Phantom black holes and critical phenomena

被引:16
作者
Azreg-Ainou, Mustapha [1 ]
Marques, Glauber T. [2 ]
Rodrigues, Manuel E. [3 ]
机构
[1] Baskent Univ, Fac Engn, TR-06490 Ankara, Turkey
[2] Univ Fed Rural Amazonia ICIBE LASIC, BR-66077901 Belem, Para, Brazil
[3] Fed Univ Para, Fac Ciencias Exatas & Tecnol, BR-68440000 Abaetetuba, Para, Brazil
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2014年 / 07期
关键词
modified gravity; GR black holes; dark energy theory; CRITICAL-BEHAVIOR; THERMODYNAMICS; CLASSIFICATION;
D O I
10.1088/1475-7516/2014/07/036
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We consider the two classes cosh and sinh of normal and phantom black holes of Einstein-Maxwell-dilaton theory. The thermodynamics of these holes is characterized by heat capacities that may have both signs depending on the parameters of the theory. Leaving aside the normal Reissner-Nordstrom black hole, it is shown that only some phantom black holes of both classes exhibit critical phenomena. The two classes share a nonextremality, but special, critical point where the transition is continuous and the heat capacity, at constant charge, changes sign with an infinite discontinuity. This point yields a classification scheme for critical points. It is concluded that the two unstable and stable phases coexist on one side of the criticality state and disappear on the other side, that is, there is no configuration where only one phase exists. The sinh class has an extremality critical point where the entropy diverges. The transition from extremality to nonextremality with the charge held constant is accompanied by a loss of mass and an increase in the temperature. A special case of this transition is when the hole is isolated (microcanonical ensemble), it will evolve by emission of energy, which results in a decrease of its mass, to the final state of minimum mass and vanishing heat capacity. The Ehrenfest scheme of classification is inaccurate in this case but the generalized one due to Hilfer leads to conclude that the transition is of order less than unity. Fluctuations near criticality are also investigated.
引用
收藏
页数:23
相关论文
共 66 条
  • [1] Large N field theories, string theory and gravity
    Aharony, O
    Gubser, SS
    Maldacena, J
    Ooguri, H
    Oz, Y
    [J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 2000, 323 (3-4): : 183 - 386
  • [2] Is the semi-classical analysis valid for extreme black holes?
    Alvarenga, FG
    Batista, AB
    Fabris, JC
    Marques, GT
    [J]. PHYSICS LETTERS A, 2003, 320 (2-3) : 83 - 94
  • [3] Non-minimally coupled scalar fields and isolated horizons
    Ashtekar, A
    Corichi, A
    Sudarsky, D
    [J]. CLASSICAL AND QUANTUM GRAVITY, 2003, 20 (15) : 3413 - 3425
  • [4] Light paths of normal and phantom Einstein-Maxwell-dilaton black holes
    Azreg-Ainou, Mustapha
    [J]. PHYSICAL REVIEW D, 2013, 87 (02)
  • [5] Phantom black holes and sigma models
    Azreg-Ainou, Mustapha
    Clement, Gerard
    Fabris, Julio C.
    Rodrigues, Manuel E.
    [J]. PHYSICAL REVIEW D, 2011, 83 (12)
  • [6] Critical behavior of Born-Infeld AdS black holes in higher dimensions
    Banerjee, Rabin
    Roychowdhury, Dibakar
    [J]. PHYSICAL REVIEW D, 2012, 85 (10):
  • [7] Critical phenomena in Born-Infeld AdS black holes
    Banerjee, Rabin
    Roychowdhury, Dibakar
    [J]. PHYSICAL REVIEW D, 2012, 85 (04):
  • [8] Glassy phase transition and stability in black holes
    Banerjee, Rabin
    Modak, Sujoy Kumar
    Samanta, Saurav
    [J]. EUROPEAN PHYSICAL JOURNAL C, 2010, 70 (1-2): : 317 - 328
  • [9] Barlow AM, 2005, PHYS REV D, V72, DOI [10.1103/PhysRevD.72.024008, 10.1103/PhysRevLett.72.024008]