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- S. Odintsov3 profiles252 · h 104
- I. Buchbinder159 · h 47
- S. Nojiri2 profiles106 · h 90
- P. Lavrov2 profiles85 · h 14
- V. Oikonomou2 profiles76 · h 53
- S. Capozziello63 · h 89
- I. Shapiro55 · h 42
- V. K. Oikonomou4 profiles47 · h 35
- A. Timoshkin46 · h 18
- I. Brevik2 profiles40 · h 39
- E. Elizalde2 profiles30 · h 47
- A. Reshetnyak26 · h 16
- National Research Tomsk State UniversityRU267 papers
- Tomsk State University of Control Systems and Radio-ElectronicsRU197 papers
- Institute of Space SciencesES153 papers
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- Consejo Superior de Investigaciones CientíficasES72 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT72 papers
- Universidade Federal de Juiz de ForaBR69 papers
- Tomsk Polytechnic UniversityRU68 papers
- Aristotle University of ThessalonikiGR66 papers
- Joint Institute for Nuclear ResearchRU58 papers
- National Defense Academy of JapanJP58 papers
- Nagoya UniversityJP54 papers
841 papers
Singularity softening and avoidance by the action of thermal radiation in a generalized entropic cosmology
E. Elizalde, A. V. Yurov, A. V. Timoshkin
Some relevant aspects of a new form of generalized entropic cosmology, recently introduced by Nojiri, Odintsov and Faraoni, are considered. The setup is a logarithmic equation of s…
Secondary gravitational waves against a strong gravitational wave in the Bianchi VI universe
Konstantin E. Osetrin
A proper-time method for constructing models of dynamic gravitational-wave fields is presented. Using the proper-time method, analytical (not numerical) models of secondary gravita…
Linear perturbations of an exact gravitational wave in the Bianchi IV universe
Konstantin Osetrin
The proper-time method for constructing perturbative dynamical gravitational fields is presented. Using the proper-time method, a perturbative analytical model of gravitational wav…
Towards Lagrangian dynamics for constrained mixed-symmetric interacting higher-spin fields
A. Reshetnyak
The necessary and sufficient conditions to construct consistent Lagrangian formulation for irreducible interacting massless higher-spin (HS) fields on -dimensional Minkowski spa…
Holographic bounce cosmological models induced by viscous dark fluid from a generalized non-singular entropy function
E. Elizalde, A. V. Yurov, A. V. Timoshkin
Bounce cosmological models containing a dark viscous fluid in a spatially flat Friedmann-Robertson-Walker (FRW) universe are considered. The universe evolution is described in term…
Rips and regular future scenario with Holographic Dark Energy: A comprehensive look
I. Brevik, Maxim Khlopov, S. D. Odintsov +2
Interest on the possible future scenarios the universe could have has grew substantially with breakthroughs on late-time acceleration. Holographic dark energy (HDE) presents a very…