Einstein@home/en

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Einstein@Home is a method to search for gravitational waves from very dense, rapidly-spinning stars, such as neutron or quark stars. The frequency of the waves is typically twice the star's spin frequency, though other frequencies are also possible. Thus, if the star is spinning about its axis 100 times per second, we might expect gravitational waves to be emitted primarily at a frequency of 200 cycles per second (Hz).		Einstein@home Screensaver Start 2004 End Status Admin Bruce Allen, Bernd Machenschalk Institution Collaboration Country International Area Physics Apps Win {{{Windows}}} Linux {{{Linux}}} Mac {{{Mac}}} 64bit {{{64bit}}} PS3 {{{PS3}}} ATI {{{ATI}}} CUDA {{{CUDA}}} Intel {{{Intel}}} Android [[Bild:{{{Android}}}.gif|link=]] RPi [[Bild:{{{RPI}}}.gif|link=]] NCI [[Bild:{{{NCI}}}.gif|link=]] System-Specs VRAM {{{VRAM}}} SP [[Bild:{{{SP}}}.gif|link=]] DP [[Bild:{{{DP}}}.gif|link=]] RAM 7MB Runtime HDD 50MB Traffic dl/ul 6MB / 137kb Deadline 14 days Checkpoints

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