Conservation law at high speeds

  • Thread starter Thread starter stevebd1
  • Start date Start date
  • Tags Tags
    Conservation Law
stevebd1
Science Advisor
Insights Author
Messages
747
Reaction score
41
While I understand (in principle) the relationship of gravitational potential energy, kinetic energy and the conservation law in a system for an object falling towards a large mass, I'm not so familiar with how this is applies to an object traveling at high speeds. Say in the example of a spaceship, are we supposed to assume that the potential energy is the fuel on board which is slowly converted to kinetic energy as the object builds up in speed (allowing for some 'work done' quantity) so that the conservation law applies as potential energy reduces (fuel being used) kinetic energy increases? Also how does the conservation law apply at ultra-high speeds where the kinetic energy increases exponentially relative to the Lorentz factor?
 
Last edited:
Physics news on Phys.org
Here is a good page for relativistic rockets.

http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.html
 
Last edited by a moderator:
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...
Thread 'Dirac's integral for the energy-momentum of the gravitational field'
See Dirac's brief treatment of the energy-momentum pseudo-tensor in the attached picture. Dirac is presumably integrating eq. (31.2) over the 4D "hypercylinder" defined by ##T_1 \le x^0 \le T_2## and ##\mathbf{|x|} \le R##, where ##R## is sufficiently large to include all the matter-energy fields in the system. Then \begin{align} 0 &= \int_V \left[ ({t_\mu}^\nu + T_\mu^\nu)\sqrt{-g}\, \right]_{,\nu} d^4 x = \int_{\partial V} ({t_\mu}^\nu + T_\mu^\nu)\sqrt{-g} \, dS_\nu \nonumber\\ &= \left(...
In Philippe G. Ciarlet's book 'An introduction to differential geometry', He gives the integrability conditions of the differential equations like this: $$ \partial_{i} F_{lj}=L^p_{ij} F_{lp},\,\,\,F_{ij}(x_0)=F^0_{ij}. $$ The integrability conditions for the existence of a global solution ##F_{lj}## is: $$ R^i_{jkl}\equiv\partial_k L^i_{jl}-\partial_l L^i_{jk}+L^h_{jl} L^i_{hk}-L^h_{jk} L^i_{hl}=0 $$ Then from the equation: $$\nabla_b e_a= \Gamma^c_{ab} e_c$$ Using cartesian basis ## e_I...
Back
Top