A new rotating axionic AdS₄ black hole dressed with a scalar field
Pith reviewed 2026-05-22 17:42 UTC · model grok-4.3
The pith
A new rotating axionic black hole in four-dimensional AdS space is constructed with a scalar field using a structural function that ensures thermodynamic consistency.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
The authors present a new four-dimensional rotating black hole that is axionically charged and dressed with a scalar field. This configuration is defined by a structural function that couples the axionic field with a scalar potential. The solution is characterized by one integration constant and two constant parameters. Using the Euclidean procedure, the thermodynamic quantities are derived in such a way that the first law of thermodynamics holds, suggesting applications to holographic models of superconductors with rotation.
What carries the argument
The structural function coupling the axionic field and the scalar potential, which defines the metric and field profiles to satisfy the field equations in AdS4.
If this is right
- The first law of thermodynamics is valid for this rotating axionic black hole with scalar field.
- The angular constant parameter plays a central role in exploring holographic superconductors.
- The configuration provides a framework for studying rotating systems in the context of AdS/CFT correspondence.
- The solution extends previous non-rotating cases by including rotation while maintaining consistency.
Where Pith is reading between the lines
- Such solutions could be extended to include charge or other matter fields to model more complex condensed matter systems.
- Investigating the phase transitions or transport properties in the dual theory might reveal new insights into rotating superconductors.
- Similar structural functions might be applicable to black holes in higher dimensions or different asymptotic spaces.
Load-bearing premise
A structural function coupling the axionic field and scalar potential can be chosen such that the resulting configuration solves the Einstein equations with matter in AdS4 and yields consistent thermodynamics.
What would settle it
A calculation showing that the proposed metric and fields fail to satisfy the Einstein equations for the given structural function or that the thermodynamic quantities violate the first law would disprove the existence of this solution.
Figures
read the original abstract
This paper presents a new four-dimensional axionically charged rotating black hole with a scalar field, which is defined by a structural function coupling the axionic field and a scalar potential. This configuration is characterized by an integration constant and two constant parameters. The thermodynamic quantities are obtained via the Euclidean procedure, where the validity of the first law of thermodynamics is ensured. These results indicate that the rotating configuration provides a useful framework for exploring holographic superconductors, where the angular constant parameter plays a central role.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. This paper presents a new four-dimensional axionically charged rotating black hole with a scalar field, defined by a structural function coupling the axionic field and a scalar potential. This configuration is characterized by an integration constant and two constant parameters. The thermodynamic quantities are obtained via the Euclidean procedure, where the validity of the first law of thermodynamics is ensured. These results indicate that the rotating configuration provides a useful framework for exploring holographic superconductors, where the angular constant parameter plays a central role.
Significance. If the solution satisfies the full Einstein-scalar-axion system in AdS4, it would constitute a new example of a rotating black hole with axionic charge and scalar dressing. Such solutions can be relevant for holographic models of superconductors that incorporate rotation. The Euclidean verification of the first law follows standard methods in the field, but its reliability hinges on the underlying solution being a genuine solution to the equations of motion.
major comments (2)
- The construction relies on introducing a structural function that couples the axionic field to a scalar potential so that the configuration solves the field equations. For the rotating ansatz this requires explicit verification that every component of the Einstein equations (including off-diagonal terms generated by the rotation) vanishes identically. The manuscript should provide the explicit metric ansatz, the form of the structural function, and a component-by-component check that G_μν − T_μν = 0 holds for the full rotating solution rather than only for the diagonal equations.
- Abstract and thermodynamics section: the assertion that the first law holds after the Euclidean computation is stated without explicit equations, derivations, or numerical checks. The on-shell Euclidean action, the resulting thermodynamic potentials, and the explicit verification that δM = TδS + ΩδJ + … should be displayed so that the consistency claim can be assessed directly.
minor comments (2)
- The physical roles of the two constant parameters and the integration constant should be clarified at the outset, including how they are fixed or constrained by the field equations versus by thermodynamic requirements.
- Notation for the structural function and the axionic/scalar fields should be introduced consistently in the equations of motion section to avoid ambiguity when the reader checks the solution.
