Observational Aspects of General Relativity
1.
Slowing Clocks in Gravitational Fields.
Earlier we saw that Einstein's
general theory of relativity predicts that clocks run slower in gravitational
fields (a phenomenon called 'gravitational time dilation') In this case,
for the Earth, one would have the fractional difference in proper time, as a
fraction of time passage t[1]:
Dt/ t » dt2 - dt1/ dt » GM(1/r1 - 1/r2)
Dt/ t » dt2 - dt1/ dt » GM(1/r1 - 1/r2)
where G is the Newtonian gravitational constant, M is the Earth's mass, and g is the acceleration of gravity (g = 980 cm/ sec2 in cgs) and c = 3 x 1010 cm/sec.
In terms of frequency (or clock tick rate) this amounts to a shift in frequency. A large elapsed time (dt2 - dt1) implies a fast tick rate so high frequency. This shows the difference in frequency must be proportional to the elapsed time so:
Dn/ n = (n2 - n1)/ n
= Dt/ t » GM [1/r1 - 1/r2]
Generalizing, any atom placed inside a significant
gravitational potential will display a redshift compared with a similar atom
outside the potential. Thus, inside the potential (at smaller radius r1) the
tick rate slows compared to that measured at radius r2. This means the
frequency is slower or redshifted.
Near to Earth’s surface it is common to
make the approximation:
GM
[1/r1 - 1/r2] »
GM Dr/ R2 = g Dr
Let
us say that in one experiment (r2 - r1) = 0.001 mm = 0.0001cm, then:
Dt/ t ~ (980 cm/s2)(10-4 cm)/ (3 x 1010 cm/sec )2
Dt/ t » 10-22
and for an interval say t = 0.01 sec, Dt =
Dt/ t ~ (980 cm/s2)(10-4 cm)/ (3 x 1010 cm/sec )2
Dt/ t » 10-22
and for an interval say t = 0.01 sec, Dt =
(10-22
)(0.01 sec) = 10-24 sec
2. Deflection of Light in Gravitational Field
The deflection of star light in a gravitational
field was tested during solar eclipse in 1919, and was actually described in
Eddington’s book in detail[2]. A rough illustration of the effect is shown
below:
Fig. 1.
Deflection of star light as predicted by General Relativity
In the diagram the light from the star at actual
position S2 is seen to deflect by some angle a, thereby altering the image position to
that seen at S1. This is a direct result of the effect of the gravitational
field of the Sun on the light rays. The true direction is thus alone the ray
ES2 while the deflected position is along the ray ES1.
Theoretically and quantitatively, one get obtain an estimate of the
magnitude of deflection by incorporating another parameter – call it b – as shown in the diagram below:
Fig. 2:
Determining the linear deflection parameter, b.
Then we obtain for the deflection angle, a:
a = -
4 GM/ b or (in cgs units):
a = - 4 GM/ b c2
Einstein, in his own paper: ‘On the Influence of
Gravitation on the Propagation of Light’, gives the result as:
aq = 2k M/ c2 D
Fig. 3 Diagram for Einstein’s derivation of a (
Here k = G, the
gravitational constant and D = the distance of the ray from the center of the
body. It is obtained from the diagram of Fig. 2.
Einstein used the cosine
of the angle and integrated from the negative angle
q = - p/ 2 to q = p/ 2:
a = 1/ c2
ò - p/ 2 p/ 2 k M/ r2 cos q ds
3. Advance of Mercury’s Perihelion
Another prediction from General Relativity is the
advance of Mercury’s perihelion. This is a phenomenon in no way predictable
from Newtonian gravitation and is illustrated below, with the orbits separated
in exaggerated fashion:
Fig. 4. Advance of Mercury’s Perihelion
The
amount of rotation of 'the planetary ellipse' due to the effects of gravitation
in general relativity was set out in the following equation of Einstein’s:
e
= [24 (p)3 a2]/
T2 c2 [1 - e2]
where e is the advance (or rotation) in seconds of arc, T is the period of revolution in seconds, c the velocity of light and e the eccentricity of the orbit.
Einstein, on page 164 of the same paper, asserts that for Mercury e= 43 seconds per century
where e is the advance (or rotation) in seconds of arc, T is the period of revolution in seconds, c the velocity of light and e the eccentricity of the orbit.
Einstein, on page 164 of the same paper, asserts that for Mercury e= 43 seconds per century
Problem: Validate the magnitude
of the perihelion advance of Mercury from Einstein’s given equation.
The
key to the solution is to note that Einstein framed his equation in cgs units,
so we must have:
c
= 3 x 1010 cm/s
a
= (1.5 x 1013 cm) (0.387) =
5.8 x 1012 cm
Based
on using 1 astronomical unit (AU) = 1.5 x 1013 cm. But from a Table
of distances, Mercury's semi-major axis a = 0.387 AU.
The
period, T (in seconds) is just the length of Mercury's year (in days = 87.96,
again from a Table ) multiplied by the seconds-length of an Earth day, or
86,400 s:
T = 7.6 x 106 s
T = 7.6 x 106 s
The
eccentricity, e from a similar Table is e = 0.205.
Substituting all these values into the given equation yields:
e = 5.036 x 10-7 radian
To get the equivalent seconds of arc (or arcsec) we use 1 rad (radian) = 57.3 degree where one degree has 3600 seconds. Thus, 1 radian will have:
2.063 x 105 arcsec
So, the associated arcsec for e will be:
(5.036 x 10- 7 rad) x (2.063 x 105 arcsec/ rad) =
0.104 arcsec
Substituting all these values into the given equation yields:
e = 5.036 x 10-7 radian
To get the equivalent seconds of arc (or arcsec) we use 1 rad (radian) = 57.3 degree where one degree has 3600 seconds. Thus, 1 radian will have:
2.063 x 105 arcsec
So, the associated arcsec for e will be:
(5.036 x 10- 7 rad) x (2.063 x 105 arcsec/ rad) =
0.104 arcsec
We
are still not finished because the quantity is defined per century.
At this point, you need to recall the PERIOD of Mercury is 0.2405 YRS.
So, the number of arcsec of perihelion advance per Earth years is:
0.104 arcsec/ 0.2405 years = 0.432
At this point, you need to recall the PERIOD of Mercury is 0.2405 YRS.
So, the number of arcsec of perihelion advance per Earth years is:
0.104 arcsec/ 0.2405 years = 0.432
Or
43 seconds of arc per century.
Other Problems:
1) The
tick rate of a clock is found to slow from 10-24 sec to 10-10 sec when placed
inside a strong gravity well. Find the amount by which the frequency is
redshifted.
2) Using
Einstein’s relation for the deflection of starlight in a strong gravitational
field:
a = ò - p/ 2 p/ 2 k M/ r2 cos q ds
Show that this would actually be equal to: a = 2 F/ c2
(Where
F is the gravitational
potential.)
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