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Trapping of null geodesics in slowly rotating spacetimes

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F47813059%3A19630%2F20%3AA0000058" target="_blank" >RIV/47813059:19630/20:A0000058 - isvavai.cz</a>

  • Result on the web

    <a href="https://link.springer.com/article/10.1140/epjc/s10052-020-08642-z" target="_blank" >https://link.springer.com/article/10.1140/epjc/s10052-020-08642-z</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1140/epjc/s10052-020-08642-z" target="_blank" >10.1140/epjc/s10052-020-08642-z</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Trapping of null geodesics in slowly rotating spacetimes

  • Original language description

    Extremely compact objects containing a region of trapped null geodesics could be of astrophysical relevance due to trapping of neutrinos with consequent impact on cooling processes or trapping of gravitational waves. These objects have previously been studied under the assumption of spherical symmetry. In the present paper, we consider a simple generalization by studying trapping of null geodesics in the framework of the Hartle-Thorne slow-rotation approximation taken to first order in the angular velocity, and considering a uniform-density object with uniform emissivity for the null geodesics. We calculate effective potentials and escape cones for the null geodesics and how they depend on the parameters of the spacetimes, and also calculate the "local" and "global" coefficients of efficiency for the trapping. We demonstrate that due to the rotation the trapping efficiency is different for co-rotating and retrograde null geodesics, and that trapping can occur even for R&gt;3GM/c2, contrary to what happens in the absence of rotation.

  • 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

    10303 - Particles and field physics

Result continuities

  • Project

    <a href="/en/project/LTC18058" target="_blank" >LTC18058: Neutron stars and pulsars</a><br>

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2020

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    European Physical Journal C

  • ISSN

    1434-6044

  • e-ISSN

    1434-6052

  • Volume of the periodical

    80

  • Issue of the periodical within the volume

    11

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    20

  • Pages from-to

    „1065-1“-„1065-20“

  • UT code for WoS article

    000595358600007

  • EID of the result in the Scopus database

    2-s2.0-85096210789