Energy Momentum Tensor - EM - Derivative

In summary: Yes, I was thinking of it as acting only on ##u_{b}##.Later you do ##\nabla^{a}(\rho u_{a}) = 0##, where you pull in ##\rho##.When can you do that, and when is it not allowed?You can always do that, since ##\nabla_{a}## is a derivative operator. You just use the product rule.If ##\rho## is just a scalar, you can pull it in, because
  • #1
ProfDawgstein
80
1
I have a short question about the derivative of a given EM-Tensor.

##\rho## = mass density
##U^\mu## = 4 velocity

##T^{\mu\nu} = \rho U^\mu U^\nu##

Now I do ##\partial_\mu##

Should I get

a) ##\partial_\mu T^{\mu\nu} = (\partial_\mu \rho) (U^\mu U^\nu) + \rho (\partial_\mu U^\mu) U^\nu + \rho U^\mu (\partial_\mu U^\nu)##

b) ##\partial_\mu T^{\mu\nu} = (\partial_\mu \rho) (U^\mu U^\nu) + \rho (\partial_\mu U^\mu) U^\nu##

This should be the product rule, right?
So I should get 3 terms?

##(\partial_\mu \rho) (U^\mu U^\nu) = 0##

because

##(\rho \partial_\mu U^\mu) = 0## (mass conservation)

Solution is

##\partial_\mu T^{\mu\nu} = \rho (U^\mu \partial_\mu) U^\nu##

where ##\partial_\mu (\rho U^\mu) = 0##

What am I missing?
 
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  • #2
ProfDawgstein said:
This should be the product rule, right?
So I should get 3 terms?

a) looks correct, all 3 terms should be there.

ProfDawgstein said:
##(\partial_\mu \rho) (U^\mu U^\nu) = 0##

because

##(\rho \partial_\mu U^\mu) = 0## (mass conservation)

No, this is not correct. Local conservation of energy is

$$
\partial_{\mu} T^{\mu \nu} = 0
$$

(Note, btw, that that only holds in flat spacetime; in curved spacetime local energy conservation is ##\nabla_{\mu} T^{\mu \nu} = 0##.)
 
  • #3
PeterDonis said:
a) looks correct, all 3 terms should be there.

No, this is not correct. Local conservation of energy is

$$
\partial_{\mu} T^{\mu \nu} = 0
$$

(Note, btw, that that only holds in flat spacetime; in curved spacetime local energy conservation is ##\nabla_{\mu} T^{\mu \nu} = 0##.)

I should have added that this is:
-special relativity
-comoving frame

I just want to know how to get from

##\partial_\mu T^{\mu\nu} = (\partial_\mu \rho) (U^\mu U^\nu) + \rho (\partial_\mu U^\mu) U^\nu + \rho U^\mu (\partial_\mu U^\nu)##

to

##\partial_\mu T^{\mu\nu} = \rho (U^\mu \partial_\mu) U^\nu##

Cheng used

(mass conservation) ##\partial_\mu (\rho U^\mu) = 0##

(comoving) ##U^\mu = \gamma (c, 0, 0, 0)##

##U^\mu \partial_\mu = \gamma \partial_t = \partial_\tau##

##\rho \partial_\tau U^\nu## is the 4 force density

This is for a system of EM field and charges.

So this really is ##T^{\mu\nu}_{charge}##
 
  • #4
ProfDawgstein said:
I should have added that this is:
-special relativity
-comoving frame

Ok, good.

ProfDawgstein said:
I just want to know how to get from

##\partial_\mu T^{\mu\nu} = (\partial_\mu \rho) (U^\mu U^\nu) + \rho (\partial_\mu U^\mu) U^\nu + \rho U^\mu (\partial_\mu U^\nu)##

to

##\partial_\mu T^{\mu\nu} = \rho (U^\mu \partial_\mu) U^\nu##

You mention "Cheng"; can you give a more specific reference? Several things that you quote in what follows don't look right to me, but I can't tell for sure without seeing the context.
 
  • #5
PeterDonis said:
Ok, good.

You mention "Cheng"; can you give a more specific reference? Several things that you quote in what follows don't look right to me, but I can't tell for sure without seeing the context.

https://www.amazon.com/dp/0199573646/?tag=pfamazon01-20

page 399 - 12.15 - visible on book preview

EDIT:

I think ##j^\mu = \rho U^\mu## can be considered to be the 'mass current'.

