162 Chapter 4
If we let f
2
= 0, h denote the height up to f
1
, and g denote the gravitational accelera-
tion near the ground and then substitute f
1
= gh and f
2
= 0 into equation {, we obtain the
following:
The clock at the higher altitude measures a time Dt
1
that is ahead of the clock below,
which reads Dt
2
. We know this to be true, because in the equation above, gh/c
2
and Dt
1
are both greater than zero, and therefore ; hence, .
The True Nature of Gravity in General Relativity
Space-time surrounding the existence of matter is warped, as explained in the manga. It is
apparent that this warping of space-time has the same effect as gravity in attracting sur-
rounding matter.
Einstein unified these effects in a set of equations called the Einstein field equations.
The Einstein field equations showed that time and space (space-time), which were previously
thought to exist as a framework for measuring the motion of matter, were fundamentally
connected with matter itself.
Phenomena Discovered from General Relativity
This section introduces the following phenomena, which were discovered from general
relativity:
Gravitational lensing
Anomalous perihelion precession of Mercury
Black holes
Bending of Light (Gravitational Lensing) Near a Large
Mass (Such as the Sun)
Gravitational lensing is the phenomenon that when light passes in the vicinity of the Sun,
the path of that light bends.
Space is bent in the vicinity of the Sun because of the large mass of the Sun, as shown
in Figure 4-4. Since light advances along that curvature, the light from a distant star bends,
and the direction of the star is observed with a slight shift. This effect was verified during a
total solar eclipse. It is noted as the first proof discovered of general relativity.
Also, when light is coming from a distant galaxy, as shown in Figure 4-5, if a massive
object (such as a galaxy) lies at an intermediate point, it will bend the light from the distant
galaxy as though there were a condensing lens at that intermediate point. This bend may
make the distant galaxy seem distorted. Many instances of this effect have been observed.
This is another instance of gravitational lensing.
τ τ
τ
φ φ
1 2
1
1 2
2 2 2
0
=
=
c
gh
c
gh
c
τ τ
1 2
0 >
τ τ
1 2
>
RELATIVITY_03.indb 162 3/15/2011 3:28:15 PM
What Is General Relativity? 163
Earth
Actual direction of star
Apparent star
(The star appears in
this direction since
its light is bent.)
Sun
Figure 4-4: Bending of light near a large mass
Figure 4-5: Gravitational lensing
Light from the distant galaxy is
bent by an object with a large
mass, as if a condensing lens
were there.
Earth
RELATIVITY_03.indb 163 3/15/2011 3:28:15 PM

Get The Manga Guide to Relativity now with O’Reilly online learning.

O’Reilly members experience live online training, plus books, videos, and digital content from 200+ publishers.