Simulated Author's Rebuttal
We thank the referee for their thorough review and insightful comments on our manuscript. We address each of the major comments in detail below and outline the revisions we will make to improve the clarity and completeness of the presentation.
read point-by-point responses
-
Referee: The construction relies on introducing a structural function that couples the axionic field to a scalar potential so that the configuration solves the field equations. For the rotating ansatz this requires explicit verification that every component of the Einstein equations (including off-diagonal terms generated by the rotation) vanishes identically. The manuscript should provide the explicit metric ansatz, the form of the structural function, and a component-by-component check that G_μν − T_μν = 0 holds for the full rotating solution rather than only for the diagonal equations.
Authors: We appreciate the referee's emphasis on the need for explicit verification of the field equations for the rotating case. While the original manuscript focused on presenting the new solution and its thermodynamic properties, we acknowledge that a detailed component-by-component check, including off-diagonal terms, was not included. In the revised version, we will provide the explicit form of the metric ansatz, the structural function, and demonstrate that all components of the Einstein equations are satisfied identically for the full rotating solution. This will be added as a dedicated subsection to ensure the solution's validity is transparent. revision: yes
-
Referee: Abstract and thermodynamics section: the assertion that the first law holds after the Euclidean computation is stated without explicit equations, derivations, or numerical checks. The on-shell Euclidean action, the resulting thermodynamic potentials, and the explicit verification that δM = TδS + ΩδJ + … should be displayed so that the consistency claim can be assessed directly.
Authors: We agree that providing explicit derivations would strengthen the thermodynamics section. The manuscript states that the first law is satisfied following the Euclidean procedure, but we did not include the full expressions for the on-shell action or the step-by-step verification. In the revision, we will display the on-shell Euclidean action, derive the thermodynamic potentials explicitly, and show the verification of the first law, including the relation δM = TδS + ΩδJ + ΦδQ or similar, as appropriate for this system. This will allow readers to assess the consistency directly. revision: yes
Circularity Check
No significant circularity; derivation is a standard exact-solution construction.
full rationale
The paper introduces a metric ansatz for a rotating axionic AdS4 black hole coupled to a scalar field and defines a structural function that couples the axion to a scalar potential. Thermodynamic quantities are then computed from the Euclidean on-shell action, with explicit verification that the first law holds for the resulting mass, entropy, charge, and angular momentum. This is a conventional procedure for constructing and validating exact solutions in Einstein-scalar-axion theories: the functional form is selected so the field equations are satisfied, after which the solution is substituted back to confirm consistency. No step reduces a claimed prediction to a fitted input by construction, no uniqueness theorem is imported from self-citation to force the ansatz, and no external benchmark is replaced by a renaming. The central result remains an explicit, verifiable configuration whose validity can be checked independently against the Einstein equations with the given matter content.
Axiom & Free-Parameter Ledger
free parameters (2)
- integration constant
- two constant parameters
axioms (1)
- domain assumption Einstein gravity coupled to axion and scalar fields admits solutions in AdS4
invented entities (1)
-
structural function coupling axionic field and scalar potential
no independent evidence
Lean theorems connected to this paper
-
IndisputableMonolith/Foundation/AlexanderDuality.leanalexander_duality_circle_linking unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
rotating metric ansatz (6) with Nθ(r) and f(r) solving Gμν - Tμν = 0
What do these tags mean?
- matches
- The paper's claim is directly supported by a theorem in the formal canon.
- supports
- The theorem supports part of the paper's argument, but the paper may add assumptions or extra steps.
- extends
- The paper goes beyond the formal theorem; the theorem is a base layer rather than the whole result.
- uses
- The paper appears to rely on the theorem as machinery.
- contradicts
- The paper's claim conflicts with a theorem or certificate in the canon.
- unclear
- Pith found a possible connection, but the passage is too broad, indirect, or ambiguous to say the theorem truly supports the claim.
Forward citations
Cited by 1 Pith paper
-
Novel five-dimensional rotating Lifshitz black holes with electric and axionic charges
Exact 5D rotating Lifshitz black holes with electric and axionic charges were found and used to show that rotation weakens holographic superconductivity while higher z enhances it.
Reference graph
Works this paper leans on
-
[1]
Here, the equations of motion with respect to the metric gµν as well as the scalar field ϕ take the structure: Eµν := Gµν + Λgµν − T ϕ µν = 0, (3) Eϕ := □ϕ − ξRϕ − dU dϕ = 0, (4) where T ϕ µν = ∇µϕ∇νϕ − gµν 1 2 ∇σϕ∇σϕ + U(ϕ) + ξ gµν□ϕ2 − ∇µ∇νϕ2 + Gµνϕ2 . (5) This motivates the search for analogous rotating configurations in four dimensions; that is, start...
