Entropic route to Brown-York tensor: A unified framework for null and timelike hypersurfaces
Pith reviewed 2026-05-22 05:08 UTC · model grok-4.3
The pith
The Brown-York tensor emerges uniformly from the projection of canonical momentum derived from a shared entropy density on both timelike and null hypersurfaces.
A machine-rendered reading of the paper's core claim, the machinery that carries it, and where it could break.
Core claim
Using the same entropy density, the Brown-York tensor arises naturally as the projection of the canonical momentum conjugate to the normal vectors on the relevant hypersurface, thereby providing a common construction applicable to both timelike and null hypersurfaces. This perspective also offers insight into the structural differences of the null BY tensor, including its non-symmetric character. The formulation reproduces the expected equations of motion and the corresponding BY tensor in scalar-tensor theories while clarifying its non-conservation when the scalar field is non-minimally coupled.
What carries the argument
Padmanabhan's entropy functional, from which the canonical momentum conjugate to the normal is obtained and then projected to define the Brown-York tensor.
If this is right
- The identical entropy density supplies the Brown-York tensor for both timelike and null hypersurfaces.
- The non-symmetric character of the null Brown-York tensor follows directly from the projection structure.
- In scalar-tensor theories the same entropy route reproduces both the equations of motion and the associated Brown-York tensor.
- Non-conservation of the Brown-York tensor appears when the scalar field is non-minimally coupled.
Where Pith is reading between the lines
- The same entropy-based projection might generate other quasi-local quantities such as the Misner-Sharp mass or Komar integrals.
- Boundary terms in gravitational actions could be reinterpreted as entropy variations across a wider class of modified theories.
- Numerical checks on simple black-hole spacetimes with null boundaries could test whether the derived tensor satisfies the expected conservation properties.
Load-bearing premise
Padmanabhan's entropy functional remains valid and directly yields the conjugate momentum projection that defines the Brown-York tensor on both classes of hypersurface.
What would settle it
An explicit computation on a known null hypersurface in general relativity where the projected conjugate momentum from the entropy density fails to equal the standard Brown-York tensor expression would falsify the unified construction.
read the original abstract
Building on Padmanabhan's entropy functional, originally introduced to derive Einstein's equations and highlight the emergent nature of gravity, we demonstrate its robustness in a broader context. Using the same entropy density, we show that the Brown-York (BY) tensor arises naturally as the projection of the canonical momentum conjugate to the normal vectors on the relevant hypersurface, thereby providing a common construction applicable to both timelike and null hypersurfaces. This perspective also offers insight into the structural differences of the null BY tensor, including its non-symmetric character. We further extend the analysis to scalar-tensor theories, showing that the entropy-based formulation reproduces the expected equations of motion along with the corresponding BY tensor, and, clarifies its non-conservation in the presence of additional scalar field which is non-minimally coupled. Our results provide a coherent variational interpretation of quasi-local gravitational quantities and reveal a common underlying structure linking bulk dynamics and boundary momentum.
Editorial analysis
A structured set of objections, weighed in public.
Referee Report
Summary. The manuscript claims that Padmanabhan's entropy functional, previously used to derive Einstein's equations, directly yields the Brown-York tensor as the projection of the canonical momentum conjugate to the normal vectors. This construction is asserted to apply uniformly to both timelike and null hypersurfaces, to account for the non-symmetric character of the null BY tensor, and to extend to scalar-tensor theories where it reproduces the equations of motion while clarifying the non-conservation of the boundary term due to a non-minimally coupled scalar field.
Significance. If the central derivation holds without additional counterterms or redefinitions, the work would supply a thermodynamic route to quasi-local gravitational quantities that unifies bulk dynamics with boundary momentum across different hypersurface types. It would also strengthen the entropic interpretation of gravity by showing that the same functional produces both the field equations and the associated boundary tensor in modified theories.
major comments (2)
- [null hypersurface derivation] The central step for null hypersurfaces requires that the identical entropy density produces a well-defined conjugate momentum whose projection gives the BY tensor even though the induced metric is degenerate and n^a n_a = 0. The manuscript must supply the explicit variation and projection formulas (presumably in the section deriving the null case) to demonstrate that no extra renormalization is introduced by hand; otherwise the claim of a common construction without modification is not yet secured.
