On the thermodynamics of the black hole and hairy black hole transitions in the asymptotically flat spacetime with a box
arXiv:1708.01411 · doi:10.1140/epjc/s10052-018-5652-0
Abstract
We study the asymptotically flat quasi-local black hole/hairy black hole model with nonzero mass of the scalar filed. We disclose effects of the scalar mass on transitions in a grand canonical ensemble with condensation behaviors of a parameter , which is similar to approaches in holographic theories. We find that more negative scalar mass makes the phase transition easier to happen. We also obtain an analytical relation around the critical phase transition points implying a second order phase transition. Besides the parameter , we show that metric solutions can be used to disclose properties of transitions. In this work, we observe that phase transitions in a box are strikingly similar to holographic transitions in the AdS gravity and the similarity provides insights into holographic theories.
12 pages, 6 figures. Accepted for publication in EPJC. arXiv admin note: text overlap with arXiv:1705.08694
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