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Nonlocal gravity cosmology: An overview

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F61989100%3A27120%2F22%3A10250360" target="_blank" >RIV/61989100:27120/22:10250360 - isvavai.cz</a>

  • Result on the web

    <a href="https://www.worldscientific.com/doi/10.1142/S0218271822300099" target="_blank" >https://www.worldscientific.com/doi/10.1142/S0218271822300099</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1142/S0218271822300099" target="_blank" >10.1142/S0218271822300099</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Nonlocal gravity cosmology: An overview

  • Original language description

    We discuss some main aspects of theories of gravity containing nonlocal terms in view of cosmological applications. In particular, we consider various extensions of general relativity based on geometrical invariants as f (R, square(-1) R), f (G, square(-1) G) and f (T, square(-1) T) gravity where R is the Ricci curvature scalar, G is the Gauss-Bonnet topological invariant, T the torsion scalar and the operator square(-1) gives rise to nonlocality. After selecting their functional form by using Noether symmetries, we find out exact solutions in a cosmological background. It is possible to reduce the dynamics of selected models and to find analytic solutions for the equations of motion. As a general feature of the approach, it is possible to address the accelerated expansion of the Hubble flow at various epochs, in particular the dark energy issues, by taking into account nonlocality corrections to the gravitational Lagrangian. On the other hand, it is possible to search for gravitational nonlocal effects also at astrophysical scales. In this perspective, we search for symmetries of f(R, square R-1) gravity also in a spherically symmetric background and constrain the free parameters, Specifically, by taking into account the S2 star orbiting around the Galactic Center SgrA*, it is possible to study how nonlocality affects stellar orbits around such a massive self-gravitating object.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database

  • CEP classification

  • OECD FORD branch

    10300 - Physical sciences

Result continuities

  • Project

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2022

  • Confidentiality

    S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Data specific for result type

  • Name of the periodical

    International Journal of Modern Physics D

  • ISSN

    0218-2718

  • e-ISSN

    1793-6594

  • Volume of the periodical

    31

  • Issue of the periodical within the volume

    06

  • Country of publishing house

    SG - SINGAPORE

  • Number of pages

    42

  • Pages from-to

    "nestrankovano"

  • UT code for WoS article

    000797247400001

  • EID of the result in the Scopus database

    2-s2.0-85121581471