- [scalar-tensor theories] In the scalar-tensor extension, the non-conservation of the BY tensor is attributed to the non-minimal coupling. The manuscript should exhibit the precise term arising from the entropy variation that produces this non-conservation (e.g., the contribution proportional to the scalar gradient or its coupling function) so that the result can be checked against the standard field-equation derivation.
minor comments (2)
- [abstract] The abstract states that the BY tensor 'arises naturally' but does not indicate whether the projection operator is the same for timelike and null normals or whether a limiting procedure is used; a short clarifying sentence would help readers.
- [notation] Notation for the normal vector and its conjugate momentum should be checked for consistency between the timelike and null sections to avoid ambiguity when the same symbols are reused.
Simulated Author's Rebuttal
We thank the referee for the careful reading and constructive comments on our manuscript. These remarks help clarify the presentation of the unified entropic construction. We respond to each major comment below.
read point-by-point responses
-
Referee: [null hypersurface derivation] The central step for null hypersurfaces requires that the identical entropy density produces a well-defined conjugate momentum whose projection gives the BY tensor even though the induced metric is degenerate and n^a n_a = 0. The manuscript must supply the explicit variation and projection formulas (presumably in the section deriving the null case) to demonstrate that no extra renormalization is introduced by hand; otherwise the claim of a common construction without modification is not yet secured.
Authors: We thank the referee for highlighting the need for greater explicitness in the null case. The derivation proceeds by varying the same entropy functional with respect to the normal vector, obtaining the conjugate momentum, and projecting it onto the hypersurface using the (degenerate) induced metric. In the revised manuscript we will insert the explicit variation formula together with the projection step, confirming that the construction employs the identical entropy density and introduces no additional counterterms or renormalizations by hand. revision: yes
-
Referee: [scalar-tensor theories] In the scalar-tensor extension, the non-conservation of the BY tensor is attributed to the non-minimal coupling. The manuscript should exhibit the precise term arising from the entropy variation that produces this non-conservation (e.g., the contribution proportional to the scalar gradient or its coupling function) so that the result can be checked against the standard field-equation derivation.
Authors: We agree that displaying the explicit contribution will strengthen the exposition. The non-conservation originates from the variation of the entropy functional in the presence of the non-minimal coupling; the relevant term is proportional to the scalar-field gradient contracted with the coupling function. In the revised version we will isolate and write this term explicitly, allowing direct comparison with the divergence obtained from the bulk field equations. revision: yes
Circularity Check
No significant circularity; entropic derivation applies external functional to new boundary quantity
full rationale
The paper takes Padmanabhan's entropy functional (an external, previously published construction used to obtain Einstein equations) as given input and applies it to define the conjugate momentum whose projection yields the Brown-York tensor on both timelike and null hypersurfaces. This constitutes a variational reinterpretation rather than a redefinition of the input by construction. The extension to scalar-tensor theories follows the same logic without introducing fitted parameters or self-referential loops. No quoted step reduces the claimed result to a prior fit or to a self-citation whose validity is presupposed inside the paper. The framework is therefore self-contained against the external benchmark of Padmanabhan's entropy and standard hypersurface projections.
Axiom & Free-Parameter Ledger
axioms (1)
- domain assumption Padmanabhan's entropy functional remains valid for deriving the Brown-York tensor as conjugate momentum on hypersurfaces
Lean theorems connected to this paper
-
IndisputableMonolith/Cost/FunctionalEquation.leanwashburn_uniqueness_aczel unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
Using the same entropy density, we show that the Brown-York (BY) tensor arises naturally as the projection of the canonical momentum conjugate to the normal vectors on the relevant hypersurface
-
IndisputableMonolith/Foundation/AlphaCoordinateFixation.leanJ_uniquely_calibrated_via_higher_derivative unclear?
unclearRelation between the paper passage and the cited Recognition theorem.
the entropy functional for a timelike surface, denoted S[s], is postulated as S[s] = 1/16π ∫ √−g s[s] with s[s] = −(4P^{cd}_{ab} ∇_c s_a ∇_d s_b − T_{ab} s^a s^b)
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.