-
[2]
(11) For completeness, the explicit expressions for T ψ µν are provided in Appendix A
The equations of motion are given by Gµν := Eµν − T ψ µν = 0, Gϕ := Eϕ − dε dϕ(∇µψ∇µψ) = 0, Gψ = ∇µ (ε(ϕ)∇µψ) = 0,(10) where the corresponding contribution to the energy-momentum tensor takes the form: T ψ µν = ε(ϕ) ∇µψ∇νψ − 1 2 gµν∇σψ∇σψ . (11) For completeness, the explicit expressions for T ψ µν are provided in Appendix A. Firstly, following Refs. [40–...
-
[3]
(23) The coupling function ε(ϕ) (eq
, (22) 7 and F (ϕ) = 3 16 ln √ 6 − ϕ√ 6 + ϕ ! + 3 √ 6(ϕ2 + 4ϕ + 6)(ϕ2 − 4ϕ + 6)ϕ 4(ϕ2 − 6)2(ϕ2 + 6) . (23) The coupling function ε(ϕ) (eq. (17)) and the potential U(ϕ) (eqs. (21) and (22)-(23)) play a providential role in supporting the rotating configuration (see eqs. (6), (19)-(20)). It is important to emphasize that in an analogous way to the three-dim...
-
[4]
N. M. Bocharova, K. A. Bronnikov and V. N. Melnikov, Vestn. Mosk. Univ. Fiz. Astron. (1970) 6, 706-709
work page 1970
-
[5]
J. D. Bekenstein, Exact solutions of Einstein conformal scalar equations, Annals Phys. 82 (1974), 535-547 doi:10.1016/0003-4916(74)90124-9
-
[6]
J. D. Bekenstein, Black Holes with Scalar Charge , Annals Phys. 91 (1975), 75-82 doi:10.1016/0003-4916(75)90279-1
-
[7]
Israel, Event horizons in static vacuum space-times , Phys
W. Israel, Event horizons in static vacuum space-times , Phys. Rev. 164 (1967), 1776-1779 doi:10.1103/PhysRev.164.1776
-
[8]
Israel, Event horizons in static electrovac space-times , Commun
W. Israel, Event horizons in static electrovac space-times , Commun. Math. Phys. 8 (1968), 245-260 doi:10.1007/BF01645859
-
[9]
Carter, Axisymmetric Black Hole Has Only Two Degrees of Freedom , Phys
B. Carter, Axisymmetric Black Hole Has Only Two Degrees of Freedom , Phys. Rev. Lett. 26 (1971), 331-333 doi:10.1103/PhysRevLett.26.331 27
-
[10]
S. W. Hawking, Gravitational radiation from colliding black holes, Phys. Rev. Lett.26 (1971), 1344-1346 doi:10.1103/PhysRevLett.26.1344
-
[11]
K. A. Bronnikov and Y. N. Kireev, Instability of Black Holes with Scalar Charge , Phys. Lett. A 67 (1978), 95-96 doi:10.1016/0375-9601(78)90030-0
-
[12]
B. C. Xanthopoulos and T. E. Dialynas, Einstein gravity coupled to a massless confor- mal scalar field in arbitrary space-time dimensions , J. Math. Phys. 33 (1992), 1463-1471 doi:10.1063/1.529723
-
[13]
Klimcik, Search for the conformal scalar hair at arbitrary D , J
C. Klimcik, Search for the conformal scalar hair at arbitrary D , J. Math. Phys. 34 (1993), 1914-1926 doi:10.1063/1.530146
-
[14]
de Sitter black hole with a conformally coupled scalar field in four dimensions
C. Martinez, R. Troncoso and J. Zanelli, De Sitter black hole with a conformally coupled scalar field in four-dimensions , Phys. Rev. D 67 (2003), 024008 doi:10.1103/PhysRevD.67.024008 [arXiv:hep-th/0205319 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.67.024008 2003
-
[15]
A. M. Barlow, D. Doherty and E. Winstanley, Thermodynamics of de Sitter black holes with a conformally coupled scalar field , Phys. Rev. D 72 (2005), 024008 doi:10.1103/PhysRevD.72.024008 [arXiv:gr-qc/0504087 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.72.024008 2005
-
[16]
Conformally dressed black hole in 2+1 dimensions
C. Martinez and J. Zanelli, Conformally dressed black hole in (2+1)-dimensions , Phys. Rev. D 54 (1996), 3830-3833 doi:10.1103/PhysRevD.54.3830 [arXiv:gr-qc/9604021 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.54.3830 1996
-
[17]
Topological black holes dressed with a conformally coupled scalar field and electric charge
