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
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Czech description
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Classification
Type
J<sub>imp</sub> - Article in a specialist periodical, which is included in the Web of Science database
CEP classification
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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