Reference graph
Works this paper leans on
-
[1]
Canonical variables for general relativity,
R. L. Arnowitt, S. Deser and C. W. Misner, “Canonical variables for general relativity,” Phys. Rev. 117, 1595-1602 (1960)
work page 1960
-
[2]
The Dynamics of General Relativity
R. L. Arnowitt, S. Deser and C. W. Misner, “The Dynamics of general relativity,” Gen. Rel. Grav. 40, 1997-2027 (2008) [arXiv:gr-qc/0405109 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1997
- [3]
-
[4]
Waves from axisymmetric isolated systems,” Proc. Roy. Soc. Lond. A269, 21-52 (1962) 19
work page 1962
-
[5]
Gravitational waves in general relativity. 8. Waves in asymptotically flat space-times,
R. K. Sachs, “Gravitational waves in general relativity. 8. Waves in asymptotically flat space-times,” Proc. Roy. Soc. Lond. A270, 103-126 (1962)
work page 1962
-
[6]
Covariant conservation laws in general relativity,
A. Komar, “Covariant conservation laws in general relativity,” Phys. Rev.113, 934-936 (1959)
work page 1959
-
[7]
Stability of Gravity with a Cosmological Constant,
L. F. Abbott and S. Deser, “Stability of Gravity with a Cosmological Constant,” Nucl. Phys. B195, 76-96 (1982)
work page 1982
-
[8]
Gravitational Energy in Quadratic Curvature Gravities
S. Deser and B. Tekin, “Gravitational energy in quadratic curvature gravities,” Phys. Rev. Lett.89, 101101 (2002) [arXiv:hep-th/0205318 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2002
-
[9]
Energy in Generic Higher Curvature Gravity Theories
S. Deser and B. Tekin, “Energy in generic higher curvature gravity theories,” Phys. Rev. D67, 084009 (2003) [arXiv:hep-th/0212292 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2003
-
[10]
Black Hole Entropy is Noether Charge
R. M. Wald, “Black hole entropy is the Noether charge,” Phys. Rev. D48, no.8, R3427-R3431 (1993) [arXiv:gr-qc/9307038 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1993
-
[11]
Some Properties of Noether Charge and a Proposal for Dynamical Black Hole Entropy
V. Iyer and R. M. Wald, “Some properties of Noether charge and a proposal for dynamical black hole entropy,” Phys. Rev. D50, 846-864 (1994) [arXiv:gr-qc/9403028 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1994
-
[12]
Relativistic equations for adiabatic, spherically symmetric gravita- tional collapse,
C. W. Misner and D. H. Sharp, “Relativistic equations for adiabatic, spherically symmetric gravita- tional collapse,” Phys. Rev.136, B571-B576 (1964)
work page 1964
-
[13]
Gravitational radiation in an expanding universe,
S. Hawking, “Gravitational radiation in an expanding universe,” J. Math. Phys.9, 598-604 (1968)
work page 1968
-
[14]
Gravitational Energy in Spherical Symmetry
S. A. Hayward, “Gravitational energy in spherical symmetry,” Phys. Rev. D53, 1938-1949 (1996) [arXiv:gr-qc/9408002 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1938
-
[15]
Quasilocal gravitational energy,
S. A. Hayward, “Quasilocal gravitational energy,” Phys. Rev. D49, 831-839 (1994) [arXiv:gr- qc/9303030 [gr-qc]]
-
[16]
Quasilocal mass and angular momentum in general relativity,
R. Penrose, “Quasilocal mass and angular momentum in general relativity,” Proc. Roy. Soc. Lond. A 381, 53-63 (1982)
work page 1982
-
[17]
Quasilocal Energy and Conserved Charges Derived from the Gravitational Action
J. D. Brown and J. W. York, Jr., “Quasilocal energy and conserved charges derived from the gravi- tational action,” Phys. Rev. D47, 1407-1419 (1993) [arXiv:gr-qc/9209012 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1993
-
[18]
Action and energy of the gravitational field,
J. D. Brown, S. R. Lau and J. W. York, Jr., “Action and energy of the gravitational field,” [arXiv:gr- qc/0010024 [gr-qc]]
-
[19]
Brown-York charges at null boundaries,