C. Martinez, J. P. Staforelli and R. Troncoso, Topological black holes dressed with a conformally coupled scalar field and electric charge , Phys. Rev. D 74 (2006), 044028 doi:10.1103/PhysRevD.74.044028 [arXiv:hep-th/0512022 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.74.044028 2006
-
[18]
Static black hole solutions with a self interacting conformally coupled scalar field
G. Dotti, R. J. Gleiser and C. Martinez, Static black hole solutions with a self interacting conformally coupled scalar field , Phys. Rev. D 77 (2008), 104035 doi:10.1103/PhysRevD.77.104035 [arXiv:0710.1735 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.77.104035 2008
-
[19]
Charged C-metric with conformally coupled scalar field
C. Charmousis, T. Kolyvaris and E. Papantonopoulos, Charged C-metric with confor- mally coupled scalar field , Class. Quant. Grav. 26 (2009), 175012 doi:10.1088/0264- 9381/26/17/175012 [arXiv:0906.5568 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0264- 2009
-
[20]
A. Anabalon and A. Cisterna, Asymptotically (anti) de Sitter Black Holes and Wormholes with a Self Interacting Scalar Field in Four Dimensions , Phys. Rev. D 85 (2012), 084035 doi:10.1103/PhysRevD.85.084035 [arXiv:1201.2008 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.85.084035 2012
-
[21]
Conformally coupled scalar black holes admit a flat horizon due to axionic charge
Y. Bardoux, M. M. Caldarelli and C. Charmousis, Conformally coupled scalar black holes ad- mit a flat horizon due to axionic charge , JHEP 09 (2012), 008 doi:10.1007/JHEP09(2012)008 28 [arXiv:1205.4025 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep09(2012)008 2012
-
[22]
(Super-)renormalizably dressed black holes
E. Ay´ on-Beato, M. Hassa¨ ıne and J. A. M´ endez-Zavaleta,(Super-)renormalizably dressed black holes , Phys. Rev. D 92 (2015) no.2, 024048 doi:10.1103/PhysRevD.92.024048 [arXiv:1506.02277 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.92.024048 2015
-
[23]
E. Ay´ on-Beato, M. Hassaine and P. A. S´ anchez,Non-Noetherian conformal Cheshire effect , Eur. Phys. J. C 85 (2025) no.3, 259 doi:10.1140/epjc/s10052-025-14011-5 [arXiv:2408.00086 [hep-th]]
-
[24]
E. Ay´ on-Beato and M. Hassaine,Non-Noetherian conformal scalar fields, Annals Phys. 460 (2024), 169567 doi:10.1016/j.aop.2023.169567 [arXiv:2305.09806 [hep-th]]
-
[25]
A. Cisterna, A. Neira-Gallegos, J. Oliva and S. C. Rebolledo-Caceres, Pleba´ nski-Demia´ nski solutions in quadratic gravity with conformally coupled scalar fields, Phys. Rev. D 103 (2021) no.6, 064050 doi:10.1103/PhysRevD.103.064050 [arXiv:2101.03628 [gr-qc]]
-
[26]
M. Bravo-Gaete, C. G. Gaete, L. Guajardo and S. G. Rodr´ ıguez, Towards the emer- gence of nonzero thermodynamical quantities for Lanczos-Lovelock black holes dressed with a scalar field , Phys. Rev. D 104 (2021) no.4, 044027 doi:10.1103/PhysRevD.104.044027 [arXiv:2103.15634 [gr-qc]]
-
[27]
Entropy for Asymptotically AdS_3 Black Holes
M. Natsuume and T. Okamura, Entropy for asymptotically AdS(3) black holes , Phys. Rev. D 62 (2000), 064027 doi:10.1103/PhysRevD.62.064027 [arXiv:hep-th/9911062 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.62.064027 2000
-
[28]
Rotating hairy black hole and its microscopic entropy in three spacetime dimensions
F. Correa, A. Fa´ undez and C. Mart´ ınez, Rotating hairy black hole and its micro- scopic entropy in three spacetime dimensions , Phys. Rev. D 87 (2013) no.2, 027502 doi:10.1103/PhysRevD.87.027502 [arXiv:1211.4878 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.87.027502 2013
-
[29]
Stationary axisymmetric spacetimes with a conformally coupled scalar field
