- #36
PeterDonis
Mentor
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Mentz114 said:This chart of the Minkowski metric ##ds^2= -x^2dt^2+t^2dx^2+dy^2+dz^2##
Can you give the coordinate transformation from the standard Minkowski chart to this one? It's not the standard Rindler chart; that line element doesn't have the ##t^2## coefficient in front of ##dx^2##. But with that coefficient there I'm not sure what the coordinate transformation is supposed to be.
Mentz114 said:gives an acceleration of ##1/x## and expansion scalar ##1/xt##.
I assume you mean that these are the proper acceleration and expansion scalar for the congruence of worldlines that are at rest (i.e., have constant ##x##, ##y##, ##z## coordinates) in this chart, correct? Acceleration and expansion are properties of congruences of worldlines, not coordinate charts.
Mentz114 said:The expansion tensor is defined as ##\theta_{\mu\nu}= \Theta h_{\mu\nu}## where ##h=g_{\mu\nu}+U_\mu U_\nu##.
[STRIKE]I'm not sure this is a correct expression for the expansion tensor.[/STRIKE] This expression for the expansion tensor is restricted to the case where the shear is zero (see below). I'm assuming that ##\Theta## is supposed to be the expansion scalar, which is the trace of the expansion tensor; but the expansion tensor itself includes shear as well as expansion (shear is the trace-free part, expansion is the trace). The formula I'm used to seeing for the full expansion tensor (including shear) is
$$
\theta_{\mu \nu} = \frac{1}{2} h^{\alpha}{}_{\mu} h^{\beta}{}_{\nu} \left( \partial_{\beta} U_{\alpha} + \partial_{\alpha} U_{\beta} \right)
$$
[STRIKE]I'm not sure I see how to get from that to the formula you give.[/STRIKE] If the trace-free part of this (i.e., the shear) is zero, then this can be reduced to the expression you give (note that a factor of 1/3 is normally included because there are three spatial dimensions and the expansion tensor is supposed to be purely spatial).
In the particular case we're discussing, the shear *is* zero, so all of the information in the expansion tensor is contained in its trace, the expansion scalar; so I'm not sure why you are computing the full tensor anyway. The expansion scalar, as we've seen, is just ##\Theta = \partial_{\mu} U^{\mu}##, which can be computed in any inertial frame; you just need the correct transformed expression for ##U^{\mu}## in that frame.
Mentz114 said:For ##U_\mu=-\sinh(at) dt + \cosh(at) dx##
I'm not sure this is right either. The 4-velocity field in question is ##U^{\mu} = \gamma \partial_t + \gamma \beta \partial_x##; lowering an index on this gives ##U_{\mu} = \eta_{\mu \nu} U^{\nu} = - \gamma dt + \gamma \beta dx##. Since ##\gamma = \cosh (at)## and ##\gamma \beta = \sinh (at)##, this gives ##U_{\mu} = - \cosh (at) dt + \sinh (at) dx##.
Mentz114 said:if we boost this tensor by ##\beta = a t##
I'm also not sure what you mean by this. Are you transforming from one inertial frame to another? If so, ##\beta## should be a constant, not a function of ##t##, which is what it looks like you're doing here. Unless what you mean is that you are picking some particular value of ##t##, and boosting everywhere by the (constant) value of ##\beta## associated with that value of ##t##; but if you're doing that, then you are basically boosting into the instantaneous rest frame of one of the spaceships at time ##t##, and the expansion tensor you get should be purely spatial in that frame (i.e., it should have no 0-0 component, which yours does).
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