V. Chandrasekaran, E. E. Flanagan, I. Shehzad and A. J. Speranza, “Brown-York charges at null boundaries,” JHEP01, 029 (2022) doi:10.1007/JHEP01(2022)029 [arXiv:2109.11567 [hep-th]]
-
[20]
Hydro & thermo dynamics at causal boundaries, examples in 3d gravity,
H. Adami, A. Parvizi, M. M. Sheikh-Jabbari, V. Taghiloo and H. Yavartanoo, “Hydro & thermo dynamics at causal boundaries, examples in 3d gravity,” JHEP07, 038 (2023) doi:10.1007/JHEP07(2023)038 [arXiv:2305.01009 [hep-th]]
-
[21]
K. Bhattacharya and K. Bamba, “Boundary terms and Brown-York quasilocal parameters for scalar- tensor theory: A study on both timelike and null hypersurfaces,” Phys. Rev. D109, no.6, 064026 (2024) [arXiv:2307.06674 [gr-qc]]. 20
-
[22]
A note on gravity and fluid dynamic correspondence on a null hypersurface,
K. Bhattacharya, S. Dey and B. R. Majhi, “A note on gravity and fluid dynamic correspondence on a null hypersurface,” Phys. Scripta101, no.2, 025213 (2026) [arXiv:2411.06914 [gr-qc]]
-
[23]
T. Padmanabhan, “Gravity as elasticity of spacetime: A Paradigm to understand horizon thermody- namics and cosmological constant,” Int. J. Mod. Phys. D13, 2293-2298 (2004) [arXiv:gr-qc/0408051 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2004
-
[24]
Entropy of Null Surfaces and Dynamics of Spacetime
T. Padmanabhan and A. Paranjape, “Entropy of null surfaces and dynamics of spacetime,” Phys. Rev. D75, 064004 (2007) [arXiv:gr-qc/0701003 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2007
-
[25]
General Relativity: An Einstein Centenary Survey,
S. W. Hawking and W. Israel, “General Relativity: An Einstein Centenary Survey,” Univ. Pr., 1979, ISBN 978-0-521-29928-2
work page 1979
-
[26]
A Boundary Term for the Gravitational Action with Null Boundaries
K. Parattu, S. Chakraborty, B. R. Majhi and T. Padmanabhan, “A Boundary Term for the Gravita- tional Action with Null Boundaries,” Gen. Rel. Grav.48, no.7, 94 (2016) [arXiv:1501.01053 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[27]
Variational Principle for Gravity with Null and Non-null boundaries: A Unified Boundary Counter-term
K. Parattu, S. Chakraborty and T. Padmanabhan, “Variational Principle for Gravity with Null and Non-null boundaries: A Unified Boundary Counter-term,” Eur. Phys. J. C76, no.3, 129 (2016) [arXiv:1602.07546 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[28]
A Novel Derivation of the Boundary Term for the Action in Lanczos-Lovelock Gravity
S. Chakraborty, K. Parattu and T. Padmanabhan, “A Novel Derivation of the Boundary Term for the Action in Lanczos-Lovelock Gravity,” Gen. Rel. Grav.49, no.9, 121 (2017) [arXiv:1703.00624 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2017
-
[29]
Null boundary terms for Lanczos-Lovelock gravity
S. Chakraborty and K. Parattu, “Null boundary terms for Lanczos–Lovelock gravity,” Gen. Rel. Grav. 51, no.2, 23 (2019) [erratum: Gen. Rel. Grav.51, no.3, 47 (2019)] [arXiv:1806.08823 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[30]
Gravitational action with null boundaries
L. Lehner, R. C. Myers, E. Poisson and R. D. Sorkin, “Gravitational action with null boundaries,” Phys. Rev. D94, no.8, 084046 (2016) [arXiv:1609.00207 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[31]
Gravity Degrees of Freedom on a Null Surface
F. Hopfm¨ uller and L. Freidel, “Gravity Degrees of Freedom on a Null Surface,” Phys. Rev. D95, no.10, 104006 (2017) [arXiv:1611.03096 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2017
-
[32]
R. Oliveri and S. Speziale, “Boundary effects in General Relativity with tetrad variables,” Gen. Rel. Grav.52, no.8, 83 (2020) [arXiv:1912.01016 [gr-qc]]
-
[33]
S. Aghapour, G. Jafari and M. Golshani, “On variational principle and canonical structure of gravitational theory in double-foliation formalism,” Class. Quant. Grav.36, no.1, 015012 (2019) [arXiv:1808.07352 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[34]
