Matches in SemOpenAlex for { <https://semopenalex.org/work/W3199474384> ?p ?o ?g. }
- W3199474384 endingPage "262" @default.
- W3199474384 startingPage "262" @default.
- W3199474384 abstract "A possible detection of sub-solar mass ultra-compact objects would lead to new perspectives on the existence of black holes that are not of astrophysical origin and/or pertain to formation scenarios of exotic ultra-compact objects. Both possibilities open new perspectives for better understanding of our universe. In this work, we investigate the significance of detection of sub-solar mass binaries with components mass in the range: 10-2M⊙ up to 1M⊙, within the expected sensitivity of the ground-based gravitational waves detectors of third generation, viz., the Einstein Telescope (ET) and the Cosmic Explorer (CE). Assuming a minimum of amplitude signal-to-noise ratio for detection, viz., ρ=8, we find that the maximum horizon distances for an ultra-compact binary system with components mass 10-2M⊙ and 1M⊙ are 40 Mpc and 1.89 Gpc, respectively, for ET, and 125 Mpc and 5.8 Gpc, respectively, for CE. Other cases are also presented in the text. We derive the merger rate and discuss consequences on the abundances of primordial black hole (PBH), fPBH. Considering the entire mass range [10-2-1]M⊙, we find fPBH<0.70 (<0.06) for ET (CE), respectively." @default.
- W3199474384 created "2021-09-27" @default.
- W3199474384 creator A5086929880 @default.
- W3199474384 date "2022-02-11" @default.
- W3199474384 modified "2023-09-30" @default.
- W3199474384 title "Search for Sub-Solar Mass Binaries with Einstein Telescope and Cosmic Explorer" @default.
- W3199474384 cites W1509168094 @default.
- W3199474384 cites W1969823825 @default.
- W3199474384 cites W1978916504 @default.
- W3199474384 cites W1983380408 @default.
- W3199474384 cites W1998388948 @default.
- W3199474384 cites W2046680903 @default.
- W3199474384 cites W2065913386 @default.
- W3199474384 cites W2067683407 @default.
- W3199474384 cites W2077768234 @default.
- W3199474384 cites W2081835848 @default.
- W3199474384 cites W2103857591 @default.
- W3199474384 cites W2106723786 @default.
- W3199474384 cites W2289010674 @default.
- W3199474384 cites W2506531441 @default.
- W3199474384 cites W2510539355 @default.
- W3199474384 cites W2607779736 @default.
- W3199474384 cites W2757338357 @default.
- W3199474384 cites W2796755404 @default.
- W3199474384 cites W2801940103 @default.
- W3199474384 cites W2885150380 @default.
- W3199474384 cites W2885848671 @default.
- W3199474384 cites W2888075871 @default.
- W3199474384 cites W2898313720 @default.
- W3199474384 cites W2898584704 @default.
- W3199474384 cites W2903375752 @default.
- W3199474384 cites W2920511893 @default.
- W3199474384 cites W2933980750 @default.
- W3199474384 cites W2951990651 @default.
- W3199474384 cites W2956256443 @default.
- W3199474384 cites W2962876006 @default.
- W3199474384 cites W2978017091 @default.
- W3199474384 cites W3039738912 @default.
- W3199474384 cites W3041081567 @default.
- W3199474384 cites W3081562793 @default.
- W3199474384 cites W3081838188 @default.
- W3199474384 cites W3084422685 @default.
- W3199474384 cites W3088952054 @default.
- W3199474384 cites W3095088070 @default.
- W3199474384 cites W3097427857 @default.
- W3199474384 cites W3097998806 @default.
- W3199474384 cites W3098069234 @default.
- W3199474384 cites W3098245943 @default.
- W3199474384 cites W3099011942 @default.
- W3199474384 cites W3099071754 @default.
- W3199474384 cites W3099138539 @default.
- W3199474384 cites W3099485846 @default.
- W3199474384 cites W3099955570 @default.
- W3199474384 cites W3100187076 @default.
- W3199474384 cites W3101478357 @default.
- W3199474384 cites W3102014803 @default.
- W3199474384 cites W3104489202 @default.
- W3199474384 cites W3106254327 @default.
- W3199474384 cites W3106308919 @default.
- W3199474384 cites W3120709288 @default.
- W3199474384 cites W3128133039 @default.
- W3199474384 cites W3158601608 @default.
- W3199474384 cites W3165680606 @default.
- W3199474384 cites W3167053542 @default.
- W3199474384 cites W3169101650 @default.
- W3199474384 cites W3171870391 @default.
- W3199474384 cites W3179775611 @default.
- W3199474384 cites W3184240428 @default.
- W3199474384 cites W4206714946 @default.
- W3199474384 doi "https://doi.org/10.3390/e24020262" @default.
- W3199474384 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/35205556" @default.
- W3199474384 hasPublicationYear "2022" @default.
- W3199474384 type Work @default.
- W3199474384 sameAs 3199474384 @default.
- W3199474384 citedByCount "3" @default.
- W3199474384 countsByYear W31994743842022 @default.
- W3199474384 countsByYear W31994743842023 @default.
- W3199474384 crossrefType "journal-article" @default.
- W3199474384 hasAuthorship W3199474384A5086929880 @default.
- W3199474384 hasBestOaLocation W31994743841 @default.
- W3199474384 hasConcept C121332964 @default.
- W3199474384 hasConcept C1276947 @default.
- W3199474384 hasConcept C150846664 @default.
- W3199474384 hasConcept C165129702 @default.
- W3199474384 hasConcept C188232333 @default.
- W3199474384 hasConcept C190330329 @default.
- W3199474384 hasConcept C2780490093 @default.
- W3199474384 hasConcept C2780848835 @default.
- W3199474384 hasConcept C33923547 @default.
- W3199474384 hasConcept C44870925 @default.
- W3199474384 hasConcept C48372109 @default.
- W3199474384 hasConcept C539450922 @default.
- W3199474384 hasConcept C59375849 @default.
- W3199474384 hasConcept C84999194 @default.
- W3199474384 hasConcept C8673692 @default.
- W3199474384 hasConcept C94375191 @default.
- W3199474384 hasConceptScore W3199474384C121332964 @default.
- W3199474384 hasConceptScore W3199474384C1276947 @default.