Gravitational radiation

In physics, a gravitational wave consists of energy transmitted in the form of a wave through the gravitational field of space-time. Gravitational radiation is the overall result of gravitational waves in bulk. The theoretical treatment of gravitational waves is governed by general relativity. The Einstein field equations imply that any accelerated mass emits gravitational radiation, travelling at c, similar to how the Maxwell equations describe the electromagnetic radiation emitted by an accelerated electric charge.

Gravitational waves should not be confused with gravity waves in hydrodynamics.


Gravitational waves


According to general relativity, gravity can cause oscillations (or waves) in spacetime which can transmit energy. Roughly speaking, the strength of gravity will vary as a gravitational wave passes, much as the depth of a body of water will vary as a water wave passes. More precisely, it is the strength and direction of tidal forces (measured by the Weyl tensor) that oscillate, which should cause objects in the path of the wave to change shape (but not size) in a pulsating fashion. Similarly, gravitational waves will be emitted by physical objects with a pulsating shape, specifically objects with a changing quadrupole moment.

In 2005 it was announced that observations of the binary pulsar PSR J0737-3039 appeared to confirm predictions of general relativity with respect to energy emitted by gravitational waves, with the system's orbit observed to shrink 7 mm per day.

Sources of gravitational waves

One reason for the lack of direct detection so far is that the gravitational waves that we expect to be produced in nature are very weak, so that the signals for gravitational waves, if they exist, are buried under noise generated from other sources. Reportedly, ordinary terrestrial sources would be undetectable, despite their closeness, because of the great relative weakness of the gravitational force.

Scientists are eager to find a way to detect these gravitational waves, since they could help reveal information about the very structure of the universe. In contrast to electromagnetic radiation, it is not fully understood what difference the presence of gravitational radiation would make for the workings of the universe. A sufficiently strong sea of primordial gravitational radiation, with an energy density exceeding that of the big bang electromagnetic radiation by a few orders of magnitude, would shorten the life of the universe, violating existing data that show it is at least 13 billion years old. More promising is the hope to detect waves emitted by sources on astronomic size scales, such as:

What is more, a detection of gravitational waves of these objects might also give information about the objects themselves. Although the idea is far-fetched, some astronomers already dream of "gravitational telescopes" to see in gravity, as opposed to light.

Gravitational wave detectors

Gravitational radiation has not been directly observed, although there are a number of proposed experiments such as LIGO that intend to do so. Scientists are eager to implement experiments which propose to detect gravitational waves, not so much because of the expected observations, but because unexpected and surprising results are believed to be likely to be found. A number of teams are working on making more sensitive and selective gravitational wave detectors and analysing their results. A commonly used technique to reduce the effects of noise is to use coincidence detection to filter out events that do not register on both detectors. There are two common types of detectors used in these experiments:

In November 2002, a team of Italian researchers at the Instituto Nazionale di Fisica Nucleare and the University of Rome La Sapienza produced an analysis of their experimental results that may be further indirect evidence of the existence of gravitational waves. Their paper, entitled "Study of the coincidences between the gravitational wave detectors EXPLORER and NAUTILUS in 2001", is based on a statistical analysis of the results from their detectors which shows that the number of coincident detections is greatest when both of their detectors are pointing into the center of our Milky Way galaxy.

MiniGRAIL is a spherical gravitational wave antenna based at Leiden University.

Energy, momentum and angular momentum

Do gravitational waves carry energy, momentum and angular momentum? Well, in a vacuum, their stress-energy tensor would be zero. However, it's possible to define a noncovariant pseudo stress-energy tensor which is "conserved" such that they do carry them.


Bruce Allen of UWM's LIGO Scientific Collaboration, LSC group is leading the development of the Einstein@Home project, developed to search data from LIGO in the US and from the GEO 600 gravitational wave observatory in Germany for signals coming from selected, extremely dense, rapidly rotating stars. Such sources are believed to be either quark stars or neutron stars, and a subclass of these are already observed by conventional means, and are known as pulsars, electromagnetic wave emitting celestial bodies. If some of these stars are not quite near-perfectly spherical, they should emit gravitational waves, which LIGO and GEO 600 may begin to detect.

Einstein@Home is a small part of the LSC scientific program. It has been set up and released as a distributed computing project, like SETI@home. Meaning, it relies on computer time donated by private computer users to process data generated by LIGO's and GEO 600's search for gravity waves.

External links


ca:Ona gravitatria ja:重力波 (相対論) de:Gravitationswelle fr:Onde_gravitationnelle pl:Fale_grawitacyjne ru:Гравитационные волны


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