Graduate Hypersurface Definition Confusion in General Relativity

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Hypersurfaces in general relativity are defined by the condition that the function f is constant, leading to confusion about the partial differential being zero. It is clarified that while f can be constant on a hypersurface, the gradient (∂_a f) must be non-zero at that hypersurface to define it properly. This is analogous to contour lines in a 2D plane, where the gradient is perpendicular to the contour line, indicating that it is not zero. The discussion emphasizes that the requirement for the gradient to be non-zero is specific to the hypersurface being described, rather than universally applicable. Understanding this distinction is crucial for correctly interpreting hypersurfaces in the context of general relativity.
tm33333
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In my notes on general relativity, hypersurfaces are defined as in the image. What confuses me is that if f=constant, surely the partial differential is going to be zero? I'm not sure if I'm missing something, but surely the function can't be equal to a constant and its partial differential be non-zero?

thanks.
 

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It's requiring that ##\partial_af## be non-zero everywhere, then saying the subset of points with the same value of ##f## define a hypersurface. Analogously, you can define a function ##f(x,y)## on a two dimensional Euclidean plane and the lines of constant ##f## are the contour lines (1d analogues to 3d hypersurfaces). The gradient on a contour isn't zero, it is perpendicular to the contour line.

(Note that geographical contour lines can close, but a closed contour line encloses at least one point where the gradient is zero, so the definition of a hypersurface excludes this possibility).
 
Well, the requirement that ##\partial_a f=0## everywhere is a bit strict. It is sufficient that it is non-zero at the hypersurface being described by the particular constant. (Although you will need the full requirement if you intend to make a foliation of the manifold.)

As an example, consider the sphere in standard Euclidean space with ##f = x^2 + y^2 + z^2##. For ##R>0##, ##f = R^2## defines a sphere of radius ##R##, which is a level surface of ##f## in ##\mathbb R^3##.
 
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Thank you both. That definitely clarifies things!
 
Moderator's note: Thread title edited to be more descriptive of the specific question.
 
tm33333 said:
Thank you both. That definitely clarifies things!
I guess you can say that they broke it down for you. :wink:
 
MOVING CLOCKS In this section, we show that clocks moving at high speeds run slowly. We construct a clock, called a light clock, using a stick of proper lenght ##L_0##, and two mirrors. The two mirrors face each other, and a pulse of light bounces back and forth betweem them. Each time the light pulse strikes one of the mirrors, say the lower mirror, the clock is said to tick. Between successive ticks the light pulse travels a distance ##2L_0## in the proper reference of frame of the clock...

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