Schwarzschild: Energy Conservation at Finite r

In summary, the four velocity and four momentum of a massive particle are denoted by ##u^\alpha## and ##p^\alpha## respectively. The time like Killing vector ##\xi^\alpha = (1,0,0,0)## leads to the conservation of ##E / m## as ##r \longrightarrow \infty##. However, for finite values of ##r##, the quantity being conserved is the GR analogue of total energy, which includes both kinetic and potential energy in the weak field limit with non-relativistic velocities relative to ##\xi##.
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kent davidge
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Let ##u^\alpha## and ##p^\alpha## denote a massive particle's four velocity and four momentum, respectively. Also, let ##\xi^\alpha = (1,0,0,0)## be a time like Killing vector. Since ##g_{00} \xi^0 u^0 = g_{00} p^0 / m = -(1 - 2m / r) E / m## is conserved, if we let ##r \longrightarrow \infty## we have that ##E / m## is conserved. This is the particle's energy per mass. But how to think about that term when ##r## is finite? What's the quantity that's being conserved there?
 
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A GR analogue of total energy in this case. If you look at the weak field limit with non-relativistic velocities relative to ##\xi##, you can expand in small quantities and obtain the Newtonian total energy = kinetic + potential.
 
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1. What is Schwarzschild: Energy Conservation at Finite r?

Schwarzschild: Energy Conservation at Finite r is a concept in physics that describes how energy is conserved in a black hole according to the Schwarzschild metric, which is a mathematical solution to Einstein's field equations of general relativity.

2. How does the Schwarzschild metric relate to energy conservation?

The Schwarzschild metric describes the curvature of spacetime around a non-rotating, spherically symmetric mass, such as a black hole. This curvature affects the motion of particles and photons, and through the conservation of energy, it determines the behavior of energy in this region.

3. What is the significance of energy conservation at finite r in black holes?

Energy conservation at finite r is significant because it helps us understand how energy behaves in the extreme conditions of a black hole. It also plays a crucial role in the study of black hole thermodynamics and the information paradox.

4. How does energy conservation at finite r impact our understanding of the universe?

Energy conservation at finite r is an important concept in the study of general relativity and the behavior of matter and energy in the universe. It helps us understand the properties of black holes, which are some of the most mysterious and fascinating objects in the universe.

5. Are there any real-world applications of energy conservation at finite r?

While there are currently no direct real-world applications of energy conservation at finite r, the principles and concepts involved have been used in the development of technologies such as GPS systems, which rely on the precise calculations of time and space based on the curvature of spacetime.

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