Anomalies in gravitational charge algebras of null boundaries and black hole entropy,
V. Chandrasekaran and A. J. Speranza, “Anomalies in gravitational charge algebras of null boundaries and black hole entropy,” JHEP01, 137 (2021) [arXiv:2009.10739 [hep-th]]
-
[35]
Stress Tensor on Null Boundaries
G. Jafari, “Stress Tensor on Null Boundaries,” Phys. Rev. D99, no.10, 104035 (2019) [arXiv:1901.04054 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2019
-
[36]
Gravitation: Foundations and frontiers,
T. Padmanabhan, “Gravitation: Foundations and frontiers,” Cambridge University Press, 2014, ISBN 978-7-301-22787-9
work page 2014
-
[37]
Entropy density of spacetime and the Navier-Stokes fluid dynamics of null surfaces
T. Padmanabhan, “Entropy density of spacetime and the Navier-Stokes fluid dynamics of null sur- faces,” Phys. Rev. D83, 044048 (2011) [arXiv:1012.0119 [gr-qc]]. 21
work page internal anchor Pith review Pith/arXiv arXiv 2011
-
[38]
Action principle for the Fluid-Gravity correspondence and emergent gravity
S. Kolekar and T. Padmanabhan, “Action Principle for the Fluid-Gravity Correspondence and Emer- gent Gravity,” Phys. Rev. D85, 024004 (2012) [arXiv:1109.5353 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2012
-
[39]
A 3+1 perspective on null hypersurfaces and isolated horizons
E. Gourgoulhon and J. L. Jaramillo, “A 3+1 perspective on null hypersurfaces and isolated horizons,” Phys. Rept.423, 159-294 (2006) [arXiv:gr-qc/0503113 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[40]
A Relativist’s Toolkit: The Mathematics of Black-Hole Mechanics,
E. Poisson, “A Relativist’s Toolkit: The Mathematics of Black-Hole Mechanics,” Cambridge Univer- sity Press, 2009
work page 2009
-
[41]
T. Damour (1979),“Quelques propri´ et´ es m´ ecaniques, ´ electromagn´ etiques, thermodynamiques et quan- tiques des trous noirs”, Th` ese de doctorat d ´Etat, Universit´ e Paris 6; T. Damour (1982), “Surface effects in black hole physics, Proceedings of the Second Marcel Grossmann Meeting on General Rel- ativity”, Ed. R. Ruffini, North Holland, p. 587
work page 1979
-
[42]
S. Dey and B. R. Majhi, “Possible fluid interpretation and tidal force equation on a generic null hypersurface in Einstein-Cartan theory,” Phys. Rev. D106(2022) no.10, 104005 [arXiv:2206.11875 [gr-qc]]
-
[43]
Thermodynamic structure of a generic null surface and the zeroth law in scalar-tensor theory,
S. Dey, K. Bhattacharya and B. R. Majhi, “Thermodynamic structure of a generic null surface and the zeroth law in scalar-tensor theory,” Phys. Rev. D104, no.12, 124038 (2021) [arXiv:2105.07787 [gr-qc]]
-
[44]
S. Dey and B. R. Majhi, “Kinematics and dynamics of null hypersurfaces in the Einstein-Cartan spacetime and related thermodynamic interpretation,” Phys. Rev. D105(2022) no.6, 064047 [arXiv:2201.01131 [gr-qc]]
-
[45]
Gravitational field equations near an arbitrary null surface expressed as a thermodynamic identity
S. Chakraborty, K. Parattu and T. Padmanabhan, “Gravitational field equations near an arbitrary null surface expressed as a thermodynamic identity,” JHEP10, 097 (2015) [arXiv:1505.05297 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2015
-
[46]
Covariant approach to the thermodynamic structure of a generic null surface,
S. Dey and B. R. Majhi, “Covariant approach to the thermodynamic structure of a generic null surface,” Phys. Rev. D102, no.12, 124044 (2020) [arXiv:2009.08221 [gr-qc]]
-
[47]
Introduction to Modified Gravity and Gravitational Alternative for Dark Energy
S. Nojiri and S. D. Odintsov, “Introduction to modified gravity and gravitational alternative for dark energy,” eConfC0602061, 06 (2006) [arXiv:hep-th/0601213 [hep-th]]
work page internal anchor Pith review Pith/arXiv arXiv 2006
-
[48]
Einstein frame or Jordan frame ?