##\partial_\mu j^\mu = 0## leads to mass conservation.

Which is the same as ##\partial_\mu (\rho U^\mu) = 0##.
 
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  • #6
ProfDawgstein said:
I think ##j^\mu = \rho U^\mu## can be considered to be the 'mass current'.

Where are you getting that from? Cheng uses ##j^{\mu}## to represent the charge-current density 4-vector, which is not the same as mass current. So ##\partial_{\mu} j^{\mu} = 0## represents charge conservation, not mass conservation.

After looking at the page you referenced, I'm still not sure I understand Cheng's notation. I need to look at this some more.
 
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  • #7
PeterDonis said:
Where are you getting that from? Cheng uses ##j^{\mu}## to represent the charge-current density 4-vector, which is not the same as mass current. So ##\partial_{\mu} j^{\mu} = 0## represents charge conservation, not mass conservation.

After looking at the page you referenced, I'm still not sure I understand Cheng's notation. I need to look at this some more.

I just used ##j^\mu## to illustrate that mass density equation.

Bad choice of letter...

First he does mass, and then he switches to charge/current (charge per mass).
 
  • #8
ProfDawgstein said:
First he does mass, and then he switches to charge/current (charge per mass).

Yes, I see that, but I can't see the actual page where the problem is posed in the book preview (the page you referenced is where the solution is given), so I'm not sure how much headway I'm going to make in understanding his notation.
 
  • #9
Consider ##T_{ab} = (\rho + p)u_{a}u_{b} + g_{ab}p##. I will prove something just a bit more general that holds for fluids with non-vanishing pressure. Now ##\nabla^{a}T_{ab} = 0 \Rightarrow (\rho + p)u_{a}\nabla^{a}u_{b} + (\rho + p)u_{b}\nabla^{a}u_{a} + u_{a}u_{b}\nabla^{a}(\rho + p) + \nabla_{b}p##
so contracting with ##u^{b}## and using the fact that ##u^{b}\nabla^{a}u_{b} = 0## we find that ##(\rho + p)\nabla^{a}u_{a} + u_{a}\nabla^{a}\rho = 0##. In your case we have a pressureless fluid so we get ##\nabla^{a}(\rho u_{a}) = 0##. Hence ##\nabla^{a}T_{ab} = \rho u_{a}\nabla^{a}u_{b} ##. Note that this works for any space-time ##(M,g_{ab})## and metric compatible derivative operator ##\nabla_{a}##.

EDIT: As Peter remarked, ##\nabla^{a}T_{ab} = 0## and ##\nabla^{a}j_{a} = 0## are different physical conditions; the latter is a simple consequence of Maxwell's equations ##\nabla^{a}F_{ab} = j_{b} ## and ##\nabla_{[a}F_{bc]} = 0##. As an aside, if ##T_{ab}## is the energy momentum tensor for the electromagnetic field in particular then what one can show is that ##\nabla^{a}T_{ab} = j^{a}F_{ab}## (proof on request).
 
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  • #10
WannabeNewton said:
##\nabla^{a}T_{ab} = 0 \Rightarrow (\rho + p)u_{a}\nabla^{a}u_{b} + (\rho + p)u_{b}\nabla^{a}u_{a} + u_{a}u_{b}\nabla^{a}(\rho + p) + \nabla_{b}p##

without pressure (p = 0)

##\nabla^{a} T_{ab} = \rho u_a (\nabla^{a} u_b) + \rho u_b (\nabla^{a} u_a) + u_a u_b (\nabla^{a} \rho)##

1st term: ##\rho u_a (\nabla^{a} u_b)## where ##\nabla^{a}## applies only to ##u_b## ?

Later you do ##\nabla^{a}(\rho u_{a}) = 0##, where you pull in ##\rho##.

When can you do that, and when is it not allowed?

If ##\rho## is just a scalar, you can pull it in, because of the linearity of ##\nabla^{a}##.

Why do you contract with ##u^{b}## ?

How do we know that ##u^{b}\nabla^{a}u_{b} = 0##?

Slightly confused here, or just too much of it...
 
