Universe@Home
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| Developer(s) | University of Warsaw |
|---|---|
| Operating system | cross-platform |
| Platform | BOINC |
| Average performance | 538,537.00 GigaFLOPS |
| Active users | 51,166 |
| Website | universeathome |
Universe@Home is a volunteer computing project that performs astrophysical research and is sponsored by the University of Warsaw.[1] The Universe@Home application runs on Windows, Linux, Android and Raspbian operating systems by using the Berkeley Open Infrastructure for Network Computing (BOINC) platform to distribute work to volunteers. Universe@Home is officially listed on the BOINC website[2] and approved by Science United.[3]
Objectives[edit]
This project simulates the evolution of star clusters, estimates observations of gravitational waves, and tests models of supernovae explosions.[4] Universe@Home calculates the physical properties of individual stars, tracks their evolution over time, and observe how they interact with one another as they age using a cutting-edge collection of computational tools. The project aims to create the first database of the simulated stellar content of the Universe. Astronomers will have access to this extensive stellar library, which will also serve as an educational asset for the general public.[5]
The research has resulted in a deeper understanding of Black holes; the project website maintains a publicly-accessible database of known Black holes[6] (among other discoveries from their research) which has led to several scientific publications and citations.
Scientific publications[edit]
- Nature of the Extreme Ultraluminous X-Ray Sources[7]
- The first gravitational-wave source from the isolated evolution of two 40–100 M⊙ stars[8]
- The Origin of the Ultraluminous X-Ray Sources[9]
- Dynamical formation of black hole low-mass X-ray binaries in the field: an alternative to the common envelope[10]
- Strange Quark Stars in Binaries: Formation Rates, Mergers, and Explosive Phenomena[11]
- The origin of the first neutron star – neutron star merger[12]
- Binary neutron star formation and the origin of GW170817[13]
- Merger of Compact Stars in the Two-families Scenario[14]
- The Observed versus Total Population of ULXs[15]
- Populations of Stellar-mass Black Holes from Binary Systems[16]
- Noninteracting Black Hole Binaries with Gaia and LAMOST[17]
- Wind-powered Ultraluminous X-ray Sources[18]
- Predicting the self-lensing population in optical surveys[19]
References[edit]
- ↑ "Universe@Home/en – Rechenkraft". www.rechenkraft.net. Archived from the original on 2020-08-04. Retrieved 2022-09-05. Unknown parameter
|url-status=ignored (help) - ↑ "Choosing BOINC projects". boinc.berkeley.edu. Retrieved 2022-09-16.
- ↑ "Science". scienceunited.org. Archived from the original on 2021-09-18. Retrieved 2021-09-14. Unknown parameter
|url-status=ignored (help) - ↑ "Research in physics, astronomy Poland Universe@Home". universeathome.pl. Archived from the original on 2022-08-15. Retrieved 2022-09-05. Unknown parameter
|url-status=ignored (help) - ↑ "Universe@Home/en - BC-Wiki". wiki.bc-team.org. Retrieved 2022-09-29.
- ↑ "Universe@Home Universe@Home results database". universeathome.pl. Archived from the original on 2021-09-14. Retrieved 2021-09-14. Unknown parameter
|url-status=ignored (help) - ↑ Wiktorowicz, Grzegorz; Sobolewska, Małgorzata; Sa˛dowski, Aleksander; Belczynski, Krzysztof (2015-08-25). "Nature of the Extreme Ultraluminous X-Ray Sources". The Astrophysical Journal. 810 (1): 20. arXiv:1503.08745. Bibcode:2015ApJ...810...20W. doi:10.1088/0004-637x/810/1/20. hdl:1721.1/100049. ISSN 1538-4357. Unknown parameter
|s2cid=ignored (help) - ↑ Belczynski, Krzysztof; Holz, Daniel E.; Bulik, Tomasz; O'Shaughnessy, Richard (2016-06-23). "The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars". Nature. 534 (7608): 512–515. arXiv:1602.04531. doi:10.1038/nature18322. ISSN 0028-0836. PMID 27337338. Unknown parameter
|s2cid=ignored (help) - ↑ Wiktorowicz, Grzegorz; Sobolewska, Małgorzata; Lasota, Jean-Pierre; Belczynski, Krzysztof (2017-08-25). "The Origin of the Ultraluminous X-Ray Sources". The Astrophysical Journal. 846 (1): 17. arXiv:1705.06155. Bibcode:2017ApJ...846...17W. doi:10.3847/1538-4357/aa821d. ISSN 1538-4357. Unknown parameter
|s2cid=ignored (help) - ↑ Klencki, Jakub; Wiktorowicz, Grzegorz; Gładysz, Wojciech; Belczynski, Krzysztof (2017-06-01). "Dynamical formation of black hole low-mass X-ray binaries in the field: an alternative to the common envelope". Monthly Notices of the Royal Astronomical Society. 469 (3): 3088–3101. doi:10.1093/mnras/stx842. ISSN 0035-8711.
