| 1. Identity statement | ||||
| Reference Type | Journal Article | |||
| Site | mtc-m21d.sid.inpe.br | |||
| Holder Code | isadg {BR SPINPE} ibi 8JMKD3MGPCW/3DT298S | |||
| Identifier | 8JMKD3MGP3W34T/46HABF5 | |||
| Repository | sid.inpe.br/mtc-m21d/2022/03.18.12.50 | |||
| Last Update | 2022:03.18.12.50.33 (UTC) simone | |||
| Metadata Repository | sid.inpe.br/mtc-m21d/2022/03.18.12.50.33 | |||
| Metadata Last Update | 2023:01.03.16.46.02 (UTC) administrator | |||
| DOI | 10.1093/mnras/stab3748 | |||
| ISSN | 0035-8711 1365-2966 | |||
| Citation Key | KamlahLSAABBGHBKW:2022:EvSiBi | |||
| Title | Preparing the next gravitational million-body simulations: evolution of single and binary stars in nbody6++gpu, mocca, and mcluster  | |||
| Year | 2022 | |||
| Month | Feb. | |||
| Access Date | 2024, May 14 | |||
| Type of Work | journal article | |||
| Secondary Type | PRE PI | |||
| Number of Files | 1 | |||
| Size | 3960 KiB | |||
| 2. Context | ||||
| Author | 1 Kamlah, A. W. H. 2 Leveque, A. 3 Spurzem, R. 4 Arca Sedda, M. 5 Askar, A. 6 Banerjee, S. 7 Berczik, P. 8 Giersz, M. 9 Hurley, J. 10 Belloni, Diogo Teixeira 11 Kühmichel, L. 12 Wang, L. | |||
| ORCID | 1 0000-0001-8768-4510 2 0000-0002-3111-863X 3 0000-0003-2264-7203 4 0000-0002-3987-0519 5 0000-0001-9688-3458 6 0000-0002-1254-2603 7 0000-0003-4176-152X 8 0000-0002-5987-5077 9 0000-0003-2694-0415 10 0000-0003-1535-0866 11 12 0000-0001-8713-0366 | |||
| Group | 1 2 3 4 5 6 7 8 9 10 DIAST-CGCE-INPE-MCTI-GOV-BR | |||
| Affiliation | 1 Max-Planck-Institut für Astronomie 2 Peking University 3 University of Heidelberg 4 University of Heidelberg 5 Chinese Academy of Sciences 6 Polish Academy of Sciences 7 National Academy of Sciences of Ukraine 8 Peking University 9 Swinburne University of Technology 10 Instituto Nacional de Pesquisas Espaciais (INPE) 11 University of Heidelberg 12 The University of Tokyo | |||
| Author e-Mail Address | 1 albrechtk@hotmail.de 2 3 4 5 6 7 8 9 10 diogobellonizorzi@gmail.com | |||
| Journal | Monthly Notices of the Royal Astronomical Society | |||
| Volume | 511 | |||
| Number | 3 | |||
| Pages | 4060-4089 | |||
| Secondary Mark | A1_QUÍMICA A1_INTERDISCIPLINAR A1_GEOCIÊNCIAS A1_ENGENHARIAS_III A2_MATEMÁTICA_/_PROBABILIDADE_E_ESTATÍSTICA A2_ASTRONOMIA_/_FÍSICA B2_ENSINO B5_ENGENHARIAS_IV | |||
| History (UTC) | 2022-03-18 12:50:33 :: simone -> administrator :: 2022-03-18 12:50:34 :: administrator -> simone :: 2022 2022-03-18 12:53:49 :: simone -> administrator :: 2022 2023-01-03 16:46:02 :: 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 | methods: numerical software: development software: documentation binaries: general stars: general globular clusters: general | |||
| Abstract | We present the implementation of updated stellar evolution recipes in the codes nbody6++gpu, mocca, and mcluster. We test them through numerical simulations of star clusters containing 1.1 x 10(5) stars (with 2.0 x 10(4) in primordial hard binaries) performing high-resolution direct N-body (nbody6++gpu) and Monte Carlo (mocca) simulations to an age of 10 Gyr. We compare models implementing either delayed or core-collapse supernovae mechanisms, a different mass ratio distribution for binaries, and white dwarf (WD) natal kicks enabled/disabled. Compared to nbody6++gpu, the mocca models appear to be denser, with a larger scatter in the remnant masses, and a lower binary fraction on average. The mocca models produce more black holes (BHs) and helium WDs, while nbody6++gpu models are characterized by a much larger amount of WD-WD binaries. The remnant kick velocity and escape speed distributions are similar for the BHs and neutron stars (NSs), and some NSs formed via electron-capture supernovae, accretion-induced collapse, or merger-induced collapse escape the cluster in all simulations. The escape speed distributions for the WDs, on the other hand, are very dissimilar. We categorize the stellar evolution recipes available in nbody6++gpu into four levels: the one implemented in previous nbody6++gpu and mocca versions (level A), state-of-the-art prescriptions (level B), some in a testing phase (level C), and those that will be added in future versions of our codes. | |||
| Area | CEA | |||
| Arrangement | urlib.net > BDMCI > Fonds > Produção a partir de 2021 > CGCE > Preparing the next... | |||
| doc Directory Content | access | |||
| source Directory Content | there are no files | |||
| agreement Directory Content |
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| 4. Conditions of access and use | ||||
| data URL | http://mtc-m21d.sid.inpe.br/ibi/8JMKD3MGP3W34T/46HABF5 | |||
| zipped data URL | http://mtc-m21d.sid.inpe.br/zip/8JMKD3MGP3W34T/46HABF5 | |||
| Language | en | |||
| Target File | khamla_2022_preparing.pdf | |||
| User Group | simone | |||
| Reader Group | administrator simone | |||
| Visibility | shown | |||
| Archiving Policy | allowpublisher allowfinaldraft | |||
| 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; PORTALCAPES; MGA; COMPENDEX. | |||
| Host Collection | urlib.net/www/2021/06.04.03.40 | |||
| 6. Notes | ||||
| Empty Fields | alternatejournal archivist callnumber copyholder copyright creatorhistory descriptionlevel e-mailaddress format isbn label lineage mark mirrorrepository nextedition notes parameterlist parentrepositories previousedition previouslowerunit progress project readpermission resumeid rightsholder schedulinginformation secondarydate secondarykey session shorttitle sponsor subject tertiarymark tertiarytype url | |||
| 7. Description control | ||||
| e-Mail (login) | simone | |||
| update | ||||