Entanglement in a model for Hawking radiation: An Application of Quadratic Algebras

Authors: Bindu A. Bambah, C. Mukku, T. Shreecharan, K. Siva Prasad

20 pages, 15 figures. revised version with one figure removed

Results of the summarizing process for the arXiv paper: 1204.2122v2

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, , , , In their paper titled "Entanglement in a Model for Hawking Radiation: An Application of Quadratic Algebras," authors Bindu A. Bambah, C. Mukku, T. Shreecharan, and K. Siva Prasad explore the use of quadratic polynomially deformed $su(1,1)$ and $su(2)$ algebras in model Hamiltonians to investigate the gravitational system involving black holes and radiation processes. By utilizing these mathematical tools, the researchers provide exact solutions for this complex system and analyze its long-term behavior. They also calculate bipartite entanglement entropies for different subsystems within their models, shedding light on potential modifications in the nature of Hawking radiation over time. Additionally, the paper delves into exploring superradiance within their model and drawing parallels with atomic Dicke superradiance to deepen our understanding of how certain phenomena observed in quantum systems can manifest in gravitational contexts. Overall, this research contributes to advancing our comprehension of complex gravitational systems by utilizing innovative mathematical frameworks and drawing connections to established principles in quantum physics.
AI-generated keywords: Entanglement

AI-generated Key Points

  • Authors explore the use of quadratic polynomially deformed $su(1,1)$ and $su(2)$ algebras in model Hamiltonians
  • Provide exact solutions for gravitational system involving black holes and radiation processes
  • Analyze long-term behavior of the system
  • Calculate bipartite entanglement entropies for different subsystems within models
  • Explore superradiance within their model and draw parallels with atomic Dicke superradiance
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Abstract: Quadratic polynomially deformed $su(1,1)$ and $su(2)$ algebras are utilised in model Hamiltonians to show how the gravitational system consisting of a black hole, infalling radiation and outgoing (Hawking) radiation can be solved exactly. The models allow us to study the long-time behaviour of the black hole and its outgoing modes. In particular, we calculate the bipartite entanglement entropies of subsystems consisting of a) infalling plus outgoing modes and b) black hole modes plus the infalling modes,using the Janus-faced nature of the model.The long-time behaviour also gives us glimpses of modifications in the character of Hawking radiation. Lastly, we study the phenomenon of superradiance in our model in analogy with atomic Dicke superradiance.

Submitted to arXiv on 10 Apr. 2012

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