Universe@Home: Difference between revisions
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# '''[https://arxiv.org/abs/1811.08998 ''The observed vs total population of ULXs'']''' Wiktorowicz et al. 2019 | # '''[https://arxiv.org/abs/1811.08998 ''The observed vs total population of ULXs'']''' Wiktorowicz et al. 2019 | ||
# '''[https://arxiv.org/abs/1812.10065 ''Binary neutron star formation and the origin of GW170817'']''' Belczynki et al. 2018 | # '''[https://arxiv.org/abs/1812.10065 ''Binary neutron star formation and the origin of GW170817'']''' Belczynki et al. 2018 | ||
# '''[https://arxiv.org/abs/1712.00632 The origin of the first neutron star -- neutron star merger]''' Belczynki et al. 2018 | # '''[https://arxiv.org/abs/1712.00632 ''The origin of the first neutron star -- neutron star merger'']''' Belczynki et al. 2018 | ||
# '''[https://arxiv.org/abs/1708.07885 ''Double neutron stars: merger rates revisited'']''' Chruślińska et al. 2017 | # '''[https://arxiv.org/abs/1708.07885 ''Double neutron stars: merger rates revisited'']''' Chruślińska et al. 2017 | ||
# '''[https://arxiv.org/abs/1707.01586 ''Strange quark stars in binaries: formation rates, mergers and explosive phenomena'']''' Wiktorowicz et al. 2017 | # '''[https://arxiv.org/abs/1707.01586 ''Strange quark stars in binaries: formation rates, mergers and explosive phenomena'']''' Wiktorowicz et al. 2017 | ||
Revision as of 22:50, 7 April 2024
BOINC project page template
[[File:{{#setmainimage:[email protected]}}|alt=Universe@home logo image|center|frameless]]
Universe@Home is a BOINC platform based volunteer computing project that needs your help to run simulations of our Universe.
Why Universe@Home?
- why this topic/object of study?
Goal
- summarize the objectives and challenges which the project addresses, before jumping into details
Methods
- always including "why BOINC"?
- insert MediaWiki image or upload
example MediaWiki image - impactful final statement
Project team / Sponsors
Copernicus Astronomical Centre of the Polish Academy of Sciences. Project server managed: Krzysztof 'krzyszp' Piszczek.
Scientific results
At the moment there are six sets of data:
- X-ray
- QuarkStars
- Black hole database
- Dynamical formation of XRBs with black holes
- BH NS formation database files
- Self-lensing binary predictions
Scientific publications
- Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries Banerjee et al. 2023
- Populations of stellar mass Black holes from binary systems Wiktorowicz et al. 2019
- Merger of compact stars in the two-families scenario De Pietri et al. 2019
- The observed vs total population of ULXs Wiktorowicz et al. 2019
- Binary neutron star formation and the origin of GW170817 Belczynki et al. 2018
- The origin of the first neutron star -- neutron star merger Belczynki et al. 2018
- Double neutron stars: merger rates revisited Chruślińska et al. 2017
- Strange quark stars in binaries: formation rates, mergers and explosive phenomena Wiktorowicz et al. 2017
- The evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates of LIGO/Virgo binary black holes Belczynski et al. 2017
- The origin of the Ultraluminous X-ray Sources Wiktorowicz et al. 2017
- The Effect of Pair-Instability Mass Loss on Black Hole Mergers Belczynski et al. 2016
- Spectroscopy of Kerr black holes with Earth- and space-based interferometers Berti et al. 2016
- The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars Belczynski et al. 2016
- Nature of the Extreme Ultraluminous X-ray Sources Wiktorowicz et al. 2015