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  • #11
Ok so ##\nabla^{a}T_{ab} = \rho u_{a}\nabla^{a}u_{b} + \rho u_{b}\nabla^{a}u_{a}+ u_{a}u_{b}\nabla^{a}\rho = 0 ##. Yes ##\nabla^{a}## is only being applied to ##u_{b}## in the first term. ##u^{b}u_{b} = -1## by definition which immediately implies that ##u^{b}\nabla^{a}u_{b} = 0##; contracting both sides of ##\nabla^{a}T_{ab} = 0## with ##u^b## will then simplify the expression down to ##\rho\nabla^{a}u_{a}+ u_{a}\nabla^{a}\rho = \nabla^{a}(\rho u_{a}) = 0##. All I did in that last step was use the Leibniz (product) rule for ##\nabla_{a}##.
 
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  • #12
WannabeNewton said:
Ok so ##\nabla^{a}T_{ab} = \rho u_{a}\nabla^{a}u_{b} + \rho u_{b}\nabla^{a}u_{a}+ u_{a}u_{b}\nabla^{a}\rho = 0 ##. Yes ##\nabla^{a}## is only being applied to ##u_{b}## in the first term. ##u^{b}u_{b} = -1## by definition which immediately implies that ##u^{b}\nabla^{a}u_{b} = 0##; contracting with ##u^b## will then allow us to simplify the expression down to ##\rho\nabla^{a}u_{a}+ u_{a}\nabla^{a}\rho = \nabla^{a}(\rho u_{a}) = 0##. All I did in that last step was use the Leibniz (product) rule for ##\nabla_{a}##.

now contract with ##u^{b}##

##\nabla^{a}T_{ab} = \rho u_{a} (\nabla^{a} u^{b} u_{b}) + \rho u^{b} u_{b}\nabla^{a}u_{a}+ u_{a}u_{b} u^{b} \nabla^{a}\rho = 0##

##\nabla^{a}T_{ab} = \rho u_{a} (\nabla^{a} [-1]) + \rho u^{b} u_{b}\nabla^{a}u_{a}+ u_{a}u_{b} u^{b} \nabla^{a}\rho = 0##

##\nabla^{a}T_{ab} = 0 + \rho [-1]\nabla^{a}u_{a}+ u_{a} [-1] \nabla^{a}\rho = 0##

##\nabla^{a}T_{ab} = -2 \rho \nabla^{a}u_{a} = 0##

##\nabla^{a}T_{ab} = \nabla^{a} \rho u_{a} = 0## (scalar / linearity)

did I insert the ##u^{b}## correctly?

what if ##\rho = \rho(x)## ?
 
  • #13
No the first term vanishes because it contains ##u^{b}\nabla^{a}u_{b}## which is zero because ##\nabla^{a}(u^b u_b) = 2u^b\nabla^a u_b = \nabla^a(-1) = 0##. You can't pull the ##u^b## into the derivative like that. Also, ##\rho## is not a constant. What you have in the end is ##u^a\nabla_a \rho + \rho\nabla^a u_a = 0##. This becomes ##\nabla^a (\rho u_a) = 0## because of the usual product rule from calculus.
 
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  • #14
WannabeNewton said:
No the first term vanishes because it contains ##u^{b}\nabla^{a}u_{b}## which is zero because ##\nabla^{a}(u^b u_b) = 2u^b\nabla^a u_b = \nabla^a(-1) = 0##. You can't pull the ##u^b## into the derivative like that. Also, ##\rho## is not a constant. What you have in the end is ##u^a\nabla_a \rho + \rho\nabla^a u_a = 0##. This becomes ##\nabla^a (\rho u_a) = 0## because of the usual product rule from calculus.

So we have

##\rho = \rho(x^\mu)## mass density varies from point to point

##u_a = u_a(x^\mu)## velocity of particle different from point to point

##X_a = X_a(x^\mu) = \rho u_a = \rho(x^\mu) u_a(x^\mu)## can be considered 'mass current/flow', which also depends on position

