Further stable neutron star models from f (R) gravity AV Astashenok, S Capozziello, SD Odintsov Journal of Cosmology and Astroparticle Physics 2013 (12), 040, 2013 | 109 | 2013 |

Phantom cosmology without Big Rip singularity AV Astashenok, S Nojiri, SD Odintsov, AV Yurov Physics Letters B 709 (4-5), 396-403, 2012 | 93 | 2012 |

Maximal neutron star mass and the resolution of the hyperon puzzle in modified gravity AV Astashenok, S Capozziello, SD Odintsov Physical Review D 89 (10), 103509, 2014 | 82 | 2014 |

Extreme neutron stars from Extended Theories of Gravity AV Astashenok, S Capozziello, SD Odintsov Journal of Cosmology and Astroparticle Physics 2015 (01), 001, 2015 | 57 | 2015 |

Astronomical bounds on a future big freeze singularity AV Yurov, AV Astashenok, PF Gonzalez-Diaz Gravitation and Cosmology 14 (3), 205-212, 2008 | 52 | 2008 |

Scalar dark energy models mimicking ΛCDM with arbitrary future evolution AV Astashenok, S Nojiri, SD Odintsov, RJ Scherrer Physics Letters B 713 (3), 145-153, 2012 | 50 | 2012 |

Modified Gauss–Bonnet gravity with the Lagrange multiplier constraint as mimetic theory AV Astashenok, SD Odintsov, VK Oikonomou Classical and Quantum Gravity 32 (18), 185007, 2015 | 41 | 2015 |

Magnetic neutron stars in *f*(*R*) gravityAV Astashenok, S Capozziello, SD Odintsov Astrophysics and Space Science 355 (2), 333-341, 2015 | 33 | 2015 |

Nonperturbative models of quark stars in f (R) gravity AV Astashenok, S Capozziello, SD Odintsov Physics Letters B 742, 160-166, 2015 | 30 | 2015 |

Confronting dark energy models mimicking ΛCDM epoch with observational constraints: future cosmological perturbations decay or future Rip? AV Astashenok, SD Odintsov Physics Letters B 718 (4-5), 1194-1202, 2013 | 29 | 2013 |

The realistic models of relativistic stars in f (R)= R+ αR 2 gravity AV Astashenok, SD Odintsov, Á de la Cruz-Dombriz Classical and Quantum Gravity 34 (20), 205008, 2017 | 28 | 2017 |

AV Astashenok, S. Capozziello, and SD Odintsov, J. Cosmol. Astropart. Phys. 12 (2013) 040. AV Astashenok J. Cosmol. Astropart. Phys. 2013, 040, 0 | 28 | |

Cosmological measure with volume averaging and the vacuum energy problem AV Astashenok, A Del Popolo Classical and Quantum Gravity 29 (8), 085014, 2012 | 26 | 2012 |

Equation-of-state formalism for dark energy models on the brane and the future of brane universes AV Astashenok, E Elizalde, SD Odintsov, AV Yurov The European Physical Journal C 72 (12), 2260, 2012 | 24 | 2012 |

From neutron stars to quark stars in mimetic gravity AV Astashenok, SD Odintsov Physical Review D 94 (6), 063008, 2016 | 20 | 2016 |

Effective dark energy models and dark energy models with bounce in frames of *F*(*T*) gravityAV Astashenok Astrophysics and Space Science 351 (1), 377-383, 2014 | 12 | 2014 |

The dressing procedure for the cosmological equations and the indefinite future of the universe AV Yurov, AV Astashenok, VA Yurov Gravitation and Cosmology 14 (1), 8-16, 2008 | 12 | 2008 |

Brane cosmology from observational surveys and its comparison with standard FRW cosmology AV Astashenok, E Elizalde, J de Haro, SD Odintsov, AV Yurov Astrophysics and space science 347 (1), 1-13, 2013 | 5 | 2013 |

Modified Gauss–Bonnet gravity with Lagrange multiplier constraint as mimetic theory.(2015) AV Astashenok, SD Odintsov, VK Oikonomou arXiv preprint arXiv:1504.04861, 0 | 5 | |

New exact cosmologies on the brane AV Astashenok, AV Yurov, SV Chervon, EV Shabanov, M Sami Astrophysics and Space Science 353 (2), 319-328, 2014 | 4 | 2014 |