Accelerating black holes, spin-$\frac32$ fields and C-metric
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Publication:5249393
DOI10.1142/S0217732315500443zbMath1310.83021arXiv1404.7489MaRDI QIDQ5249393
Hai Lin, Shing Tung Yau, Khalid Saifullah
Publication date: 5 May 2015
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1404.7489
black holesgeneral relativity\(C\)-metricRarita-Schwinger operatoranalysis on Riemannian manifoldsquantum fields on curved manifoldsRarita-Schwinger differential equationspin-\(\frac{3}{2}\) fields
Black holes (83C57) Spinor and twistor methods in general relativity and gravitational theory; Newman-Penrose formalism (83C60)
Related Items (2)
Quasinormal modes of C-metric from SCFTs ⋮ Effect of quantum gravity on the stability of black holes
Cites Work
- Particle creation by black holes
- Temporal contribution to gravitational WKB-like calculations
- Decay rates and probability estimates for massive Dirac particles in the Kerr-Newman black hole geometry
- The interpretation of the \(C\) metric. The charged case when \(e^ 2\leq m^ 2\)
- Dirac particles tunneling from BTZ black hole
- Emission of scalar particles from cylindrical black holes
- Co-accelerated particles in the C-metric
- SOME APPLICATIONS OF A SIMPLE STATIONARY LINE ELEMENT FOR THE SCHWARZSCHILD GEOMETRY
- Radiation via tunnelling in the charged BTZ black hole
- Global aspects of accelerating and rotating black hole spacetimes
- Interpreting the C -metric
- Fermions tunnelling from black holes
- Black hole in three-dimensional spacetime
- Hawking Radiation As Tunneling
- On a Theory of Particles with Half-Integral Spin
- Quantum tunneling from three-dimensional black holes
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