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Spinning particles in general relativity: Momentum-velocity relation for the Mathisson-Pirani spin condition

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F18%3A00497137" target="_blank" >RIV/67985815:_____/18:00497137 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/18:10388227

  • Result on the web

    <a href="http://dx.doi.org/10.1103/PhysRevD.97.084023" target="_blank" >http://dx.doi.org/10.1103/PhysRevD.97.084023</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/PhysRevD.97.084023" target="_blank" >10.1103/PhysRevD.97.084023</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Spinning particles in general relativity: Momentum-velocity relation for the Mathisson-Pirani spin condition

  • Original language description

    The Mathisson-Papapetrou-Dixon (MPD) equations, providing the pole-dipole description of spinning test particles in general relativity, have to be supplemented by a condition specifying the worldline that will represent the history of the studied body. It has long been thought that the Mathisson-Pirani (MP) spin condition-unlike other major choices made in the literature-does not yield an explicit momentum-velocity relation. We derive here the desired (and very simple) relation and show that it is in fact equivalent to the MP condition. We clarify the apparent paradox between the existence of such a definite relation and the known fact that the MP condition is degenerate (does not specify a unique worldline), thus shedding light on some conflicting statements made in the literature. We then show how, for a given body, this spin condition yields infinitely many possible representative worldlines, and derive a detailed method how to switch between them in a curved spacetime. The MP condition is a convenient choice in situations when it is easy to recognize its “nonhelical” solution, as exemplified here by bodies in circular orbits and in radial fall in the Schwarzschild spacetime.

  • 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

    10308 - Astronomy (including astrophysics,space science)

Result continuities

  • Project

    Result was created during the realization of more than one project. More information in the Projects tab.

  • Continuities

    P - Projekt vyzkumu a vyvoje financovany z verejnych zdroju (s odkazem do CEP)

Others

  • Publication year

    2018

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Physical Review D

  • ISSN

    2470-0010

  • e-ISSN

  • Volume of the periodical

    97

  • Issue of the periodical within the volume

    8

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    18

  • Pages from-to

  • UT code for WoS article

    000430061300011

  • EID of the result in the Scopus database

    2-s2.0-85046530583