- ↑ Wiktorowicz, G.; Drago, A.; Pagliara, G.; Popov, S. B. (2017). "Strange Quark Stars in Binaries: Formation Rates, Mergers, and Explosive Phenomena". The Astrophysical Journal. 846 (2): 163. arXiv:1707.01586. Bibcode:2017ApJ...846..163W. doi:10.3847/1538-4357/aa8629. Retrieved 2022-09-24. Unknown parameter
|s2cid=ignored (help) - ↑ Belczynski, K.; Askar, A.; Arca-Sedda, M.; Chruslinska, M.; Donnari, M.; Giersz, M.; Benacquista, M.; Spurzem, R.; Jin, D.; Wiktorowicz, G.; Belloni, D. (2018-07-01). "The origin of the first neutron star – neutron star merger". Astronomy & Astrophysics. 615: A91. arXiv:1712.00632. Bibcode:2018A&A...615A..91B. doi:10.1051/0004-6361/201732428. ISSN 0004-6361. Unknown parameter
|s2cid=ignored (help) - ↑ Belczynski, K.; Bulik, T.; Olejak, A.; Chruslinska, M.; Singh, N.; Pol, N.; Zdunik, L.; O'Shaughnessy, R.; McLaughlin, M.; Lorimer, D.; Korobkin, O.; Heuvel, E. P. J. van den; Davies, M. B.; Holz, D. E. (2018-12-25). "Binary neutron star formation and the origin of GW170817". arXiv:1812.10065.
- ↑ Merritt, David (2015-08-24). "Gravitational Encounters and the Evolution of Galactic Nuclei. III. Anomalous Relaxation". The Astrophysical Journal. 810 (1): 2. arXiv:1509.01263. Bibcode:2015ApJ...810....2M. doi:10.1088/0004-637x/810/1/2. ISSN 1538-4357. Unknown parameter
|s2cid=ignored (help) - ↑ Wiktorowicz, Grzegorz; Lasota, Jean-Pierre; Middleton, Matthew; Belczynski, Krzysztof (2019-04-16). "The Observed versus Total Population of ULXs". The Astrophysical Journal. 875 (1): 53. arXiv:1811.08998. Bibcode:2019ApJ...875...53W. doi:10.3847/1538-4357/ab0f27. ISSN 1538-4357. Unknown parameter
|s2cid=ignored (help) - ↑ Wiktorowicz, Grzegorz; Wyrzykowski, Łukasz; Chruslinska, Martyna; Klencki, Jakub; Rybicki, Krzysztof A.; Belczynski, Krzysztof (2019-10-24). "Populations of Stellar-mass Black Holes from Binary Systems". The Astrophysical Journal. 885 (1): 1. arXiv:1907.11431. Bibcode:2019ApJ...885....1W. doi:10.3847/1538-4357/ab45e6. hdl:2066/209230. ISSN 1538-4357. Unknown parameter
|s2cid=ignored (help) - ↑ Wiktorowicz, Grzegorz; Lu, Youjun; Wyrzykowski, Łukasz; Zhang, Haotong; Liu, Jifeng; Justham, Stephen; Belczynski, Krzysztof (2020-12-01). "Noninteracting Black Hole Binaries with Gaia and LAMOST". The Astrophysical Journal. 905 (2): 134. arXiv:2006.08317. Bibcode:2020ApJ...905..134W. doi:10.3847/1538-4357/abc699. ISSN 0004-637X. Unknown parameter
|s2cid=ignored (help) - ↑ Wiktorowicz, Grzegorz; Lasota, Jean-Pierre; Belczynski, Krzysztof; Lu, Youjun; Liu, Jifeng; Iłkiewicz, Krystian (2021-09-01). "Wind-powered Ultraluminous X-ray Sources". The Astrophysical Journal. 918 (2): 60. arXiv:2103.02026. Bibcode:2021ApJ...918...60W. doi:10.3847/1538-4357/ac0cf7. ISSN 0004-637X. Unknown parameter
|s2cid=ignored (help) - ↑ Wiktorowicz, Grzegorz; Middleton, Matthew; Khan, Norman; Ingram, Adam; Gandhi, Poshak; Dickinson, Hugh (2021). "Predicting the self-lensing population in optical surveys". Monthly Notices of the Royal Astronomical Society. 507: 374–384. doi:10.1093/mnras/stab2135. Retrieved 2022-09-24.
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