Fri - 09/05/25

There is no new related paper today

There is no new related paper today

  1. [] - Title: Unveiling horizons in quantum critical collapse - Marija Tomašević, Chih-Hung Wu

Thu - 09/04/25

There is no new related paper today

There is no new related paper today

  1. [] - Title: Deflection Angle of Regular Black Holes in Nonlinear Electrodynamics: Gauss-Bonnet Theorem, Time Delay, Shadow, and Greybody Bound - Susmita Sarkar, Nayan Sarkar, Hasrat Hussian Shah, Pankaj Balo, Farook Rahaman

Wed - 09/03/25

**Title:

      Loopy Black-Hole Remnants**  - **Authors:** Asier Alonso-Bardaji  - **Subjects:** Subjects: General Relativity and Quantum Cosmology (gr-qc)  - **Arxiv link:** [https://arxiv.org/abs/](https://arxiv.org/abs/)  - **Abstract**  The quantized area predicted by loop quantum gravity suggests the existence of a lower bound for black-hole horizons. We prove this intuition within a covariant effective model for spherical loop quantum gravity, where nonsingular quasi-static black holes evaporate until their horizons attain the smallest positive eigenvalue of the area operator. Consistent with the third law of black-hole thermodynamics, this final state -- characterized by vanishing temperature and entropy -- cannot be realized in finite time. The process thus leads to the formation of stable remnants, whose estimated masses are approximately 20.94$\mu$g, lying in the Planck regime.

There is no new related paper today

Tue - 09/02/25

**Title:

      Loopy Black-Hole Remnants**  - **Authors:** Asier Alonso-Bardaji  - **Subjects:** Subjects: General Relativity and Quantum Cosmology (gr-qc)  - **Arxiv link:** [https://arxiv.org/abs/](https://arxiv.org/abs/)  - **Abstract**  The quantized area predicted by loop quantum gravity suggests the existence of a lower bound for black-hole horizons. We prove this intuition within a covariant effective model for spherical loop quantum gravity, where nonsingular quasi-static black holes evaporate until their horizons attain the smallest positive eigenvalue of the area operator. Consistent with the third law of black-hole thermodynamics, this final state -- characterized by vanishing temperature and entropy -- cannot be realized in finite time. The process thus leads to the formation of stable remnants, whose estimated masses are approximately 20.94$\mu$g, lying in the Planck regime.

There is no new related paper today

Mon - 09/01/25

**Title:

      Loopy Black-Hole Remnants**  - **Authors:** Asier Alonso-Bardaji  - **Subjects:** Subjects: General Relativity and Quantum Cosmology (gr-qc)  - **Arxiv link:** [https://arxiv.org/abs/](https://arxiv.org/abs/)  - **Abstract**  The quantized area predicted by loop quantum gravity suggests the existence of a lower bound for black-hole horizons. We prove this intuition within a covariant effective model for spherical loop quantum gravity, where nonsingular quasi-static black holes evaporate until their horizons attain the smallest positive eigenvalue of the area operator. Consistent with the third law of black-hole thermodynamics, this final state -- characterized by vanishing temperature and entropy -- cannot be realized in finite time. The process thus leads to the formation of stable remnants, whose estimated masses are approximately 20.94$\mu$g, lying in the Planck regime.

There is no new related paper today

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