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5.7 Weak Field Limit of Einstein Equations

225

 

0 0

0

· · ·

· · ·

 

· · ·

 

 

 

0

 

 

 

 

 

0 0

0

· · ·

· · ·

 

· · ·

 

 

 

0

 

 

 

 

 

 

 

0 0

γ

33

γ

34

 

 

γ

3,m

1

 

γ

3,m

 

 

 

 

 

 

 

· · ·

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

μν

. .

.

 

.

· .

 

 

.

 

 

 

.

 

 

 

 

γ phys

0 0

γ43

γ44

· ·

γ4,m

1

 

γ4,m

 

 

(5.7.25)

 

= . .

. . .

 

 

.

 

 

 

.

 

 

 

 

 

. .

. . .

 

 

.

 

 

 

.

 

 

 

 

 

. .

. . .

 

 

.

 

 

 

.

 

 

 

 

 

. .

. . .

 

 

.

 

 

 

.

 

 

 

 

 

. .

. . .

 

 

.

 

 

 

.

 

 

 

 

 

 

γ

 

γ

 

 

 

γ

 

 

 

m

1

γ

 

 

 

0 0

· · ·

 

 

 

 

 

 

 

 

 

m3

m4

m,m1

i=3

 

ii

 

The number of these degrees of freedom is easily calculated it is:

 

 

 

 

 

 

 

 

=

 

2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

#d.o.f

 

m(m 3)

 

 

 

 

 

 

 

(5.7.26)

 

 

 

 

 

 

 

 

 

 

 

 

 

In D = 4 space-time dimensions the degrees of freedom are 2 and the corresponding gauge fixed form of the γμν tensor is the following one:

 

 

 

 

0

0

0

 

0

 

 

γμνphys

=

(u)

 

0

0

0

 

0

 

(5.7.27)

0

0

a(u)

b(u)

 

 

=

 

 

 

 

 

 

 

 

 

 

 

0

0

b(u)

a(u)

 

 

 

 

 

 

 

 

 

 

 

where the two functions a(u) and b(u) are arbitrary. We shall use this gauge-fixed form of the metric perturbation while studying the emission and propagation of gravitational waves (see Chap. 7 of this volume).

5.7.2 The Spin of the Graviton

Hence the gravitational waves, namely the small deformations of the Minkowski metric, propagate in Minkowski space-time and propagate at the speed of light since they obey the d’Alembertian equation. Moreover they are transverse waves since what varies in time along the line of flight is not the amplitude of the metric coefficient in that direction, rather all the metric coefficients in the space orthogonal to the line.

From the mathematical point of view the right way to approach this issue is from the point of view of the little group of invariance of the momentum vector. A planewave gravitational disturbance, like an electromagnetic one of the same type, is an object carrying momentum and this momentum is a light-like vector:

p(μwave) = :1, 1, 0, 0, · · · , 0;

(5.7.28)

m2

The little group of invariance of any element v D belonging to the carrier vector space of a linear representation of some Lie group G is that subgroup G (v) G which leaves the vector v invariant:

226

Table 5.1 Degrees of freedom of the graviton in diverse dimensions

 

5 Einstein Versus Yang-Mills Field Equations

D

Little group

# of d.o.f.

11

SO(9)

44

10

SO(8)

35

9

SO(7)

27

8

SO(6)

20

7

SO(5)

14

6

SO(4)

9

5

SO(3)

5

4

SO(2)

2

3

0

g G (v) : g · v = v

(5.7.29)

Typically the carrier space D is organized in orbits, under the action of G, whose little groups are different non-isomorphic subgroups of the G. In the case of the Lorentz group SO(1, m 1) and its fundamental m-dimensional representation the relevant orbits are three corresponding to the time-like, space-like and null-like vectors. The corresponding little groups are Gtime = SO(m), Gspace = SO(1, m 1) and Gnull = SO(m 2). Therefore the degrees of freedom of the graviton correspond to the following irreducible representation of the little group SO(m 2):

graviton

 

 

 

(5.7.30)

 

 

where the hat denotes the traceless nature of the symmetric tensor. The number of

independent components of such an irreducible representation is the number m(m3)

2

quoted above. Given its relevance in modern multi-dimensional gravity theories and specifically in supergravities that are the low energy limits of superstring models, in Table 5.1 we list the number of graviton degrees of freedom for all space-time dimensions between D = 11 and D = 3.

In D = 3 the graviton disappears. There is no room for its propagation since there is no residual transverse group. Gravity in three space-time dimension allows only for the Newtonian potential and there are no local propagating degrees of freedom. In D = 4 the transverse group is SO(2), whose unitary irreducible representations are all two-dimensional, as we explained in Sect. 1.6.1. For this reason the graviton has the same number of degrees of freedom as the photon or a Yang-Mills gauge boson, namely 2. Yet although all two-dimensional, the irreducible representations of SO(2) are not all equivalent. According to the discussion of Sect. 1.6.1 they are characterized by an half integer number s that we name the spin of the corresponding particle. In the case of the graviton, just as for the photon, s is integer, but it is s = 2 rather than s = 1. Physically this means that we have two states, one of helicity s = 2 and one of helicity s = −2. The two states are pictorially described in Fig. 5.5.

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