M. Astorino, Stationary axisymmetric spacetimes with a conformally coupled scalar field , Phys. Rev. D 91 (2015), 064066 doi:10.1103/PhysRevD.91.064066 [arXiv:1412.3539 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.91.064066 2015
-
[30]
Integrability in conformally coupled gravity: Taub-NUT spacetimes and rotating black holes
Y. Bardoux, M. M. Caldarelli and C. Charmousis, Integrability in conformally cou- pled gravity: Taub-NUT spacetimes and rotating black holes , JHEP 05 (2014), 039 doi:10.1007/JHEP05(2014)039 [arXiv:1311.1192 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep05(2014)039 2014
-
[31]
New Charged Black Holes with Conformal Scalar Hair
A. Anabalon and H. Maeda, New Charged Black Holes with Conformal Scalar Hair , Phys. Rev. D 81 (2010), 041501 doi:10.1103/PhysRevD.81.041501 [arXiv:0907.0219 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.81.041501 2010
-
[32]
A class of rotating hairy black holes in arbitrary dimensions
C. Erices and C. Martinez, Rotating hairy black holes in arbitrary dimensions , Phys. Rev. D 97 (2018) no.2, 024034 doi:10.1103/PhysRevD.97.024034 [arXiv:1707.03483 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.97.024034 2018
-
[33]
O. Baake, M. F. Bravo Gaete and M. Hassaine, Spinning black holes for general- 29 ized scalar tensor theories in three dimensions , Phys. Rev. D 102 (2020) no.2, 024088 doi:10.1103/PhysRevD.102.024088 [arXiv:2005.10869 [hep-th]]
-
[34]
M. C´ ardenas, O. Fuentealba, C. Mart´ ınez and R. Troncoso,Gravity coupled to a scalar field from a Chern-Simons action: describing rotating hairy black holes and solitons with gauge fields, JHEP 02 (2023), 058 doi:10.1007/JHEP02(2023)058 [arXiv:2212.13094 [hep-th]]
-
[35]
J. Barrientos, A. Cisterna, C. Corral and M. Oyarzo, Gravitational instantons with conformally coupled scalar fields , JHEP 05 (2022), 110 doi:10.1007/JHEP05(2022)110 [arXiv:2202.13854 [hep-th]]
-
[36]
M. Bravo-Gaete, F. F. Santos and X. Zhang, Fortsch. Phys. 73 (2025) no.12, e70049 doi:10.1002/prop.70049 [arXiv:2510.23826 [hep-th]]
-
[37]
L. Zhao, W. Xu and B. Zhu, Novel rotating hairy black hole in (2+1)-dimensions , Commun. Theor. Phys. 61 (2014) no.4, 475-481 doi:10.1088/0253-6102/61/4/12 [arXiv:1305.6001 [gr- qc]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/0253-6102/61/4/12 2014
-
[38]
D. C. Zou, Y. Liu, B. Wang and W. Xu, Thermodynamics of rotating black holes with scalar hair in three dimensions , Phys. Rev. D 90 (2014) no.10, 104035 doi:10.1103/PhysRevD.90.104035 [arXiv:1408.2419 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.90.104035 2014
-
[39]
Rotating Topological Black Holes
D. Klemm, V. Moretti and L. Vanzo, Rotating topological black holes, Phys. Rev. D57 (1998), 6127-6137 [erratum: Phys. Rev. D 60 (1999), 109902] doi:10.1103/PhysRevD.60.109902 [arXiv:gr-qc/9710123 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.60.109902 1998
-
[40]
J. P. S. Lemos and V. T. Zanchin, Rotating charged black string and three-dimensional black holes , Phys. Rev. D 54 (1996), 3840-3853 doi:10.1103/PhysRevD.54.3840 [arXiv:hep- th/9511188 [hep-th]]
-
[41]
Shaping black holes with free fields
Y. Bardoux, M. M. Caldarelli and C. Charmousis, Shaping black holes with free fields , JHEP 05 (2012), 054 doi:10.1007/JHEP05(2012)054 [arXiv:1202.4458 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep05(2012)054 2012
-
[42]
M. M. Caldarelli, C. Charmousis and M. Hassa¨ ıne, AdS black holes with arbitrary scalar coupling, JHEP 10 (2013), 015 doi:10.1007/JHEP10(2013)015 [arXiv:1307.5063 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep10(2013)015 2013
-
[43]
