How does gravitational redshift relate to black holes?
How does gravitational redshift relate to black holes?
General relativity predicts that light emitted by an object in a strong gravitational field—for example, close to a black hole—should be shifted to longer wavelengths. These results are more consistent with general relativity than Newtonian gravity at the 5σ level. …
What is the Schwarzschild of a black hole?
For a non-rotating black hole, the radius of the event horizon is known as the Schwarzschild radius, and marks the point at which the escape velocity from the black hole equals the speed of light.
Do black holes cause redshift?
The new measurements clearly reveal an effect called gravitational redshift. Light from the star is stretched to longer wavelengths by the very strong gravitational field of the black hole, making it appear red.
What shifts in the gravitational redshift?
Einstein’s theory of general relativity predicts that the wavelength of electromagnetic radiation will lengthen as it climbs out of a gravitational well. This corresponds to an increase in the wavelength of the photon, or a shift to the red end of the electromagnetic spectrum – hence the name: gravitational redshift.
How does the Schwarzschild solution work for black holes?
If we pick an origin, then is clearly spherically symmetric with respect to rotations around this origin. Under such rotations ( i.e., under the flow of the Killing vector fields) points move into each other, but each point stays on an S2 at a fixed distance from the origin.
What does the term gravitational redshift mean in physics?
Gravitational redshift. In Einstein’s general theory of relativity, the gravitational redshift is the phenomenon that clocks in a gravitational field tick slower when observed by a distant observer. More specifically the term refers to the shift of wavelength of a photon to longer wavelength (the red side in an optical spectrum)…
Which is the horizon of a black hole?
The Schwarzschild surface, the sphere at \\(1\\) Schwarzschild radius, is also called the horizon of a black hole, since an outside observer, even one just outside the Schwarzschild surface, can see nothing beyond the horizon.
How did Einstein discover the gravitational redshift in the Solar System?
The gravitational redshift is a simple consequence of Einstein’s equivalence principle (that gravity and acceleration are equivalent) and was found by Einstein eight years before the full theory of relativity. Observing the gravitational redshift in the solar system is one of the classical tests of general relativity.