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Bayesian sensitivity of binary pulsars to ultra-light dark matter

The result's identifiers

  • Result code in IS VaVaI

    <a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F24%3A00605032" target="_blank" >RIV/68378271:_____/24:00605032 - isvavai.cz</a>

  • Alternative codes found

    RIV/00216208:11320/24:10495250

  • Result on the web

    <a href="https://hdl.handle.net/11104/0362595" target="_blank" >https://hdl.handle.net/11104/0362595</a>

  • DOI - Digital Object Identifier

    <a href="http://dx.doi.org/10.1051/0004-6361/202449953" target="_blank" >10.1051/0004-6361/202449953</a>

Alternative languages

  • Result language

    angličtina

  • Original language name

    Bayesian sensitivity of binary pulsars to ultra-light dark matter

  • Original language description

    Ultra-light dark matter perturbs the orbital motion of binary pulsars, in particular by causing peculiar time variations of a binary's orbital parameters, which then induce variations in the pulses' times of arrival. Binary pulsars have therefore been shown to be promising detectors of ultra-light dark matter. To date, the sensitivity of binary pulsars to ultra-light dark matter has only been studied for dark matter masses in a narrow resonance band around a multiple of the binary pulsar orbital frequency. In this study we devise a two-step, bayesian method that enables us to compute semi-analytically the sensitivity for all masses, also away from the resonance, and to combine several observed binaries into one global sensitivity curve. We then apply our method to the case of a universal, linearly-coupled, scalar ultra-light dark matter. We find that with next-generation radio observatories the sensitivity to the ultra-light dark matter coupling will surpass that of Solar-System constraints for a decade in mass around m similar to 10(-21) eV, even beyond resonance.

  • 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)<br>I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Others

  • Publication year

    2024

  • Confidentiality

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

Data specific for result type

  • Name of the periodical

    Astronomy & Astrophysics

  • ISSN

    0004-6361

  • e-ISSN

    1432-0746

  • Volume of the periodical

    690

  • Issue of the periodical within the volume

    Oct

  • Country of publishing house

    FR - FRANCE

  • Number of pages

    24

  • Pages from-to

    A51

  • UT code for WoS article

    001381135700011

  • EID of the result in the Scopus database

    2-s2.0-85206296652