Max Planck Institute for Gravitational Physics

Last updated
Max Planck Institute for Gravitational Physics
(Albert Einstein Institute)
AbbreviationAEI
Formation1995
Typenon-profit research organization
Headquarters Potsdam-Golm and Hannover, Germany
Management
managing director Bruce Allen and deputy managing director Masaru Shibata
Main organ
Max Planck Society
Website www.aei.mpg.de

The Max Planck Institute for Gravitational Physics (Albert Einstein Institute) is a Max Planck Institute whose research is aimed at investigating Einstein's theory of relativity and beyond: Mathematics, quantum gravity, astrophysical relativity, and gravitational-wave astronomy. The institute was founded in 1995 and is located in the Potsdam Science Park in Golm, Potsdam and in Hannover where it closely collaborates with the Leibniz University Hannover. Both the Potsdam and the Hannover parts of the institute are organized in three research departments and host a number of independent research groups.

Contents

The institute conducts fundamental research in mathematics, data analysis, astrophysics and theoretical physics as well as research in laser physics, vacuum technology, vibration isolation and classical and quantum optics.

When the LIGO Scientific Collaboration announced the first detection of gravitational waves, researchers of the institute were involved in modeling, detecting, analysing and characterising the signals. The institute is part of a number of collaborations and projects: it is a main partner in the gravitational-wave detector GEO600; institute scientists are developing waveform-models that are applied in the gravitational-wave detectors for detecting and characterising gravitational waves. They are developing detector technology and are also analyzing data from the detectors of the LIGO Scientific Collaboration, the Virgo Collaboration and the KAGRA Collaboration. They also play a leading role in planning and preparing the space-based detector LISA (planned launch date: 2034) and are involved in developing the third generation of earth-bound gravitational-wave detectors (Einstein Telescope, Cosmic Explorer). The institute is also a major player in the Einstein@Home and PyCBC projects.

The Max Planck Institute for Gravitational Physics in Potsdam-Golm. AEI Potsdam Golm.jpg
The Max Planck Institute for Gravitational Physics in Potsdam-Golm.
The Max Planck Institute for Gravitational Physics in Hannover. AEI Hannover 2015.jpg
The Max Planck Institute for Gravitational Physics in Hannover.

From 1998 to 2015, the institute has published the open access review journal Living Reviews in Relativity. [1]

History

The newly founded institute started its work in April 1995 and has been located in Potsdam-Golm since 1999. [2]

In 2002 the institute opened a branch at the Universität Hannover with a focus on data analysis and the development and operation of gravitational-wave detectors on Earth and in space. The Hannover institute originated from the Institute for Atom and Molecule Physics (AMP) of the Universität Hannover, which was established in 1979 by the Department of Physics.

Research

The research focus of the institute is in the field of general relativity. It covers theoretical and experimental gravitational physics, quantum gravity, multi-messenger astronomy and cosmology. The institute has a strong research focus on gravitational-wave astronomy: five out of six departments are working on different aspects of this research field. Central research topics are:

All these efforts enable a new kind of astronomy, which began with the first direct detection of gravitational waves on Earth.

Scientists of the institute also work towards the unification of the fundamental theories of physicsgeneral relativity and quantum mechanics – into a theory of quantum gravity.

Departments

Directors

Independent research groups

Permanent independent research groups

Independent research groups

Max Planck Partner Groups

Max Planck Partner Groups carry out research in fields overlapping with those of the former host Max Planck institute. They are established to support junior scientists returning to their home country after a research stay at a Max Planck Institute. [18]

The Max Planck Institute for Gravitational Physics has two Max Planck Partner Groups: [19] [20]

Collaborative projects

Advanced LIGO and advanced Virgo

At AEI Hannover and AEI Potsdam, there are two LIGO Scientific Collaboration groups concerned with theory and data analysis of the LIGO and Virgo detectors. [21] [22] At AEI Hannover there is also the GEO group concerned with various experimental topics. [23] AEI researchers in Potsdam and Hannover analyse LIGO and Virgo data. They also develop predictions of gravitational-wave signals used for the search for mergers of black holes and neutron stars and their interpretation.

The AEI Hannover is a partner institution in the advanced LIGO project and contributed the pre-stabilized laser system [24] [25] [26] for the advanced LIGO detectors in Hanford and Livingston. AEI researchers help commissioning and operating the advanced LIGO interferometers.

