Simultaneity in General Relativity

syra
Messages
5
Reaction score
0
I had a much longer post typed with quotes and everything but I was auto-logged out, couldn't recover the text, and don't feel like typing it all in full. >:[

William Lane Craig, in "Einstein, Relativity, and Absolute Simultaneity" says that the Friedman metric as solution to Einstein's field equations (standard in cosmology) produces a unique hypersurface of simultaneity. Is this true, or is more than one hypersurface of simultaneity possible?
 
Physics news on Phys.org
Short answer: Each coordinate system defines simultaneity differently, but there's one particular coordinate system that's particularly well suited to describe the large-scale behavior of the universe. That's the coordinate system he's talking about. (I doubt that he fully understands that though).

Longer answer: The Friedmann(-Lemaitre-Robertson-Walker) class of solutions of Einstein's equation describe those spacetimes that can be sliced into a one-parameter family of spacelike hypersurfaces that are homogeneous and isotropic in a specific technical sense. It's convenient to choose the parameter that labels the hypersurfaces to be the proper time (from the big bang to the event where it intersects the hypersurface) of a geodesic that's orthogonal to the hypersurfaces. This convention enables us to think of the hypersurface labeled by parameter value t as "space, at time t". The "preferred" coordinate system is defined by choosing the coordinate time of any event to be equal to the parameter that labels the hypersurface, and by choosing the coordinate distance between any two points in the same hypersurface to be the proper distance in that hypersurface.

There are many ways to slice one of these spacetimes into hypersurfaces that we can think of as "space" at different "times", but there's only one slicing with the nice properties mentioned above. That's why the "nicest" coordinate system we can associate with that slicing can be considered "preferred".

Next time, make sure that you check the "remember me" box when you log in.
 
Last edited:
Ah man, thanks Fredrik. When I first read this from Craig, I instantly thought it was something like the case with the Levi-Cevita connection: it's the unique torsion-free one, but this doesn't mean that which tangent vectors are parallel or not on a manifold is uniquely determined (i.e. absolute), as there are many connections possible. Elegance and niceness isn't the same as absoluteness.
 
In this video I can see a person walking around lines of curvature on a sphere with an arrow strapped to his waist. His task is to keep the arrow pointed in the same direction How does he do this ? Does he use a reference point like the stars? (that only move very slowly) If that is how he keeps the arrow pointing in the same direction, is that equivalent to saying that he orients the arrow wrt the 3d space that the sphere is embedded in? So ,although one refers to intrinsic curvature...
I started reading a National Geographic article related to the Big Bang. It starts these statements: Gazing up at the stars at night, it’s easy to imagine that space goes on forever. But cosmologists know that the universe actually has limits. First, their best models indicate that space and time had a beginning, a subatomic point called a singularity. This point of intense heat and density rapidly ballooned outward. My first reaction was that this is a layman's approximation to...
So, to calculate a proper time of a worldline in SR using an inertial frame is quite easy. But I struggled a bit using a "rotating frame metric" and now I'm not sure whether I'll do it right. Couls someone point me in the right direction? "What have you tried?" Well, trying to help truly absolute layppl with some variation of a "Circular Twin Paradox" not using an inertial frame of reference for whatevere reason. I thought it would be a bit of a challenge so I made a derivation or...
Back
Top