- OA status
-
greenOpen access status per OpenAlex
- OA URL
-
https://arxiv.org/pdf/2511.21318Direct OA link when available
- Concepts
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Physics, Scattering, Quantum electrodynamics, Superradiance, Black hole (networking), Scalar field, Scattering length, Electromagnetic radiation, Scattering theory, Scattering amplitude, Classical mechanics, Scalar (mathematics), Rayleigh scattering, Lorentz transformation, Electromagnetic field, Field (mathematics), Forward scatter, Light scattering, Optical theorem, Computational physics, Mott scattering, Cross section (physics), Scattering cross-section, Quantum mechanics, Anomalous scattering, Hawking radiation, Rainbow, Spin-flipTop concepts (fields/topics) attached by OpenAlex
- Cited by
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0Total citation count in OpenAlex
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| abstract_inverted_index.charged, | 201 |
| abstract_inverted_index.computed | 28 |
| abstract_inverted_index.enhanced | 169 |
| abstract_inverted_index.exhibits | 118 |
| abstract_inverted_index.findings | 195 |
| abstract_inverted_index.forward) | 185 |
| abstract_inverted_index.prograde | 152, 170 |
| abstract_inverted_index.rotating | 134, 202 |
| abstract_inverted_index.section. | 67 |
| abstract_inverted_index.analyses. | 209 |
| abstract_inverted_index.direction | 93 |
| abstract_inverted_index.highlight | 196 |
| abstract_inverted_index.incidence | 12 |
| abstract_inverted_index.increases | 160, 180 |
| abstract_inverted_index.influence | 52 |
| abstract_inverted_index.intensity | 110 |
| abstract_inverted_index.reduction | 42 |
| abstract_inverted_index.scattered | 108 |
| abstract_inverted_index.Meanwhile, | 174 |
| abstract_inverted_index.attraction | 125 |
| abstract_inverted_index.directions | 186 |
| abstract_inverted_index.divergence | 37 |
| abstract_inverted_index.equatorial | 15, 65 |
| abstract_inverted_index.increases, | 129, 166 |
| abstract_inverted_index.regardless | 72 |
| abstract_inverted_index.repulsive. | 193 |
| abstract_inverted_index.scattering | 1, 24, 104, 116, 153, 177 |
| abstract_inverted_index.signatures | 199 |
| abstract_inverted_index.technique. | 43 |
| abstract_inverted_index.135^{\circ} | 156 |
| abstract_inverted_index.Kerr-Newman | 8 |
| abstract_inverted_index.contrasting | 100 |
| abstract_inverted_index.enhancement | 121, 138 |
| abstract_inverted_index.interaction | 77 |
| abstract_inverted_index.spacetimes, | 203 |
| abstract_inverted_index.differential | 23 |
| abstract_inverted_index.interference | 97 |
| abstract_inverted_index.investigated | 18 |
| abstract_inverted_index.particularly | 130 |
| abstract_inverted_index.superradiant | 176 |
| abstract_inverted_index.270^{\circ}$) | 159 |
| abstract_inverted_index.interactions, | 59 |
| abstract_inverted_index.superradiance | 142 |
| abstract_inverted_index.contributions. | 173 |
| abstract_inverted_index.distinguishing | 204 |
| abstract_inverted_index.frame-dragging | 83 |
| abstract_inverted_index.systematically | 49 |
| abstract_inverted_index.electromagnetic | 58, 76 |
| abstract_inverted_index.equatorial-plane | 198 |
| abstract_inverted_index.frequency-dependent. | 140 |
| cited_by_percentile_year | |
| countries_distinct_count | 0 |
| institutions_distinct_count | 3 |
| citation_normalized_percentile.value | 0.80589456 |
| citation_normalized_percentile.is_in_top_1_percent | False |
| citation_normalized_percentile.is_in_top_10_percent | False |