Universal exponents of black hole phase transition at zero-temperature limit
Fuente:
arXiv
Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Preprint |
| Published: |
2025
|
| Subjects: | |
| Online Access: | |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866912517981208576 |
|---|---|
| author | Wei, Shao-Wen Wu, Shan-Ping Zhang, Yu-Peng Liu, Yu-Xiao |
| author_facet | Wei, Shao-Wen Wu, Shan-Ping Zhang, Yu-Peng Liu, Yu-Xiao |
| contents | In this work, we investigate the universal thermodynamic characteristics of black hole phase transitions at the zero-temperature limit. Our results reveal that, far below the critical point, the near zero-temperature region also exhibits universal properties. By employing the Maxwell equal area law and analyzing the coexistence curve of black hole phase transitions, we derive three universal exponents: $α=1$, $β=2$, and $γ=d-3$, where $d$ represents the spacetime dimension number. Furthermore, additional studies show that these exponents remain unchanged regardless of the black hole's charge and spin. These universal exponents provide valuable insights into enhancing our understanding of black hole thermodynamic phase transitions near zero temperature and shed light on the fundamental aspects of quantum gravity. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2507_10028 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Universal exponents of black hole phase transition at zero-temperature limit Wei, Shao-Wen Wu, Shan-Ping Zhang, Yu-Peng Liu, Yu-Xiao General Relativity and Quantum Cosmology High Energy Physics - Theory In this work, we investigate the universal thermodynamic characteristics of black hole phase transitions at the zero-temperature limit. Our results reveal that, far below the critical point, the near zero-temperature region also exhibits universal properties. By employing the Maxwell equal area law and analyzing the coexistence curve of black hole phase transitions, we derive three universal exponents: $α=1$, $β=2$, and $γ=d-3$, where $d$ represents the spacetime dimension number. Furthermore, additional studies show that these exponents remain unchanged regardless of the black hole's charge and spin. These universal exponents provide valuable insights into enhancing our understanding of black hole thermodynamic phase transitions near zero temperature and shed light on the fundamental aspects of quantum gravity. |
| title | Universal exponents of black hole phase transition at zero-temperature limit |
| topic | General Relativity and Quantum Cosmology High Energy Physics - Theory |
| url | https://arxiv.org/abs/2507.10028 |