Mr. Tompkins in Wonderland - a clarification

  • Thread starter Thread starter ahaanomegas
  • Start date Start date
ahaanomegas
Messages
28
Reaction score
0
I don't have the book Mr. Tompkins in Wonderland, but I have heard about it. A little introduction is needed. Mr. Tompkins lives in a world where the speed of light is 20 mph. Here, of course, relativity must be taken into account almost always. I was wondering about length contraction, though. If Mr. Tompkins is riding his bike at a speed close to that of light, he looks thinner to those standing on the sidewalk and the men on the sidewalk look fatter to Mr. Tompkins. Am I right? I'm a little confused about that about what is seen to whom and who sees what.

Thanks in advance!
 
Physics news on Phys.org
No. If Mr Topkins is moving at speed v relative to the people on the side walk, then they are moving at speed v relative to him. He sees them as thinner and they see him as thinner than if they were motionless relative to him.
 
Nice link, thanks.
 
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