Why scalar–tensor equivalent theories are not physically equivalent? (English)
- New search for: Sk, Nayem
- New search for: Sk, Nayem
- New search for: Sanyal, Abhik Kumar
In:
International journal of modern physics / D
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26
, 14
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2017
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ISSN:
- Article (Journal) / Print
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Title:Why scalar–tensor equivalent theories are not physically equivalent?
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Contributors:Sk, Nayem ( author ) / Sanyal, Abhik Kumar
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Published in:
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Publisher:
- New search for: World Scientific Publ.
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Place of publication:Singapore [u.a.]
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Publication date:2017
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ISSN:
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ZDBID:
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DOI:
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Type of media:Article (Journal)
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Type of material:Print
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Language:English
- New search for: 33.00
- Further information on Basic classification
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Keywords:
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Classification:
BKL: 33.00 -
Source:
Table of contents – Volume 26, Issue 14
The tables of contents are generated automatically and are based on the data records of the individual contributions available in the index of the TIB portal. The display of the Tables of Contents may therefore be incomplete.
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Viscous cosmology for early- and late-time universeBrevik, Iver et al. | 2017
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The effective Tolman temperature in curved spacetimesKim, Wontae et al. | 2017
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Lorenz gauge fixing of f(T) teleparallel cosmologyEl Hanafy, W et al. | 2017
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Role of structure scalars on viscous and heat conducting spherical systems in f(R,T) gravityHussain, T et al. | 2017
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Observing the shadow of modified gravity black holeAlhamzawi, Ahmed et al. | 2017
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Dispersion relations for gravitational waves in different models of dark energyDzhunushaliev, Vladimir et al. | 2017
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Stability of spherically symmetric timelike thin-shells in general relativity with a variable equation-of-stateMazharimousavi, S. Habib et al. | 2017
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Implications of a frame dependent gravitational effective action for perturbations on the Robertson–Walker metricAdler, Stephen L et al. | 2017
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Quasinormal modes of scalar and Dirac perturbations of Bardeen de Sitter black holesWahlang, Wadbor et al. | 2017
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Estimation of mass composition of high energy cosmic rays via modeling a relation between lateral distribution parameters and shower ageDoostmohammadi, Saeed et al. | 2017
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Why scalar–tensor equivalent theories are not physically equivalent?Sk, Nayem et al. | 2017
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Covariant response theory and the boost transform of the dielectric tensorStarke, R et al. | 2017
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Dynamics of two-scalar-field cosmological models beyond the exponential potentialLi, Yu et al. | 2017
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Test of indestructibility of a nonsingular black holePaik, Biplab et al. | 2017
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Minimal-supersymmetric extended inflation field in Horava–Lifshitz gravityTawfik, Abdel Nasser et al. | 2017
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Cartesian Kerr–Schild variation on the Newman–Janis trickRajan, Del et al. | 2017
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A possible new cosmological redshift effect due to Λ on traveling gravitational waves in Friedmann universesViaggiu, Stefano et al. | 2017
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The geodesics structure of Schwarzschild black hole immersed in an electromagnetic universeAl-Badawi, A et al. | 2017