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1. Identity statement Reference Type Journal Article Site mtc-m21d.sid.inpe.br Holder Code isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S Identifier 8JMKD3MGP3W34T/46DTC9B Repository sid.inpe.br/mtc-m21d/2022/02.25.19.27   (restricted access) Last Update 2022:02.25.19.27.27 (UTC) simone Metadata Repository sid.inpe.br/mtc-m21d/2022/02.25.19.27.27 Metadata Last Update 2023:01.03.16.46.01 (UTC) administrator DOI 10.3390/e24020262 ISSN 1099-4300 Citation Key Nunes:2022:SeSuMa Title Search for Sub-Solar Mass Binaries with Einstein Telescope and Cosmic Explorer Year 2022 Month Feb. Access Date 2024, May 13 Type of Work journal article Secondary Type PRE PI Number of Files 1 Size 553 KiB 2. Context Author Nunes, Rafael da Costa ORCID 0000-0002-8432-5616 Group DIAST-CGCE-INPE-MCTI-GOV-BR Affiliation Instituto Nacional de Pesquisas Espaciais (INPE) Author e-Mail Address rafadcnunes@gmail.com Journal Entropy Volume 24 Number 2 Pages e262 Secondary Mark B1_GEOCIÊNCIAS B1_ENGENHARIAS_IV B1_CIÊNCIA_DA_COMPUTAÇÃO B2_INTERDISCIPLINAR B3_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA B3_ASTRONOMIA_/_FÍSICA History (UTC) 2022-02-25 19:27:38 :: simone -> administrator :: 2022 2023-01-03 16:46:01 :: administrator -> simone :: 2022 3. Content and structure Is the master or a copy? is the master Content Stage completed Transferable 1 Content Type External Contribution Version Type publisher Keywords Gravitational wave astronomy Ground-based detectors Primordial black hole 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: 10−2 M⊙ 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 10−2 M⊙ 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. Area CEA Arrangement urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Search for Sub-Solar... doc Directory Content access source Directory Content there are no files agreement Directory Content agreement.html 25/02/2022 16:27 1.0 KiB  4. Conditions of access and use Language en Target File Nunes_2022_search.pdf User Group simone Reader Group administrator simone Visibility shown Read Permission deny from all and allow from 150.163 Update Permission not transferred 5. Allied materials Next Higher Units 8JMKD3MGPCW/46KTFK8 Citing Item List sid.inpe.br/bibdigital/2022/04.03.17.52 1 Dissemination WEBSCI; SCOPUS. Host Collection urlib.net/www/2021/06.04.03.40 6. Notes Empty Fields alternatejournal archivingpolicy archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url 7. Description control e-Mail (login) simone update

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