People

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Prof. Dr. Bruce Allen
Director
Phone:+49 511 762-17148Fax:+49 511 762-17182

Homepage of Bruce Allen

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Christian Beer
Phone:+49 511 762-17468Fax:+49 511 762-2784
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Oliver Bock
Phone:+49 511 762-17165Fax:+49 511 762-2784
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Dr. Colin Clark
Phone:+49 511 762-17187Fax:+49 511 762-2784
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Heinz-Bernd Eggenstein
Phone:+49 511 762-17098Fax:+49 511 762-2784
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Bernd Machenschalk
Phone:+49 511 762-19463Fax:+49 511 762-2784
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Dr. Maria Alessandra Papa
Phone:+49 511 762-17160Fax:+49 511 762-17182
Email:papa@...

Personal homepage

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Dr. Reinhard Prix
Phone:+49 511 762-17154Fax:+49 511 762-2784
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Avneet Singh
Phone:+49 511 762-17150Fax:+49 511 762-2784
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Dr. Sinéad Walsh
Phone:+49 511 762-17120Fax:+49 511 762-2784

Member of Astrophysical and Cosmological Relativity

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Dr. Sylvia Zhu
Phone:+49 511 762-17169Fax:+49 511 762-2784

volunteer distributed computing

Einstein@Home

Einstein@Home is one of the largest distributed volunteer computing projects in the world and has more than 440,000 participants. Their computers provide a sustained computing power of roughly 1.7 PetaFlop/s. If the project were listed on the Top-500, Einstein@Home would be one of the 60 most powerful computers in the world (as of Nov. 2016).

Join Einstein@Home!

Einstein@Home uses idle computing time donated by volunteers all around the world to search for weak astrophysical signals from spinning neutron stars (also called pulsars). The project analyzes data from the LIGO gravitational-wave detectors, the Arecibo and Parkes radio telescopes, and the Fermi gamma-ray satellite.

Einstein@Home volunteers have already discovered more than 70 new neutron stars, and we hope to find many more in the future. Our long-term goal is to make the first direct detections of gravitational-wave emission from spinning neutron stars. Gravitational waves were predicted by Albert Einstein almost a century ago. In September 2015 they were finally detected for the first time ever, ushering in a new era in astronomy.

Einstein@Home was started in 2005 and since then has been searching for gravitational wave signals from rapidly rotating neutron stars in the data from the LIGO and Virgo detectors. Search runs with improving sensititivity provide improving upper limits on the emission of continuous gravitational waves from a Galactic population of neutron stars.

In spring 2009, Einstein@Home launched a new search for radio pulsars in binary systems using data from the Arecibo Radio Observatory in Puerto Rico. This work was developed at the AEI in Hannover in collaboration with the PALFA collaboration, then led by Prof. Jim Cordes at Cornell. While this search is intended to find new radio pulsars in sub-hour period binary orbits, it is also sensitive to isolated radio pulsars and to radio pulsars in longer period orbits. By late 2016 this search had already discovered 55 previously unknown pulsars.

The Einstein@Home radio pulsar search codes also run on GPU-based hardware that can carry out floating-point operations a factor of twenty (or even more) faster than conventional CPUs. Einstein@Home provides applications for Nvidia GPUs using CUDA and for ATI/AMD graphics cards through OpenCL.

Since mid 2011, Einstein@Home also analyzes data from the Fermi gamma-ray satellite using novel methods initially developed for continuous gravitational-wave searches at the AEI in Hannover. As of December 2016, Einstein@Home has discovered 18 new gamma-ray pulsars.

Einstein@Home is a World Year of Physics 2005 and an International Year of Astronomy 2009 project supported by the American Physical Society (APS) and by a number of international organizations.

Einstein@Home research releases

 
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