Einstein@Home

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Einstein@Home is a distributed computing project running on the Berkeley Open Infrastructure for Network Computing (BOINC) software platform. It searches for unknown pulsars and gravitational waves.

1 Introduction
2 Scientific objectives
3 Data analysis
4 Optimized data analysis
5 See also
6 References
7 Further reading
8 External links

[edit] Introduction

A BOINC distributed computing project

Einstein@Home is designed to search data collected by the Laser Interferometer Gravitational-Wave Observatory (LIGO) and GEO 600 for gravitational waves. The project was officially launched on 19 February 2005 as part of American Physical Society's contribution to the World Year of Physics 2005. ^[1] It uses the power of volunteer-driven distributed computing in solving the computationally intensive problem of analyzing a large volume of data. Such an approach was pioneered by the SETI@home project, which is designed to look for signs of extra-terrestrial life by analyzing radio wave data. Einstein@Home runs through the same software platform as SETI@home, the Berkeley Open Infrastructure for Network Computing (BOINC).

As of June 3, 2006, over 120,000 volunteers in 186 countries have participated in the project, making it the second most popular BOINC project. ^[2]

[edit] Scientific objectives

The Einstein@home screensaver

The Einstein@Home project searches for previously unknown pulsars, via an "all-sky pulsar search". ^[3] The results of this search are then used by the LIGO/GEO teams to search their data for gravitational waves emitted from bumps on the surface of known pulsars.

Einstein@Home may result in the first confirmed direct detection of a gravitational wave if LIGO/GEO detect a distinctive sequence of signals which should result from the inwards spiral and merger of a pair of black holes. However the rate of binary inspiral and the number density and properties of pulsars have large uncertainties.

A successful detection of gravitational waves would constitute a significant milestone in physics, as this the first detection of a previously unknown astronomical object by means of gravitational radiation alone.

[edit] Data analysis

The Einstein@Home program processes data from the LIGO and GEO instruments using Fast Fourier Transforms. The resulting signals are then analyzed using a method called matched filtering. This method involves the computation of hypothetical signals that might result if there were a physically plausible source of gravitational waves in the part of the sky being examined. The measured signal is then compared to the hypothetical signal. A matching signal is a candidate for further examination by more sophisticated analysis. ^[4]

Einstein@Home analyzes data from the LIGO S3, S4 and S5 datasets, each of which represent improvements in the accuracy compared with the previous data set. Processing of the S3 dataset was conducted between 22 February 2005 and 2 August 2005. Work on the S4 data set was started interlaced with the S3 calculations, and has finished in July 2006. Processing of the S5 data set, which should reach design sensitivity for the first time, began on 15 June 2006.^[5]

As of November 2006, the project reports 80.5 teraflops of computational power.[1]

[edit] Optimized data analysis

Einstein@home has gained considerable attention of the world's distributed computing community when an optimized application for the S4 data set analysis was developed and released in March 2006 by project volunteer Akos Fekete, a Hungarian programmer. ^[6] Fekete improved the official S4 application and introduced SSE, 3DNow! and SSE3 optimizations into the code improving performance by up to 800%^{[citation needed]}. Fekete was recognized for his efforts and was afterwards officially involved with the Einstein@home team in the development of the new S5 application. ^[7] As of late July 2006 this new official application became widely distributed among the Einstein@home users, creating a large surge in the project's total performance and productivity, best measured by floating point speed (or FLOPS), which has increased by approximately 50% compared to non-optimized S4 application. ^[8]