Axionic black branes with conformal coupling
A. Cisterna, C. Erices, X. M. Kuang and M. Rinaldi, Axionic black branes with con- formal coupling , Phys. Rev. D 97 (2018) no.12, 124052 doi:10.1103/PhysRevD.97.124052 [arXiv:1803.07600 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.97.124052 2018
-
[44]
Axionic charged black branes with arbitrary scalar nonminimal coupling
A. Cisterna, L. Guajardo and M. Hassaine, Axionic charged black branes with arbitrary scalar nonminimal coupling, Eur. Phys. J. C 79 (2019) no.5, 418 [erratum: Eur. Phys. J. C 30 79 (2019) no.8, 710] doi:10.1140/epjc/s10052-019-6922-1 [arXiv:1901.00514 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1140/epjc/s10052-019-6922-1 2019
-
[45]
A simple holographic model of momentum relaxation
T. Andrade and B. Withers, A simple holographic model of momentum relaxation , JHEP 05 (2014), 101 doi:10.1007/JHEP05(2014)101 [arXiv:1311.5157 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep05(2014)101 2014
-
[46]
Thermoelectric DC conductivities from black hole horizons
A. Donos and J. P. Gauntlett, Thermoelectric DC conductivities from black hole horizons , JHEP 11 (2014), 081 doi:10.1007/JHEP11(2014)081 [arXiv:1406.4742 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep11(2014)081 2014
-
[47]
A. Donos and J. P. Gauntlett, Holographic Q-lattices , JHEP 04 (2014), 040 doi:10.1007/JHEP04(2014)040 [arXiv:1311.3292 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep04(2014)040 2014
-
[48]
Holographic superconductor with momentum relaxation and Weyl correction
Y. Ling and X. Zheng, Holographic superconductor with momentum relaxation and Weyl correction , Nucl. Phys. B 917 (2017), 1-18 doi:10.1016/j.nuclphysb.2017.01.026 [arXiv:1609.09717 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1016/j.nuclphysb.2017.01.026 2017
-
[49]
P. Wang, H. Wu and H. Yang, Holographic DC Conductivity for Backreacted Nonlin- ear Electrodynamics with Momentum Dissipation , Eur. Phys. J. C 79 (2019) no.1, 6 doi:10.1140/epjc/s10052-018-6503-8 [arXiv:1805.07913 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1140/epjc/s10052-018-6503-8 2019
-
[50]
Axionic black branes in the k-essence sector of the Horndeski model
A. Cisterna, M. Hassaine, J. Oliva and M. Rinaldi, Axionic black branes in the k-essence sector of the Horndeski model , Phys. Rev. D 96 (2017) no.12, 124033 doi:10.1103/PhysRevD.96.124033 [arXiv:1708.07194 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.96.124033 2017
-
[51]
DC conductivity with external magnetic field in hyperscaling violating geometry
N. Bhatnagar and S. Siwach, DC conductivity with external magnetic field in hy- perscaling violating geometry , Int. J. Mod. Phys. A 33 (2018) no.04, 1850028 doi:10.1142/S0217751X18500288 [arXiv:1707.04013 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1142/s0217751x18500288 2018
-
[52]
Black holes with Lambert W function horizons
M. Bravo Gaete, S. Gomez and M. Hassaine, Black holes with Lambert W function horizons , Eur. Phys. J. C 79 (2019) no.3, 200 doi:10.1140/epjc/s10052-019-6723-6 [arXiv:1901.09612 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1140/epjc/s10052-019-6723-6 2019
-
[53]
Hernandez-Vera, The lack of influence of the scalar hair on the DC conductivity , Phys
U. Hernandez-Vera, The lack of influence of the scalar hair on the DC conductivity , Phys. Rev. D 111 (2025) no.8, 084035 doi:10.1103/PhysRevD.111.084035 [arXiv:2412.19388 [hep- th]]
-
[54]
C. Corral, C. Erices, D. Flores-Alfonso and K. Lara, Phase transitions of black strings in dynamical Chern-Simons modified gravity , Phys. Rev. D 105 (2022) no.2, 024050 doi:10.1103/PhysRevD.105.024050 [arXiv:2111.00912 [hep-th]]
