Galaxies are not solitary objects – usually, they cluster together. Our own galaxy for instance, the Milky Way, is part of a small cluster called the local group of galaxies. The next-closest large galaxy cluster is the Virgo cluster.
Synonyms: gamma radiation
Astronomical events visible as extremely strong flashes of gamma rays. Their origin is still unclear; In the context of general relativity they are interesting because they are thought to signal the mergers of neutron stars and/or black holes. Shortly after the observation of the gravitational wave GW170817 a gamma ray burst was detected and thus underpins the hypothesis.
Synonyms: gamma burst
In a strict sense: A state of matter in which the atoms and/or molecules wildly careen and collide, without being bound to each other. This movement leads to an inner pressure, while the average kinetic energy of the moving particles is a measure for the temperature of the gas.
In a broader sense, gas is also used to denote other mixtures of freely careening particles, for instance in the case of the electron gas whose pressure stabilizes a white dwarf against further collapse.
general theory of relativity
For information about the concepts and applications of this theory, we recommend the chapter general relativity of our introductory section Elementary Einstein. Further information about many different aspects of general relativity and its applications can be found in our section Spotlights on relativity.
Synonyms: general relativity
British-German gravitational wave detector located in Ruthe (close to Hannover, Germany). GEO600 is an interferometric gravitational wave detector with an arm-length of 600 metres.
In classical mechanics, the rotation axis of a gyroscope on which no external forces are acting will remain constant – a useful property that has found applications in navigation. However, in the presence of spacetime curvature, this is no longer true – the axis direction of a gyroscope in free fall will change over time; an effect predicted by Einstein’s general theory of relativity.
That part of mathematics concerning itself with surfaces or more general spaces as well as objects defined on such spaces, such as points or lines as well as the objects constructable from points and lines, such as triangles.
See electron volt
global positioning system
A system of satellites and mobile receivers that makes it possible to determine each receiver’s position with high accuracy. Used by pilots, truckers, car drivers and by many smartphone users world-wide, it is an industrial application of Einstein’s theories of special and general relativity: Without taking into account the effects predicted by these theories for moving clocks in a gravitational field, there would be errors of roughly 10 kilometres per day of operation in the determination of positions on earth.
Gold nuclei, stripped of their electrons, are among the types of heavy ions which are brought into collision in particle accelerators such as the Relativistic Heavy Ion Collider in order to recreate the state of matter in the early universe shortly after the big bang.
Gowdy spacetimes (or universes) are simple expanding model universes. In contrast with the better known Friedmann-Lemaître-Robertson-Walker universes (the basis for the big bang models), Gowdy universes are not homogeneous. Instead, they are filled with a regular pattern of gravitational waves. A Gowdy T3 universe is the simplest kind of Gowdy universe, in which space has the shape of a three-dimensional torus.
More information about Gowdy universes can be found in the spotlight text Of gravitational waves and spherical chickens.
Synonyms: Gowdy universes Gowdy T3
In Einstein’s general theory of relativity: The fact that matter that possesses mass, energy, pressure or similar properties distorts spacetime, and that this distortion in turn influences whatever matter might be present.
An introduction to the basic ideas of general relativity is provided by the section General relativity of Elementary Einstein. More information about the nature of gravity in general relativity can be found in the spotlight text Gravity: From weightlessness to curvature.
Constant of nature; the fundamental Newton’s law of gravity and thus a measure for the natural strength of gravity. Analogously, in Einstein’s equations in the general theory of relativity, it occurs as the proportionality factor determining how strongly mass, energy and similar properties of matter distort space and time. In formulae, it is usually written as G. The best current value for G is
G = 6.674 30(15)·10-11m³kg-1s-2.
Compared with other fundamental constants, G is known only to a comparatively low accuracy.
The totality of all gravitational influences that one or more massive objects can exert on bodies in their vicinity.
More precisely: At every location in space, the gravitational field is defined as the acceleration that a small test particle present at that location would feel due to the gravitational forces of the masses around it.
In Einstein’s general relativity, gravity necessarily acts not only on material bodies, but also on light – light passing a massive body is deflected. This deflection can be so strong that light of one and the same cosmic object reaches an observer along multiple paths – corresponding to the observer seeing multiple images of that object in the sky. Masses that, in this sense, act like very special optical lenses are called gravitational lenses.
More information can be found in the spotlight text A brief history of gravitational lenses.
Synonyms: gravitational lensing
According to general relativity, light flying away from a massive body (or other source of gravity) experience a redshift – its frequency decreases and the light becomes less energetic. On the other hand, light flying towards a massive body gets blueshifted – its frequency and energy increase.
gravitational wave astronomy
Discipline of astronomy which aims at using gravitational waves to gain information about cosmic objects or the cosmos as a whole – for instance about what’s happening in the core region of a supernova, about neutron star or about the heated past of our universe.
gravitational wave detector
Currently, scientists world wide are attempting the direct measurement of gravitational waves reaching us from the depths of space. They are mainly using two types of detectors: interferometric detectors like GEO600 and the LIGO detectors, and resonant detectors.
Distortions of space geometry that propagate through space with the speed of light, analogous to ripples on the surface of a pond propagating as water waves.
See frame-dragging .
Synonyms: frame-dragging Lense-Thirring effect
GRAVITY is part of the Very Large Telescope Interferometer (VLTI) at the European Southern Observatory in Chile. The instrument operates in the near infrared and combines the light of four telescopes, whereby it achieves the spatial resolution of an equivalent telescope with 130 meters in diameter. Due to its high sensitivity and accuracy, it allows researchers to render very small and faint cosmic objects visible. GRAVITY also measures distances very accurately and is therefore very suitable for the measurement of movements. For example, with the help of GRAVITY, the motion of a star around the black hole at the centre of our galaxy could be observed, confirming the predictions of general relativity.
Circle on the surface of a sphere whose center coincides with that of the sphere itself. On the globe, the equator is a great circle, while every meridian corresponds to half of a great circle.
If you want to move on a spherical surface in the straightest possible way, choose a path along a great circle – in the language of mathematics this is equivalent to saying: great circles are geodesics of a spherical surface.