Universe@Home: Difference between revisions

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== Project team / Sponsors ==
== Project team / Sponsors ==
Copernicus Astronomical Centre of the Polish Academy of Sciences. Project server managed: Krzysztof 'krzyszp' Piszczek.


== Scientific results ==
== Scientific results ==
* external links
At the moment there are six sets of data:
#'''''[https://universeathome.pl/universe/x-ray.php X-ray]'''''
#'''''[https://universeathome.pl/universe/qs.php QuarkStars]'''''
#'''''[https://universeathome.pl/universe/bhdb.php Black hole database]'''''
#'''''[https://universeathome.pl/universe/xbhms.php Dynamical formation of XRBs with black holes]'''''
#'''[https://universeathome.pl/universe/bhns.php ''BH NS formation database files'']'''
#'''''[https://universeathome.pl/universe/self_lensing.php Self-lensing binary predictions]'''''


== Scientific publications ==
== Scientific publications ==
Format example:
 
# Durech, J., B. Carry, M. Delbo, M. Kaasalainen and M. Viikinkoski. [https://arxiv.org/abs/1502.04816 Asteroid Models from Multiple Data Sources.] (2015). DOI: 10.48550/ARXIV.1502.04816.
# '''[https://arxiv.org/pdf/2302.10851.pdf ''Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries'']''' Banerjee et al. 2023
# '''[https://arxiv.org/abs/1907.11431 ''Populations of stellar mass Black holes from binary systems'']''' Wiktorowicz et al. 2019
# '''[https://arxiv.org/abs/1904.01545 ''Merger of compact stars in the two-families scenario'']''' De Pietri 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/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/1707.01586 ''Strange quark stars in binaries: formation rates, mergers and explosive phenomena'']''' Wiktorowicz et al. 2017
# '''[https://arxiv.org/abs/1706.07053 ''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
# '''[https://arxiv.org/abs/1705.06155 ''The origin of the Ultraluminous X-ray Sources'']''' Wiktorowicz et al. 2017
# '''[https://arxiv.org/abs/1607.03116 ''The Effect of Pair-Instability Mass Loss on Black Hole Mergers'']''' Belczynski et al. 2016
# '''''[https://arxiv.org/abs/1605.09286 Spectroscopy of Kerr black holes with Earth- and space-based interferometers]''''' Berti et al. 2016
# '''''[https://arxiv.org/abs/1602.04531 The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars]''''' Belczynski et al. 2016
# '''''[https://arxiv.org/abs/1503.08745 Nature of the Extreme Ultraluminous X-ray Sources]''''' Wiktorowicz et al. 2015

Revision as of 22:39, 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
    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:

  1. X-ray
  2. QuarkStars
  3. Black hole database
  4. Dynamical formation of XRBs with black holes
  5. BH NS formation database files
  6. Self-lensing binary predictions

Scientific publications

  1. Symmetry breaking in merging binary black holes from young massive clusters and isolated binaries Banerjee et al. 2023
  2. Populations of stellar mass Black holes from binary systems Wiktorowicz et al. 2019
  3. Merger of compact stars in the two-families scenario De Pietri et al. 2019
  4. The observed vs total population of ULXs Wiktorowicz et al. 2019
  5. Binary neutron star formation and the origin of GW170817 Belczynki et al. 2018
  6. The origin of the first neutron star -- neutron star merger Belczynki et al. 2018
  7. Double neutron stars: merger rates revisited Chruślińska et al. 2017
  8. Strange quark stars in binaries: formation rates, mergers and explosive phenomena Wiktorowicz et al. 2017
  9. 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
  10. The origin of the Ultraluminous X-ray Sources Wiktorowicz et al. 2017
  11. The Effect of Pair-Instability Mass Loss on Black Hole Mergers Belczynski et al. 2016
  12. Spectroscopy of Kerr black holes with Earth- and space-based interferometers Berti et al. 2016
  13. The first gravitational-wave source from the isolated evolution of two 40-100 Msun stars Belczynski et al. 2016
  14. Nature of the Extreme Ultraluminous X-ray Sources Wiktorowicz et al. 2015
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