We start with this

##\nabla^{a} T_{ab} = \rho u_a (\nabla^{a} u_b) + \rho u_b (\nabla^{a} u_a) + u_a u_b (\nabla^{a} \rho)##

then we contract with ##u^{b}##

##\nabla^{a} T_{ab} = \rho u_a u^{b} (\nabla^{a} u_b) + \rho u_b u^{b} (\nabla^{a} u_a) + u_a u_b u^{b} (\nabla^{a} \rho)##

because ##u_b u^{b} = -1## we get

##\nabla^{a} T_{ab} = \rho u_a u^{b} (\nabla^{a} u_b) + \rho [-1] (\nabla^{a} u_a) + u_a [-1] (\nabla^{a} \rho)##

then

##\nabla^{a} T_{ab} = \rho u_a u^{b} (\nabla^{a} u_b) - \rho (\nabla^{a} u_a) - u_a (\nabla^{a} \rho)##

seeing that the last two terms are ##- \nabla^{a} (\rho u_a)##

##\nabla^{a} T_{ab} = \rho u_a u^{b} (\nabla^{a} u_b) - \nabla^{a} (\rho u_a)##

the last term now is equal to ##X_a##, our 'mass current/flow' which is conserved, so ##\nabla^{a} (\rho u_a) = 0##

now we have

##\nabla^{a} T_{ab} = \rho u_a u^{b} (\nabla^{a} u_b)##

now ##\nabla^{a}(u^b u_b) = 2u^b\nabla^a u_b = \nabla^a(-1) = 0##

which means that ##\nabla^{a} T_{ab} = \rho u_a [u^{b} (\nabla^{a} u_b)] = 0##

so

##\nabla^{a} T_{ab} = 0##

BUT Cheng gets

##\partial_\mu T^{\mu\nu} = \rho (U^\mu \partial_\mu) U^\nu##

which should be the same as

##\nabla_\mu T^{\mu\nu} = \rho (U^\mu \nabla_\mu) U^\nu##

am I blind? :P
 
  • #15
WannabeNewton said:
Now ##\nabla^{a}T_{ab} = 0 \Rightarrow (\rho + p)u_{a}\nabla^{a}u_{b} + (\rho + p)u_{b}\nabla^{a}u_{a} + u_{a}u_{b}\nabla^{a}(\rho + p) + \nabla_{b}p##

Shouldn't there be a ##\nabla_b \rho## term as well?
 
  • #16
If it holds for any arbitrary metric compatible derivative operator ##\nabla_{a}## then it also holds for ##\partial_{a}##.
 
  • #17
PeterDonis said:
Shouldn't there be a ##\nabla_b \rho## term as well?
I can't see there being a ##\nabla_{b}\rho## term myself. The ##\nabla_{b}p## term comes from ##\nabla^{a}(g_{ab} p) = \nabla_{b}p##.
 
  • #18
WannabeNewton said:
I can't see there being a ##\nabla_{b}\rho## term myself. The ##\nabla_{b}p## term comes from ##\nabla^{a}(g_{ab} p) = \nabla_{b}p##.

Ah, sorry, I forgot about that term in the original ##T_{ab}##. Move along, nothing to see here. :redface:
 
  • #19
WannabeNewton said:
If it holds for any arbitrary metric compatible derivative operator ##\nabla_{a}## then it also holds for ##\partial_{a}##.

so my calculation (post #14) should be 100% correct?

Do not forget that

##T_{ab} = \rho u_a u_b##

where

##T_{ab} = T_{ab}^{charge}## (see post #1) EDIT: #3

there is also

##T_{ab}^{field}##

in the end

##\partial_\mu T^{\mu\nu} = \partial_\mu (T^{\mu\nu}_{field} + T^{\mu\nu}_{charge}) = 0##

I have no idea why you get ##\nabla^{a} T_{ab} = 0## and Cheng

##\partial_\mu T^{\mu\nu}_{field} = - \frac{1}{c} F^{\nu\lambda} j_\lambda##

##\partial_\mu T^{\mu\nu}_{charge} = \frac{1}{c} F^{\nu\lambda} j_\lambda##


basically it's all about

I just want to know how to get from

##\partial_\mu T^{\mu\nu} = (\partial_\mu \rho) (U^\mu U^\nu) + \rho (\partial_\mu U^\mu) U^\nu + \rho U^\mu (\partial_\mu U^\nu)##

to

##\partial_\mu T^{\mu\nu} = \rho (U^\mu \partial_\mu) U^\nu##

I think I just lost the feeling for UP/DOWN :confused:

the original equation

##\nabla^{a} T_{ab} = \rho u_a (\nabla^{a} u_b) + \rho u_b (\nabla^{a} u_a) + u_a u_b (\nabla^{a} \rho)##