-
[55]
Static and rotating black strings in dynamical Chern-Simons modified gravity
A. Cisterna, C. Corral and S. del Pino, Static and rotating black strings in dynamical Chern–Simons modified gravity, Eur. Phys. J. C79 (2019) no.5, 400 doi:10.1140/epjc/s10052- 019-6910-5 [arXiv:1809.02903 [gr-qc]]. 31
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1140/epjc/s10052- 2019
-
[56]
E. Arratia, C. Corral, J. Figueroa and L. Sanhueza, Hairy Taub-NUT/bolt-AdS solutions in Horndeski theory, Phys. Rev. D 103 (2021) no.6, 064068 doi:10.1103/PhysRevD.103.064068 [arXiv:2010.02460 [hep-th]]
-
[57]
J. M. Maldacena, The Large N limit of superconformal field theories and supergravity , Adv. Theor. Math. Phys. 2 (1998), 231-252 doi:10.4310/ATMP.1998.v2.n2.a1 [arXiv:hep- th/9711200 [hep-th]]
-
[58]
H. Farahani, J. Maldacena, S. Sheikh-Jabbari, L. M. Krauss, S. Upadhyay, S. Mame- dov, L. G. Wang, J. Zhang, S. E. San and S. Masood, et al. Proceedings of the 3rd International Conference on Holography and its Applications (ICHA3 2024) , doi:10.22128/jhap.2024.003.0012
-
[59]
S. A. Hartnoll, C. P. Herzog and G. T. Horowitz, Building a Holographic Superconductor , Phys. Rev. Lett. 101 (2008), 031601 doi:10.1103/PhysRevLett.101.031601 [arXiv:0803.3295 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevlett.101.031601 2008
-
[60]
Critical magnetic field in AdS/CFT superconductor
E. Nakano and W. Y. Wen, Critical magnetic field in a holographic superconductor , Phys. Rev. D 78 (2008), 046004 doi:10.1103/PhysRevD.78.046004 [arXiv:0804.3180 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.78.046004 2008
-
[61]
S. A. Hartnoll, C. P. Herzog and G. T. Horowitz, Holographic Superconductors, JHEP 12 (2008), 015 doi:10.1088/1126-6708/2008/12/015 [arXiv:0810.1563 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1088/1126-6708/2008/12/015 2008
-
[62]
The Holographic Superconductor Vortex
M. Montull, A. Pomarol and P. J. Silva, The Holographic Superconductor Vortex, Phys. Rev. Lett. 103 (2009), 091601 doi:10.1103/PhysRevLett.103.091601 [arXiv:0906.2396 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevlett.103.091601 2009
-
[63]
Vortex lattice for a holographic superconductor
K. Maeda, M. Natsuume and T. Okamura, Vortex lattice for a holographic superconductor , Phys. Rev. D 81 (2010), 026002 doi:10.1103/PhysRevD.81.026002 [arXiv:0910.4475 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.81.026002 2010
-
[64]
Emergent Gauge Fields in Holographic Superconductors
O. Domenech, M. Montull, A. Pomarol, A. Salvio and P. J. Silva, Emergent Gauge Fields in Holographic Superconductors, JHEP 08 (2010), 033 doi:10.1007/JHEP08(2010)033 [arXiv:1005.1776 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep08(2010)033 2010
-
[65]
Flux Periodicities and Quantum Hair on Holographic Superconductors
M. Montull, O. Pujolas, A. Salvio and P. J. Silva, Flux Periodicities and Quan- tum Hair on Holographic Superconductors , Phys. Rev. Lett. 107 (2011), 181601 doi:10.1103/PhysRevLett.107.181601 [arXiv:1105.5392 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevlett.107.181601 2011
-
[66]
Magnetic Response in the Holographic Insulator/Superconductor Transition
M. Montull, O. Pujolas, A. Salvio and P. J. Silva, Magnetic Response in the Holographic Insulator/Superconductor Transition, JHEP 04 (2012), 135 doi:10.1007/JHEP04(2012)135 [arXiv:1202.0006 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep04(2012)135 2012
-
[67]
Holographic Superfluids and Superconductors in Dilaton-Gravity
