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Coupled scalar-Proca soliton stars

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F23%3A00579755" target="_blank" >RIV/68378271:_____/23:00579755 - isvavai.cz</a>

  • Result on the web

    <a href="https://doi.org/10.1103/PhysRevD.108.044044" target="_blank" >https://doi.org/10.1103/PhysRevD.108.044044</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1103/PhysRevD.108.044044" target="_blank" >10.1103/PhysRevD.108.044044</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Coupled scalar-Proca soliton stars

  • Original language description

    We construct and explore the physical properties of textit{scalaroca stars}: spherically symmetric solitonic solutions made of a complex scalar field and a complex Proca field . We restrict our attention to configurations in which both fields are in the fundamental state and possess an equal mass, focusing on the cases when () the scalar and Proca fields are (non--linearly) super--imposed and do not interact with each other, and () the scalar and Proca fields interact through the term . The solutions are found numerically for the non--interacting case () as well as for both signs of the interaction coupling constant . While pure ( single--field) Proca/scalar boson stars are the most/least massive for weakly--interacting fields, one can obtain more massive solutions for a sufficiently strong interaction. Besides, in the latter case, solutions can be either in a synchronized state -- in which both fields have the same frequency -- or in a non--synchronized state. In addition, we observe that the coupling between the two fields allows solitonic solutions with a real scalar field. We further comment on the possibility of spontaneous scalarization and vectorization of the interacting solitonic solution.

  • Czech name

  • Czech description

Classification

  • Type

    J<sub>SC</sub> - Article in a specialist periodical, which is included in the SCOPUS database

  • CEP classification

  • OECD FORD branch

    10303 - Particles and field physics

Result continuities

  • Project

    <a href="/en/project/GM21-16583M" target="_blank" >GM21-16583M: New avenues in the hunt for dark energy</a><br>

  • Continuities

    I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2023

  • 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

    2470-0029

  • Volume of the periodical

    108

  • Issue of the periodical within the volume

    4

  • Country of publishing house

    US - UNITED STATES

  • Number of pages

    14

  • Pages from-to

    044044

  • UT code for WoS article

  • EID of the result in the Scopus database

    2-s2.0-85172777891