Cheng: ##\partial_\mu T^{\mu\nu}_{charge} = \rho (U^\mu \partial_\mu) U^\nu##

written another way

##\nabla^{a} T_{ab}^{charge} = \rho (\nabla^{a} U_a) U_b##

which means that

##\rho U_a (\nabla^{a} U_b) + U_a U_b (\nabla^{a} \rho) = 0## (they cancel)

if we contract that one with ##U^{b}## we get

##\rho U_a U^{b} (\nabla^{a} U_b) + U_a U_b U^{b} (\nabla^{a} \rho)##

and we use ##U_b U^{b} = -1##

##\rho U_a U^{b} (\nabla^{a} U_b) + U_a [-1] (\nabla^{a} \rho)##

so

##\rho U_a U^{b} (\nabla^{a} U_b) - U_a (\nabla^{a} \rho)##

according to WBN the 1st term equals zero, then we have

##U_a (\nabla^{a} \rho) = 0##

which is getting even more confusing...

WannabeNewton said:
(proof on request)

maybe this will make things clear...

Thanks everybody until now
 
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  • #20
Can you give the exact page in Cheng where the problem statement is given in detail? Your original post didn't include anything about the energy-momentum tensor of an electromagnetic field, it only talked about the energy-momentum tensor of dust so that's what I thought you were exclusively talking about. If the only energy-momentum is coming from dust i.e. ##T_{ab} = \rho u_{a}u_{b}## then using ##\nabla^a T_{ab} = 0## one can show that ##\nabla^a (\rho u_a) = 0## as I have previously done in this thread. From this we see that ##\nabla^a T_{ab} = u_b\nabla^a(\rho u_a) + \rho u_a \nabla^a u_b = \rho u_a \nabla^a u_b = 0## i.e. ##u^a \nabla_a u^b = 0## which is just the statement that dust particles travel on geodesics, given the above conditions.
 
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  • #21
Ok so I read the section from Cheng. He is not talking about a normal charge-free dust field (your original post made it seem like he was) but rather about a charged dust field in which case we have two separate energy-momentum sources ##T^{ab}_{\text{EM}}## and ##T^{ab}_{\text{charges}} = \rho u^a u^b## where ##\rho## is the mass-density of the charged dust field i.e. we have both the energy-momentum of the charged particles and the energy-momentum of the electromagnetic fields that they carry. What he should have mentioned is that the charge density ##\sigma## of the dust field is as measured by observers comoving with the dust hence ##j^{a} = \sigma u^{a}##.

If we assume that ##\nabla_a (\rho u^a) = 0## then we have ##\nabla_a T^{ab} = 0## (proof below). So clearly Cheng is assuming that ##\nabla_a (\rho u^a) = 0## i.e. he is assuming that conservation of mass for the dust still holds even when the dust particles are interacting with an electromagnetic field. I can't really see why this would be justified. Hopefully someone else can explain why we can still assume this.

As for the proof of ##\nabla_a T^{ab} = 0## assuming that ##\nabla_{a}(\rho u^{a}) =0 ##, first we write the total energy-momentum tensor as ##T^{ab} = T^{ab}_{\text{EM}} + T^{ab}_{\text{charges}} = F^{ac}F^{b}{}{}_{c}-\frac{1}{4}g^{ab}F^{cd}F_{cd} + \rho u^{a}u^{b}##.

Now, note that ##\nabla_{a}T^{ab}_{\text{EM}} = F_{ac}\nabla^{a}F^{bc} - F^{b}{}{}_{c}j^{c}-\frac{1}{2}F_{cd}\nabla^{b}F^{cd}\\ = F_{ac}\nabla^{a}F^{bc} - F^{b}{}{}_{c}j^{c}-\frac{1}{2}F_{cd}\nabla^{c}F^{bd} + \frac{1}{2}F_{cd}\nabla^{d}F^{bc} \\= F_{cd}\nabla^{c}F^{bd} - F^{b}{}{}_{c}j^{c}-\frac{1}{2}F_{cd}\nabla^{c}F^{bd} - \frac{1}{2}F_{cd}\nabla^{c}F^{bd} = -F^{bc}j_{c}##
where ##\nabla^{[a}F^{bc]} = 0## was used.

Since ##j_{c} = \sigma u_{c}## we have ##\nabla_a T^{ab} = -\sigma u_{a}F^{ba} + \rho u^{a}\nabla_{a}u^{b} + u^{b}\nabla_{a}(\rho u^{a}) = 0## because the charged dust field satisfies the equations of motion ##\rho u^a \nabla_a u^b = \sigma u_a F^{ba}##.
 
