Difference between revisions of "General relativity"

Latest revision as of 09:38, 11 January 2017

Explanationedit

General relativity is the theory of gravitation that is widely accepted as the modern description of gravity, after several experimentations. Albert Einstein developed this geometrical manifestation of gravity as a set of ten field equations upon his special relativity, which establishes the relationship between space and time. The general relativity theory explains that the gravity is not a force as proposed by Newton, but a geometrical consequence of an object's mass, curving the spacetime around it. For example, in our solar system, the mass of the Sun curves the spacetime around it, and as a result, the planets fall towards it. The reason why they don't actually end up falling into the Sun is due to its high tangential velocity that forces them to miss their fall and orbit the sun instead. General relativity also predicts that gravity not only influences time but interacts with light by bending its path in a stronger field.

Frequently Asked Questionsedit

How gravity affects photons if they are massless?edit

Gravity (presence of matter or energy) bends spacetime, which is obviously the path that light would travel. As the path itself is curved, light has to travel in that curved path caused by gravity.

How gravity influences time?edit

Consider two observers with identical light clocks (A clock that measures time by measuring the number of times the light bounces off the two parallel mirrors inside the clock), living in two different gravitational fields, one stronger and the other weaker. When an observer from the weaker gravitational field looks at the clock in the stronger gravitational field, that clock will be ticking at a slower rate than his own clock. On the other hand, for the observer in the stronger field, he will observe that the clock in the weaker gravitational field ticking faster than his. This phenomenon is known as gravitational time dilation. As gravity can affect the path of the light and curve it, the light clocks will tick at different rates in different gravitational fields. The clock at a weaker gravitational field will have a less curvature locally when compared to the curvature around the clock at a stronger gravitational field. Light always travels at the same speed. speed = distance/time. In the stronger gravitational field, the distance is increased due to the curvature, thereby increasing the time light would take to reach the mirror. When the observer at a weaker gravitational field observes this clock, it would appear that the clock is ticking slowly relative to his clock.

What is gravitational lensing?edit

Gravitational lensing is the phenomenon in which a massive cluster of objects bends the light that traverses around it, due to their intense gravitational field. This usually happens when observing a very distant source of light (e.g. a quasar) and a massive cluster of galaxies happens to be in between the source and the observer. The following image is a good example of this phenomenon.

Pictured above, the gravity of a luminous red galaxy (LRG) has gravitationally distorted the light from a much more distant blue galaxy. More typically, such light bending results in two discernible images of the distant galaxy, but here the lens alignment is so precise that the background galaxy is distorted into a horseshoe -- a nearly complete ring. Since such a lensing effect was generally predicted in some detail by Albert Einstein over 70 years ago, rings like this are now known as Einstein Rings. Although LRG 3-757 was discovered in 2007 in data from the Sloan Digital Sky Survey (SDSS), the image shown above is a follow-up observation taken with the Hubble Space Telescope's Wide Field Camera 3. Strong gravitational lenses like LRG 3-757 are more than oddities -- their multiple properties allow astronomers to determine the mass and dark matter content of the foreground galaxy lenses.