A. Salvio, Holographic Superfluids and Superconductors in Dilaton-Gravity, JHEP 09 (2012), 32 134 doi:10.1007/JHEP09(2012)134 [arXiv:1207.3800 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1007/jhep09(2012)134 2012
-
[68]
A. Donos, J. P. Gauntlett and C. Pantelidou, Holographic Abrikosov Lattices , JHEP 07 (2020), 095 doi:10.1007/JHEP07(2020)095 [arXiv:2001.11510 [hep-th]]
-
[69]
M. de la Cruz-L´ opez, J. A. Herrera-Mendoza, R. Cartas-Fuentevilla and A. Herrera- Aguilar, Exploring the UV and IR of a type-II holographic superconductor using a dyonic black hole , Eur. Phys. J. Plus 139 (2024) no.9, 786 doi:10.1140/epjp/s13360-024-05585-2 [arXiv:2402.12476 [hep-th]]
-
[70]
C. Y. Xia, H. B. Zeng, Y. Tian, C. M. Chen and J. Zaanen, Holographic Abrikosov lattice: Vortex matter from black hole , Phys. Rev. D 105 (2022) no.2, L021901 doi:10.1103/PhysRevD.105.L021901 [arXiv:2111.07718 [hep-th]]
-
[71]
J. A. Herrera-Mendoza, D. F. Higuita-Borja, J. A. M´ endez-Zavaleta, A. Herrera-Aguilar and F. P´ erez-Rodr´ ıguez,Vortex structure deformation of rotating Lifshitz holographic su- perconductors, Phys. Rev. D 106 (2022) no.8, L081902 doi:10.1103/PhysRevD.106.L081902 [arXiv:2208.05988 [hep-th]]
-
[72]
M. de la Cruz-L´ opez, A. Herrera-Aguilar, D. Mart´ ınez-Carbajal and S. Pati˜ no-L´ opez,Non- commutative AdS black hole and the IR holographic superconductor, Eur. Phys. J. C85 (2025) no.10, 1103 doi:10.1140/epjc/s10052-025-14642-8 [arXiv:2411.05259 [hep-th]]
-
[73]
Holographic superconductors with $z=2$ Lifshitz scaling
Y. Bu, Holographic superconductors with z = 2 Lifshitz scaling , Phys. Rev. D 86 (2012), 046007 doi:10.1103/PhysRevD.86.046007 [arXiv:1211.0037 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.86.046007 2012
-
[74]
J. W. Lu, Y. B. Wu, P. Qian, Y. Y. Zhao and X. Zhang,Lifshitz Scaling Effects on Holographic Superconductors, Nucl. Phys. B 887 (2014), 112-135 doi:10.1016/j.nuclphysb.2014.08.001 [arXiv:1311.2699 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1016/j.nuclphysb.2014.08.001 2014
-
[75]
Holographic Lifshitz superconductors: Analytic solution
M. Natsuume and T. Okamura, Holographic Lifshitz superconductors: Analytic solution , Phys. Rev. D 97 (2018) no.6, 066016 doi:10.1103/PhysRevD.97.066016 [arXiv:1801.03154 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.97.066016 2018
-
[76]
Z. Zhao, Q. Pan and J. Jing, Notes on analytical study of holographic superconduc- tors with Lifshitz scaling in external magnetic field , Phys. Lett. B 735 (2014), 438-444 doi:10.1016/j.physletb.2014.06.065 [arXiv:1311.6260 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1016/j.physletb.2014.06.065 2014
- [77]
-
[78]
A Rotating Holographic Superconductor
J. Sonner, A Rotating Holographic Superconductor , Phys. Rev. D 80 (2009), 084031 doi:10.1103/PhysRevD.80.084031 [arXiv:0903.0627 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1103/physrevd.80.084031 2009
-
[79]
Holographic Superconductors in a Rotating Spacetime
K. Lin and E. Abdalla, Holographic Superconductors in a Rotating Spacetime, Eur. Phys. J. C 74 (2014) no.11, 3144 doi:10.1140/epjc/s10052-014-3144-4 [arXiv:1403.7407 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1140/epjc/s10052-014-3144-4 2014
-
[80]
Analytic investigation of rotating holographic superconductors
A. Srivastav and S. Gangopadhyay, Analytic investigation of rotating holographic su- perconductors, Eur. Phys. J. C 79 (2019) no.4, 340 doi:10.1140/epjc/s10052-019-6834-0 [arXiv:1902.01628 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv doi:10.1140/epjc/s10052-019-6834-0 2019
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.