In early 2018 researchers at AEI Hannover have developed, built, and helped install a squeezed-light source at the Advanced Virgo gravitational-wave detector. [27] During the third joint observation run of the gravitational-wave detectors, it reduced the quantum-mechanical background noise by about third, increasing the expected detection rate of binary neutron star mergers by up to 26%. [28] [29]

Einstein Telescope

Researchers at AEI contribute to the planning, development of, and the science case [30] for the Einstein Telescope (ET), a third-generation gravitational-wave detector in Europe. The ET steering committee co-chair is at AEI Hannover, [31] and laser technology for the ET Prototype in Maastricht is to be developed at AEI Hannover. [32] AEI Potsdam researchers contribute to developing wave-form models for third generation gravitational-wave detectors such as the Einstein Telescope. [33]

GEO600

The GEO600 gravitational-wave detector south of Hannover was designed and is operated by scientists from the Max Planck Institute for Gravitational Physics and the Leibniz Universität Hannover, along with partners in the United Kingdom. [34]

LISA Pathfinder

LISA Pathfinder was a test mission by ESA for the Laser Interferometer Space Antenna (LISA). It demonstrated key technologies for gravitational-wave detection in space. The Max Planck Institute for Gravitational Physics in Hannover and the Institute for Gravitational Physics at Leibniz Universität Hannover were responsible for and coordinated the German contribution to the mission. [35]

During the operations phase, Max Planck and Leibniz Universität researchers in Hannover were partners in the mission's data analysis. [36] They also played a leading role developing the analysis software LTPDA, a MATLAB toolbox. [37] AEI scientist took part in the mission operations shifts at ESOC.

LISA

The space-based gravitational-wave observatory LISA is developed under ESA leadership in collaboration with a scientific consortium. [38] The LISA consortium is led by AEI director Karsten Danzmann. [38] At AEI Hannover and AEI Potsdam there are LISA Consortium groups. [39] At AEI Hannover there are large laboratories for LISA laser interferometry experiments. [40]

GRACE Follow-On

GRACE-FO is a satellite-based geodesy mission that takes detailed measurements of the Earth's gravitational field and its temporal and spatial variations by interferometric distance measurements between two satellites. The laser ranging interferometer used for this purpose is a cooperation between NASA and German partners, with the German contribution led by the AEI. The instrument's concept, its prototypes and technical specifications were done at the AEI. AEI researchers have been involved in developing and testing the flight hardware. [41]

Graduate Program

The institute participates in two International Max Planck Research Schools (IMPRS). Such research schools are graduate programs run by Max Planck Institutes in partnership with local universities, offering a Ph.D. degree. The IMPRS for Mathematical and Physical Aspects of Gravitation, Cosmology and Quantum Field Theory partners with the Institute for Mathematics at University of Potsdam, the Institute of Physics at Humboldt University, IIT Bombay, Chennai Mathematical Institute, and the Institute of Theoretical Physics of the Chinese Academy of Sciences [42]

The IMPRS on Gravitational Wave Astronomy is run in two collaborating branches, one in Hannover and one in Potsdam-Golm. The Hannover branch cooperates with the Leibniz University Hannover and the Laser Zentrum Hannover e.V.. [43] The Potsdam branch partners with the Humboldt University, the University of Potsdam and the Leibniz Institute for Astrophysics. [44] It cooperates with the IMPRS for Mathematical and Physical Aspects of Gravitation, Cosmology and Quantum Field Theory (also at AEI Potsdam), the master's degree program in astrophysics at the University of Potsdam, the Astrophysics Network Potsdam, the Yukawa Institute for Theoretical Physics at Kyoto University, and the University of Maryland. [45]

Jürgen Ehlers Spring School

The institute offers an annual two-week spring school for 40 international students of mathematics and physics. [46] Each year, the lectures, exercises, and discussions cover different topics from the institute's research expertise. Lectures are held by researchers from the institute.

The Jürgen Ehlers Spring School was established in 2000 and is named after the institute's founding director Jürgen Ehlers.

Outreach

Public events

The institute's outreach activities include Open Days at the AEI Potsdam and at the GEO600 gravitational-wave detector, participation in the Girls' Days and Future Days, popular science talks by researchers, [47] participation in the “November der Wissenschaft” in Hannover, [48] tours of the institutes including selected laboratories and computer clusters, and a program for visits and presentations by researchers at high schools. [49]

Einstein Online

The institute runs the popular-science webportal Einstein Online, [50] which is a hypertext network with introductory and in-depth articles about Einstein's theory of relativity and its consequences.

Journalist in Residence

Since 2018, the institute has been offering a Journalists-in-Residence program to science journalists. The goal is to improve the communication between journalists and scientists, and to provide deeper insight into the institute's research. [51]

Einstein@Home

The institute together with the University of Wisconsin–Milwaukee is one of the two host institutions of the distributed volunteer computing project Einstein@Home. [52] Einstein@Home aggregates computing time on volunteers’ computers to search for signals from rotating neutron stars in data from the LIGO gravitational-wave detectors, from large radio telescopes, and from the Fermi Gamma-ray Space Telescope.

Related Research Articles

In theories of quantum gravity, the graviton is the hypothetical quantum of gravity, an elementary particle that mediates the force of gravitational interaction. There is no complete quantum field theory of gravitons due to an outstanding mathematical problem with renormalization in general relativity. In string theory, believed by some to be a consistent theory of quantum gravity, the graviton is a massless state of a fundamental string.