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  • #22
WannabeNewton said:
Can you give the exact page in Cheng where the problem statement is given in detail?

I will post it here for future reference...

Cheng said:
problem 12.15

"##T^{\mu\nu}##for a system of EM fields and charges Because fields and particles can exchange energy and momenta between them, energy and momentum are conserved only for the combined system. Show that neither ##T^{\mu\nu}_{field}## of (12.80) nor ##T^{\mu\nu}_{charge}## of (12.83) is conserved, but their divergences mutually cancel so that ##\partial_\mu T^{\mu\nu} = 0##. Thus, for the system as a whole, energy and momentum are conserved."

equation 12.80

##T^{\mu\nu}_{field} = \frac{1}{2} \eta_{\alpha\beta} \left( F^{\mu\alpha} F^{\nu\beta} + \widetilde{F}^{\mu\alpha} \widetilde{F}^{\nu\beta} \right) = \eta_{\alpha\beta} F^{\mu\alpha} F^{\nu\beta} - \frac{1}{4} \eta^{\mu\nu} F^{\alpha\beta} F_{\alpha\beta}##

equation 12.83

##T^{\mu\nu} = T^{\mu\nu}_{field} + T^{\mu\nu}_{charge}##

where ##T^{\mu\nu}_{charge} = \rho'_{mass} U^\mu U^\nu## with ##\rho'_{mass}## being the proper mass density of the charged particles.

WannabeNewton said:
What he should have mentioned is that the charge density σ of the dust field is as measured by observers comoving with the dust hence ja=σua.

yes, he sometimes seems to "forget" things like that...

WannabeNewton said:
I can't really see why this would be justified.

Happened to me at least a few times in the previous 320 pages.

WannabeNewton said:
##\nabla_{a}T^{ab}_{\text{EM}} = F_{ac}\nabla^{a}F^{bc} - F^{b}{}{}_{c}j^{c}-\frac{1}{2}F_{cd}\nabla^{b}F^{cd}\\ = F_{ac}\nabla^{a}F^{bc} - F^{b}{}{}_{c}j^{c}-\frac{1}{2}F_{cd}\nabla^{c}F^{bd} + \frac{1}{2}F_{cd}\nabla^{d}F^{bc} \\= F_{cd}\nabla^{c}F^{bd} - F^{b}{}{}_{c}j^{c}-\frac{1}{2}F_{cd}\nabla^{c}F^{bd} - \frac{1}{2}F_{cd}\nabla^{c}F^{bd} = -F^{bc}j_{c}##

Thanks. This makes sense to me.

WannabeNewton said:
Can you give the exact page in Cheng where the problem statement is given in detail?

Sorry everybody, I wanted to post it today, I should have done it in post #1. My bad :redface:

WannabeNewton said:
conservation of mass for the dust still holds even when the dust particles are interacting with an electromagnetic field.

the EM field does only change their direction of motion, but does not change their mass?
so mass should be conserved?

Thank you again, and sorry for causing the confusion :frown:
 

1. What is the Energy Momentum Tensor?

The Energy Momentum Tensor (EM tensor) is a mathematical quantity that describes the distribution of energy and momentum in a given system. It is a symmetric tensor of rank 2 and contains 10 components.

2. How is the EM tensor calculated?

The EM tensor is calculated by taking the derivative of the Lagrangian density with respect to the metric tensor. The Lagrangian density is a mathematical function that describes the dynamics of a system and the metric tensor is a mathematical object that describes the geometry of spacetime.

3. What is the significance of the EM tensor?

The EM tensor is significant because it is a fundamental quantity in Einstein's theory of general relativity. It is used to describe the energy and momentum of matter and fields in a gravitational field. It also plays a crucial role in the equations of motion for objects in a curved space-time.

4. How is the EM tensor related to the conservation laws?

The EM tensor is related to the conservation laws by the Einstein field equations. These equations relate the curvature of spacetime to the energy and momentum of matter and fields. The conservation laws are a consequence of the symmetry of the EM tensor, which is a result of the laws of physics being independent of the location and orientation of the observer.

5. Can the EM tensor be extended to higher dimensions?

Yes, the EM tensor can be extended to higher dimensions. In fact, it is a fundamental quantity in theories of gravitation in higher dimensions, such as string theory. In these theories, the EM tensor is used to describe the dynamics of matter and fields in higher dimensional spacetimes.

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