What is the Unit of the Metric Tensor?

Click For Summary
The discussion centers on the units of the metric tensor in relation to the cosmological constant and Einstein's field equations. It asserts that the metric tensor has no units, as its components must align dimensionally with the distance formula. The conversation also highlights the importance of the metric in general relativity, which describes the geometry of spacetime and its curvature. Additionally, it touches on the stress-energy tensor, emphasizing its role in representing momentum flow in spacetime. Understanding these concepts is crucial for grasping the fundamentals of general relativity.
Antonio Lao
Messages
1,436
Reaction score
1
If the cosmological constant, \Lambda has units of reciprocal time squared then what is the unit for the metric tensor, g_{ij}?
 
Physics news on Phys.org
It has no units. A metric tensor in any coordinate can have no units, just look at how the components of a diagonal metric tensor fits into the distance formula, if it had units the units on the left would not match the units on teh right.
 
franznietzsche,

Thanks. But I'm still not clear why the righthand side of Einstein's field equations, the momentum-energy tensor has components of different units (units in pressures, and units in densities).
 
Antonio Lao said:
I'm still not clear why the righthand side of Einstein's field equations, the momentum-energy tensor has components of different units (units in pressures, and units in densities).

Here is an excellent GR tutorial:

http://math.ucr.edu/home/baez/gr/outline2.html


The METRIC is the star of general relativity. It describes everything about the geometry of spacetime, since it let's us measure angles and distances. Einstein's equation describes how the flow of energy and momentum through spacetime affects the metric. What it affects is something about the metric called the "curvature". The biggest job in learning general relativity is learning to understand curvature!

Mathematically, the metric g is a tensor of rank (0,2). It eats two tangent vectors v,w and spits out a number g(v,w), which we think of as the "dot product" or "inner product" of the vectors v and w. This let's us compute the length of any tangent vector, or the angle between two tangent vectors. Since we are talking about spacetime, the metric need not satisfy g(v,v) > 0 for all nonzero v. A vector v is SPACELIKE if g(v,v) > 0, TIMELIKE if g(v,v) < 0, and LIGHTLIKE if g(v,v) = 0.


The STRESS-ENERGY TENSOR. The stress-energy is what appears on the right side of Einstein's equation. It is a tensor of rank (0,2), and it defined as follows: given any two tangent vectors u and v at a point p, the number T(u,v) says how much momentum in the u direction is flowing through the point p in the v direction. Writing it out in terms of components in any coordinates, we have

T(u,v) = T_ab u^a v^b
 
Russell,

Thanks. Will start studying this GR tutorial.
 
I do not have a good working knowledge of physics yet. I tried to piece this together but after researching this, I couldn’t figure out the correct laws of physics to combine to develop a formula to answer this question. Ex. 1 - A moving object impacts a static object at a constant velocity. Ex. 2 - A moving object impacts a static object at the same velocity but is accelerating at the moment of impact. Assuming the mass of the objects is the same and the velocity at the moment of impact...

Similar threads

  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 21 ·
Replies
21
Views
3K
  • · Replies 11 ·
Replies
11
Views
3K
  • · Replies 6 ·
Replies
6
Views
832
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 1 ·
Replies
1
Views
978
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 10 ·
Replies
10
Views
1K
Replies
19
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K