<span class="mw-page-title-main">Gravity</span> Attraction of masses and energy

In physics, gravity (from Latin gravitas 'weight') is a fundamental interaction which causes mutual attraction between all things that have mass. Gravity is, by far, the weakest of the four fundamental interactions, approximately 1038 times weaker than the strong interaction, 1036 times weaker than the electromagnetic force and 1029 times weaker than the weak interaction. As a result, it has no significant influence at the level of subatomic particles. However, gravity is the most significant interaction between objects at the macroscopic scale, and it determines the motion of planets, stars, galaxies, and even light.

<span class="mw-page-title-main">LIGO</span> Gravitational wave detector

The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. Two large observatories were built in the United States with the aim of detecting gravitational waves by laser interferometry. These observatories use mirrors spaced four kilometers apart which are capable of detecting a change of less than one ten-thousandth the charge diameter of a proton.

<span class="mw-page-title-main">Kip Thorne</span> American physicist (born 1940)

Kip Stephen Thorne is an American theoretical physicist known for his contributions in gravitational physics and astrophysics.

<span class="mw-page-title-main">Joseph Weber</span> American physicist

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<span class="mw-page-title-main">Bruce Allen (physicist)</span> American physicist and director of the Max Planck Institute for Gravitational Physics

Bruce Allen is an American physicist and director of the Max Planck Institute for Gravitational Physics in Hannover Germany and leader of the Einstein@Home project for the LIGO Scientific Collaboration. He is also a physics professor at the University of Wisconsin–Milwaukee and the initiator / project leader of smartmontools hard disk utility.

<span class="mw-page-title-main">GEO600</span> Gravitational wave detector in Germany

GEO600 is a gravitational wave detector located near Sarstedt, a town 20 km to the south of Hanover, Germany. It is designed and operated by scientists from the Max Planck Institute for Gravitational Physics, Max Planck Institute of Quantum Optics and the Leibniz Universität Hannover, along with University of Glasgow, University of Birmingham and Cardiff University in the United Kingdom, and is funded by the Max Planck Society and the Science and Technology Facilities Council (STFC). GEO600 is capable of detecting gravitational waves in the frequency range 50 Hz to 1.5 kHz, and is part of a worldwide network of gravitational wave detectors. This instrument, and its sister interferometric detectors, when operational, are some of the most sensitive gravitational wave detectors ever designed. They are designed to detect relative changes in distance of the order of 10−21, about the size of a single atom compared to the distance from the Sun to the Earth. Construction on the project began in 1995.

Martin Bojowald is a German physicist who now works on the faculty of the Penn State Physics Department, where he is a member of the Institute for Gravitation and the Cosmos. Prior to joining Penn State he spent several years at the Max Planck Institute for Gravitational Physics in Potsdam, Germany. He works on loop quantum gravity and physical cosmology and is credited with establishing the sub-field of loop quantum cosmology.

<span class="mw-page-title-main">Gravitational wave</span> Propagating spacetime ripple

Gravitational waves are waves of the intensity of gravity that are generated by the accelerated masses of binary stars and other motions of gravitating masses, and propagate as waves outward from their source at the speed of light. They were first proposed by Oliver Heaviside in 1893 and then later by Henri Poincaré in 1905 as the gravitational equivalent of electromagnetic waves.

<span class="mw-page-title-main">Gravitational-wave astronomy</span> Branch of astronomy using gravitational waves

Gravitational-wave astronomy is an emerging field of science, concerning the observations of gravitational waves to collect relatively unique data and make inferences about objects such as neutron stars and black holes, events such as supernovae, and processes including those of the early universe shortly after the Big Bang.

Bernard F. Schutz FInstP FLSW is an American and naturalised British physicist. He is well known for his research in Einstein's theory of general relativity, especially for his contributions to the detection of gravitational waves, and for his textbooks. Schutz is a Fellow of the Royal Society and a Member of the US National Academy of Sciences. He is a professor of physics and astronomy at Cardiff University, and was a founding director of the Max Planck Institute for Gravitational Physics in Potsdam, Germany, where he led the Astrophysical Relativity division from 1995 to 2014. Schutz was a founder and principal investigator of the GEO gravitational wave collaboration, which became part of the LIGO Scientific Collaboration (LSC). Schutz was also one of the initiators of the proposal for the space-borne gravitational wave detector LISA, and he coordinated the European planning for its data analysis until the mission was adopted by ESA in 2016. Schutz conceived and in 1998 began publishing from the AEI the online open access (OA) review journal Living Reviews in Relativity, which for many years has been the highest-impact OA journal in the world, as measured by Clarivate.

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<span class="mw-page-title-main">First observation of gravitational waves</span> 2015 direct detection of gravitational waves by the LIGO and VIRGO interferometers

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52°24′59″N12°58′9″E / 52.41639°N 12.96917°E / 52.41639; 12.96917