Einstein shift
In the general theory of relativity by Albert Einstein, the gravitation redshift or Einstein shift is in the effect 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) when observed from a point in a lower gravitational field. In the latter case the 'clock' is the frequency of the photon and a lower frequency is the same as a longer ("redder") wavelength.The gravitational redshift is a simple consequence of the Einstein equivalence principle ("all bodies fall with the same acceleration, independent of their composition") and was found by Einstein eight years before the full theory.
Experimental verification of the gravitational redshift
requires good clocks since at Earth the effect is small.
The first experimental confirmation came as late as in 1960, in the famous
Pound-Rebka experiment (R.V. Pound, G.A. Rebka, Phys. Rev. Lett. 4, p.337)
later improved by Pound and Snider.
The famous experiment is generally called the
Pound-Rebka-Snider experiment.
They used a very well-defined "clock" in the form
of an atomic transition which results in a very narrow line of
electromagnetic radiation (a photon of well-defined energy). A
narrow line implies a very well defined frequency.
The line is in gamma ray range and emitted from the isotope Fe57 at 14.4 keV.
The narrowness of the line is caused by the so called Mossbauer effect.
The emitter and absorber were placed in a tower of
only 22 meter height at the bottom and top respectively.
The observed gravitational redshift
z, defined as the relative change in wavelength, the ratio
Note from the formula above that the loss of energy of the photon is just equal to the difference in potential energy ).
You can't make a perpetuum mobile by having photons going up and down in a gravitational field, something that was, strickly speaking, possible within Newton's theory of gravity.
For photons emitted from a stellar surface on a star of mass M
and radius R are expected to have a redshift
In addition, observation of much more massive and
compact stars such as white dwarfs have shown that Einstein shift does occur and is within the correct order of magnitude. Recently also the gravitational redshift of a neutron star has been measured from spectral lines in the x-ray range. The result gives the quantity M/R, the mass M and radius R of the neutron star. If the mass is obtained by other means (for example
form the motion of the neutron star around a campanion star), one can
mesure the radius of a neutron star in this way.
The gravitational redshift increases to infinity around a
black hole when an object approaches the event horizon of
the black hole which is situated at the so called
Schwarzschild radius. In fact a black hole can best be
defined as an massive compact object surrounded by an area at which the redshift (as observed from a large distance) is infinitly large.
When a star is imploding to form a black hole, one never observes
the star to pass the Schwarzschild radius. As the star approaches this radius it will appear increasingly redder and dimmer in a very short time. In the past such a star was called a frozen star in stead of a black hole. However, in a very short time the collapsing star emits its "last photon" and the object thereafter is black indeed.
The terminology black hole is prefered above frozen star.
In general the gravitational redshift z for a spherical mass M with radius R is given
Corrections for gravitational redshift are nowadays common practise
in many situations. We could almost call it "the applied side of
general relativity". When clocks are in orbit around the Earth
they must be corrected for this effect. This is in partcular
the case with satellite-based navigational systems such as
the Global Positioning System (GPS). To get accuracies of order
10 m, light travel times with an accuracy of order 30 ns (nanoseconds) have
to be measured. Special relativistic time dilatation and gravitational
redshift corrections in these satellites are of order 30000 ns
per day.
See also: redshiftFirst experimental verification
with
the difference between the observed and emitted
wavelength.
z is proportional to the difference in gravitational potential. With the
gravitational acceleration g of the Earth, c the velocity of light and with a height h=22
m, the prediction
was obtained with a 1% accuracy.
Nowadays the accuracy is measured up to 0.02%Gravitational redshift in stars
In which G is the gravitational constant and c is the speed of light.
The coefficient G/c2 = 7.414×10-29cm/g.
For the Sun, M = 2.3×1033g and R = 1.394×1011cm, so Δλ/λ = 1.23×10-6. In other words, each spectral line should be shifted towards the red end of the spectrum by a little over one millionth of its original wavelength. This effect was leasured for the
first time on the Sun in 1962.Black holes have infinite gravitational redshift
(where G is the gravitational constant and c the velocity of light). This formula reduces to the one use for the Sun for large R.
One sees that for r approaching
then .
(The quantity is called the Schwarzschild radius).Gravitational redshift, the applied side of general relativity