Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass
We test the possibility that the black holes (BHs) detected by LIGO-Virgo-KAGRA (LVK) may be cosmologically coupled and grow in mass proportionally to the cosmological scale factor to some power k, which may also act as the dark energy source if k ≈ 3. This approach was proposed as an extension of K...
Saved in:
| Main Authors: | , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
February 2024
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 2024, Volume: 528, Issue: 2, Pages: 2377-2390 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/stae143 |
| Online Access: | Resolving-System, kostenfrei, Volltext: https://doi.org/10.1093/mnras/stae143 Verlag, kostenfrei, Volltext: https://academic.oup.com/mnras/article/528/2/2377/7529208 
|
| Author Notes: | Luca Amendola, Davi C Rodrigues, Sumit Kumar and Miguel Quartin |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1897048645 | ||
| 003 | DE-627 | ||
| 005 | 20241205155408.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 240730s2024 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1093/mnras/stae143 |2 doi | |
| 035 | |a (DE-627)1897048645 | ||
| 035 | |a (DE-599)KXP1897048645 | ||
| 035 | |a (OCoLC)1475305194 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Amendola, Luca |d 1963- |e VerfasserIn |0 (DE-588)1029171270 |0 (DE-627)732547482 |0 (DE-576)377045128 |4 aut | |
| 245 | 1 | 0 | |a Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass |c Luca Amendola, Davi C Rodrigues, Sumit Kumar and Miguel Quartin |
| 264 | 1 | |c February 2024 | |
| 300 | |b Illustrationen | ||
| 300 | |a 14 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 30.07.2024 | ||
| 520 | |a We test the possibility that the black holes (BHs) detected by LIGO-Virgo-KAGRA (LVK) may be cosmologically coupled and grow in mass proportionally to the cosmological scale factor to some power k, which may also act as the dark energy source if k ≈ 3. This approach was proposed as an extension of Kerr BHs embedded in cosmological backgrounds and possibly without singularities or horizons. In our analysis, we develop and apply two methods to test these cosmologically coupled BHs (CCBHs) either with or without connection to dark energy. We consider different scenarios for the time between the binary BH formation and its merger, and we find that the standard log-uniform distribution yields weaker constraints than the CCBH-corrected case. Assuming that the minimum mass of a BH with stellar progenitor is 2 M⊙, we estimate the probability that at least one BH among the observed ones had an initial mass below this threshold. We obtain these probabilities either directly from the observed data or by assuming the LVK power-law-plus-peak mass distribution. In the latter case, we find at 2σ level, that k < 2.1 for the standard log-uniform distribution, or k < 1.1 for the CCBH-corrected distribution. Slightly weaker bounds are obtained in the direct method. Considering the uncertainties on the nature of CCBHs, we also find that the required minimum CCBH mass value to eliminate the tensions for k = 3 should be lower than 0.5 M⊙ (again at 2σ). Finally, we show that future observations have the potential to decisively confirm these bounds. | ||
| 700 | 1 | |a Rodrigues, Davi C. |e VerfasserIn |0 (DE-588)1307734332 |0 (DE-627)1868667677 |4 aut | |
| 700 | 1 | |a Kumar, Sumit |e VerfasserIn |4 aut | |
| 700 | 1 | |a Quartin, Miguel |e VerfasserIn |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |a Royal Astronomical Society |t Monthly notices of the Royal Astronomical Society |d Oxford : Oxford Univ. Press, 1827 |g 528(2024), 2 vom: Feb., Seite 2377-2390 |h Online-Ressource |w (DE-627)314059164 |w (DE-600)2016084-7 |w (DE-576)090955420 |x 1365-2966 |7 nnas |
| 773 | 1 | 8 | |g volume:528 |g year:2024 |g number:2 |g month:02 |g pages:2377-2390 |g extent:14 |a Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass |
| 856 | 4 | 0 | |u https://doi.org/10.1093/mnras/stae143 |x Resolving-System |x Verlag |z kostenfrei |3 Volltext |
| 856 | 4 | 0 | |u https://academic.oup.com/mnras/article/528/2/2377/7529208 |x Verlag |z kostenfrei |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20240730 | ||
| 993 | |a Article | ||
| 994 | |a 2024 | ||
| 998 | |g 1307734332 |a Rodrigues, Davi C. |m 1307734332:Rodrigues, Davi C. |p 2 | ||
| 998 | |g 1029171270 |a Amendola, Luca |m 1029171270:Amendola, Luca |d 130000 |d 130300 |e 130000PA1029171270 |e 130300PA1029171270 |k 0/130000/ |k 1/130000/130300/ |p 1 |x j | ||
| 999 | |a KXP-PPN1897048645 |e 4560530971 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"note":["Gesehen am 30.07.2024"],"name":{"displayForm":["Luca Amendola, Davi C Rodrigues, Sumit Kumar and Miguel Quartin"]},"recId":"1897048645","origin":[{"dateIssuedDisp":"February 2024","dateIssuedKey":"2024"}],"language":["eng"],"person":[{"display":"Amendola, Luca","role":"aut","family":"Amendola","given":"Luca"},{"display":"Rodrigues, Davi C.","role":"aut","family":"Rodrigues","given":"Davi C."},{"given":"Sumit","family":"Kumar","role":"aut","display":"Kumar, Sumit"},{"given":"Miguel","family":"Quartin","role":"aut","display":"Quartin, Miguel"}],"title":[{"title_sort":"Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass","title":"Constraints on cosmologically coupled black holes from gravitational wave observations and minimal formation mass"}],"relHost":[{"recId":"314059164","origin":[{"publisherPlace":"Oxford ; Oxford [u.a.] ; Oxford [u.a.]","dateIssuedKey":"1827","dateIssuedDisp":"1827-","publisher":"Oxford Univ. Press ; Blackwell ; Wiley-Blackwell"}],"pubHistory":["1.1827 -"],"part":{"text":"528(2024), 2 vom: Feb., Seite 2377-2390","issue":"2","pages":"2377-2390","extent":"14","year":"2024","volume":"528"},"type":{"media":"Online-Ressource","bibl":"periodical"},"id":{"eki":["314059164"],"doi":["10.1111/(ISSN)1365-2966"],"issn":["1365-2966"],"zdb":["2016084-7"]},"disp":"Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society","note":["Gesehen am 15.01.2018"],"corporate":[{"role":"aut","display":"Royal Astronomical Society"}],"language":["eng"],"title":[{"title":"Monthly notices of the Royal Astronomical Society","title_sort":"Monthly notices of the Royal Astronomical Society"}],"physDesc":[{"extent":"Online-Ressource"}]}],"physDesc":[{"noteIll":"Illustrationen","extent":"14 S."}],"id":{"doi":["10.1093/mnras/stae143"],"eki":["1897048645"]},"type":{"bibl":"article-journal","media":"Online-Ressource"}} | ||
| SRT | |a AMENDOLALUCONSTRAINT2024 | ||