Four-vector from 3 space components?

  • Thread starter Thread starter jason12345
  • Start date Start date
  • Tags Tags
    Components Space
jason12345
Messages
108
Reaction score
0
If in some frame I define a geometrical object as having 3 space components, how do I then find the time component component it must have?

I've defined a geometrical object in some frame as having components Ax, Ay, Az defined by:

d/dx Ax = Fx, d/dx Ay = Fy, d/dy Ay = Fy

I require that for any frame:

1/gamma d/dx'A'x' = Fx, d/dy' A'y' = Fy, d/dy' A'y' = Fy

Is it possible to define the form the time component A0 takes?

Thanks.
 
Physics news on Phys.org
Can't you just define your four-vector by specifying your three components in the frame in which the time component is zero, and then Lorentz transform to an arbitrary frame?
 
If you've mapped out a space grid with rulers, the usual approach is to put a bunch of clocks on that grid, synchronize them via the Einstein convention (assuming that this is possible, which requires the frame not be rotating), and then use the proper time read by each clock to determine the time coordinates of events.

I hope this answers your question?
 
Fredrik said:
Can't you just define your four-vector by specifying your three components in the frame in which the time component is zero, and then Lorentz transform to an arbitrary frame?

I don't know what the time component is at all, so I can't say if it's zero or not, but you have given me an idea. I have (A0, A1, A2, A3), with A1' transforming as:

A1' = gamma (A1 - V A0)

Setting A1 = 0 for a suitable x,t gives:

A0 = - A1'/(gamma V) -- (1)

Cheers!
 
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...
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(...
Abstract The gravitational-wave signal GW250114 was observed by the two LIGO detectors with a network matched-filter signal-to-noise ratio of 80. The signal was emitted by the coalescence of two black holes with near-equal masses ## m_1=33.6_{-0.8}^{+1.2} M_{⊙} ## and ## m_2=32.2_{-1. 3}^{+0.8} M_{⊙}##, and small spins ##\chi_{1,2}\leq 0.26 ## (90% credibility) and negligible eccentricity ##e⁢\leq 0.03.## Postmerger data excluding the peak region are consistent with the dominant quadrupolar...
Back
Top