V. Faraoni and E. Gunzig, “Einstein frame or Jordan frame?,” Int. J. Theor. Phys.38, 217-225 (1999) [arXiv:astro-ph/9910176 [astro-ph]]
work page internal anchor Pith review Pith/arXiv arXiv 1999
-
[49]
Conformal transformations in classical gravitational theories and in cosmology
V. Faraoni, E. Gunzig and P. Nardone, “Conformal transformations in classical gravitational theories and in cosmology,” Fund. Cosmic Phys.20, 121 (1999) [arXiv:gr-qc/9811047 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1999
-
[50]
Black hole entropy in scalar-tensor and f(R) gravity: an overview
V. Faraoni, “Black hole entropy in scalar-tensor and f(R) gravity: An Overview,” Entropy12, 1246 (2010) [arXiv:1005.2327 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2010
-
[51]
A question mark on the equivalence of Einstein and Jordan frames
N. Banerjee and B. Majumder, “A question mark on the equivalence of Einstein and Jordan frames,” Phys. Lett. B754, 129-134 (2016) [arXiv:1601.06152 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2016
-
[52]
Equivalence of Jordan and Einstein frames at the quantum level
S. Pandey and N. Banerjee, “Equivalence of Jordan and Einstein frames at the quantum level,” Eur. Phys. J. Plus132, no.3, 107 (2017) [arXiv:1610.00584 [gr-qc]]. 22
work page internal anchor Pith review Pith/arXiv arXiv 2017
-
[53]
K. Bhattacharya and B. R. Majhi, “Fresh look at the scalar-tensor theory of gravity in Jordan and Ein- stein frames from undiscussed standpoints,” Phys. Rev. D95, no.6, 064026 (2017) [arXiv:1702.07166 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2017
-
[54]
K. Bhattacharya, A. Das and B. R. Majhi, “Noether and Abbott-Deser-Tekin conserved quantities in scalar-tensor theory of gravity both in Jordan and Einstein frames,” Phys. Rev. D97, no.12, 124013 (2018) [arXiv:1803.03771 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 2018
-
[55]
K. Bhattacharya, B. R. Majhi and D. Singleton, “Fluid-gravity correspondence in the scalar- tensor theory of gravity: (in)equivalence of Einstein and Jordan frames,” JHEP07, 018 (2020) [arXiv:2002.04743 [hep-th]]
-
[56]
Scalar–tensor gravity from thermodynamic and fluid-gravity perspective,
K. Bhattacharya and B. R. Majhi, “Scalar–tensor gravity from thermodynamic and fluid-gravity perspective,” Gen. Rel. Grav.54, no.9, 112 (2022) [arXiv:2209.07050 [gr-qc]]
-
[57]
Scalar-tensor theories of gravity from a thermodynamic view- point,
K. Bhattacharya and S. Chakraborty, “Scalar-tensor theories of gravity from a thermodynamic view- point,” JHEP01, 037 (2025) [arXiv:2409.04176 [gr-qc]]
-
[58]
Quasilocal Thermodynamics of Dilaton Gravity coupled to Gauge Fields
J. D. E. Creighton and R. B. Mann, “Quasilocal thermodynamics of dilaton gravity coupled to gauge fields,” Phys. Rev. D52, 4569-4587 (1995) [arXiv:gr-qc/9505007 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1995
-
[59]
Behavior of Quasilocal Mass Under Conformal Transformations
S. Bose and D. Lohiya, “Behavior of quasilocal mass under conformal transformations,” Phys. Rev. D59, 044019 (1999) [arXiv:gr-qc/9810033 [gr-qc]]
work page internal anchor Pith review Pith/arXiv arXiv 1999
-
[60]
Spacetime mappings of the Brown–York quasilocal energy,
J. Cˆ ot´ e, M. Lapierre-L´ eonard and V. Faraoni, “Spacetime mappings of the Brown–York quasilocal energy,” Eur. Phys. J. C79, no.8, 678 (2019) [arXiv:1908.02595 [gr-qc]]. 23
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