Nobel Prize awarded to gravitational wave researchers
Congratulations from the Max Planck Institute for Gravitational Physics in Potsdam and Hannover, and the Leibniz Universität Hannover
The Max Planck Institute for Gravitational Physics (Albert Einstein Institute/AEI) in Potsdam and Hannover, and the Leibniz Universität Hannover congratulate Rainer Weiss, Barry C. Barish and Kip S. Thorne for receiving the 2017 Nobel Prize in Physics: “Our heartfelt congratulations to our colleagues. We are delighted that these three pioneers of gravitational wave research, who never lost track of their goal and inspired generations of young scientists, are honored with this award,” say Bruce Allen, Alessandra Buonanno and Karsten Danzmann, directors at the AEI and Bernard F. Schutz, AEI founding director, who retired in 2014. “We are proud to be part of the international collaboration which discovered the first gravitational wave passing through the Earth two years ago. This was a turning point in astronomy and astrophysics and provided us with a new tool to observe the Universe.”
Since the 1960s, gravitational wave research has been conducted by an international collaboration of scientists who worked closely together despite the challenges of the cold war and funding shortages in many countries. Max Planck scientists were involved right from the beginning and have made many key contributions. Today the field has grown into a global network of more than 1000 scientists.
Researchers at the Max Planck Institute for Gravitational Physics (Albert Einstein Institute; AEI) in Hannover and Potsdam, Germany, and from the Institute for Gravitational Physics at Leibniz Universität Hannover have made crucial contributions to the discoveries in several key areas:
- development and operation of highly sensitive detectors pushed to the limits of physics,
- efficient data analysis methods running on powerful computer clusters, and
- construction of accurate waveform models for the detection and interpretation of signals.
The first direct detection of gravitational waves on 14th of September 2015 was the culmination of decades of research in gravitational wave detection in the Max Planck Society going back to the very beginning of the field in the 1960s. A Max Planck group at the MPI for Physics and Astrophysics in Munich led by Heinz Billing († 4th of January 2017) conducted coincidence experiments between resonant mass detectors to disprove the early claims of gravitational wave detection in the 1960s. At the beginning of the 1970s, Billing's group began – at that time as the only people in the world – to work with laser interferometry. The group built prototypes and pushed technology development ahead.
The Max Planck Society consistently supported this group after Billing retired, passing the baton to Gerd Leuchs in 1986 and in 1989 to Karsten Danzmann. With British partners at the Universities of Glasgow and Cardiff, they were the first to design and propose a large-scale interferometric detector with 3 kilometer long arms, but funding for such an instrument was not available in Germany.
In 1995 the Max Planck Society brought Bernard Schutz from Cardiff to Germany to help found the AEI, first in Potsdam and in 2002 in Hannover, with the explicit mission to become a world centre for gravitational-wave research. The Leibniz Universität Hannover and the Volkswagenstiftung had come on board just before, and the cooperation with Glasgow and Cardiff was intensified. In 1994 that was the starting point for GEO600, a low-cost German-British gravitational wave observatory, which – in parallel to observation runs with the LIGO and Virgo instruments – has been serving as a think tank for detector development ever since. The high-end technology created here now can be found at the heart of all large gravitational wave observatories, including Advanced LIGO.
While experimentalists were constructing ever more sensitive instruments, theorists were developing precise ideas of what the expected gravitational wave signals and their sources would be like. Soon it became clear that complex data analysis methods would be needed to detect the faint signals. Bernard Schutz had pioneered these methods with data from the Munich and Glasgow small detector prototypes, and the AEI became a world center for the development of sophisticated analysis methods. Schutz also established what was then the world’s largest group for supercomputer simulations of black-hole mergers; such simulations were an integral part of the detection and interpretation of Advanced LIGO’s observations.
Simulated gravitational waveforms are important but not enough. Since data-analysis algorithms use several hundred thousand templates and it may take weeks to produce one single simulation, it is crucial to develop approximate but fast methods to solve the Einstein equations, so that waveforms can be quickly generated.
In the late 1990s Alessandra Buonanno, since 2014 director at the Max Planck Institute for Gravitational Physics in Potsdam and College Park Professor at the University of Maryland, and Thibault Damour (IHES, Paris) developed a novel approach to the binary-orbit problem that combines several approximate methods to construct waveforms from coalescing binary black holes. Over the last 15 years this formalism has been developed into a highly accurate method that also includes results from numerical-relativity simulations, and extends to binary neutron stars. Scientists at the AEI in Potsdam, and earlier at the University of Maryland, have been building accurate waveform models combining the best tools to solve Einstein equations and have been using them to detect gravitational waves in the Advanced LIGO observation runs. AEI Potsdam researchers also employ those waveform models to infer astrophysical and fundamental physics properties of the binary systems, and to test General Relativity.
Researchers at the Max Planck Institute for Gravitational Physics in Hannover, led by Bruce Allen, use these templates to analyze the detector data on high-performance supercomputers. Once the signals have been found, the templates are used to infer astrophysical information upon the detection: where exactly is the source? What is its nature? Black holes and/or neutron stars? What are their masses and spins?
For the first detections of gravitational waves the AEI researchers carried out most of the production data analysis. In addition, about half of the computational resources for the discoveries and analysis of the Advanced LIGO data were provided by Atlas, the most powerful computer cluster in the world designed for gravitational-wave data analysis, operated by the AEI in Hannover. Atlas has provided about 160 million CPU core hours for the analysis of Advanced LIGO data.
This close interplay of experiment, simulations, analytical calculations, and data analysis ultimately allows scientists to bring light into the dark and invisible side of the Universe. Today’s Nobel Prize announcement honors the founding fathers of this field whose pioneering work rendered the dawn of a new era of astronomy possible.
EM / KNI / HOR