Einstein's Solution to the PDE for Tau in 1905 SR Paper

In summary, Einstein solves a PDE in part 3 of his 1905 SR paper by varying x' and t' independently. He determines that the possible solution is of the form ##\tau=Ax'+Bt'## and finds the ratio of A to B by substituting the solution into the equation. He also chooses to make the constant a dimensionless. Additionally, he uses a change of variables to simplify the equation and finds the general solution as ##\tau = F(x'-bt)##.
  • #1
DoobleD
259
20
This is maybe more a maths question.

In part 3 of his 1905 SR paper, how does Einstein solves the following PDE :

img24.gif


to get :

img27.gif


?
 
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  • #2
He can vary x' and t' independently. If he keeps t' constant then ##\partial\tau/\partial t'## does not change - but he's still free to vary x'. That tells him that ##\partial\tau/\partial x'## is constant and independent of t' - in other words ##\tau=Ax'+f (t')##. He can make the same argument the other way around to get the dependence on t'. So the only possible solution is of the form ##\tau=Ax'+Bt'##. He then just substitutes that solution into get the ratio of A to B, and chooses that he wants the constant a to be dimensionless.
 
  • #3
Ibix said:
If he keeps t' constant then ∂τ/∂t′∂τ/∂t′\partial\tau/\partial t' does not change - but he's still free to vary x'.

Hmm, if t is kept constant, shouldn't ∂τ/∂t be 0 ?
 
  • #4
To solve an equation of the form
$$
\frac{\partial\tau}{\partial x'}+b\frac{\partial\tau}{\partial t} = 0
$$
where ##b## is a constant, you need the change the variables to ##\xi=x'+bt## and ##\eta=x'-bt##. Then the equation becomes very simple and you can solve it. The general solutions is
$$
\tau = F(x'-bt)
$$
where ##F## is any differentialble function. If it is linear, then you get the result in the paper.
 
  • #5
Last edited:

Related to Einstein's Solution to the PDE for Tau in 1905 SR Paper

1. What is the significance of Einstein's solution to the PDE for Tau in his 1905 Special Relativity paper?

Einstein's solution to the PDE (partial differential equation) for Tau was a crucial step in his development of the theory of Special Relativity. It allowed him to derive the famous equation E=mc^2 and laid the foundation for understanding the relationship between space and time.

2. How did Einstein come up with his solution for the PDE for Tau?

Einstein's solution for the PDE for Tau was a result of his thought experiments and mathematical reasoning. He was able to reconcile the discrepancies between the laws of electromagnetism and the principle of relativity by postulating that the speed of light is constant in all inertial reference frames.

3. What is a PDE and why is it important in Einstein's 1905 SR paper?

A PDE (partial differential equation) is a mathematical equation that involves multiple variables and their partial derivatives. In Einstein's 1905 Special Relativity paper, the PDE for Tau represented the relationship between space and time in his theory, and solving it was crucial in deriving his famous equation E=mc^2.

4. How does Einstein's solution for the PDE for Tau differ from previous theories of space and time?

Einstein's solution for the PDE for Tau was a major departure from previous theories of space and time, such as Newton's classical mechanics and Maxwell's theory of electromagnetism. It introduced the concept of a four-dimensional spacetime and challenged the traditional notions of simultaneity and the absolute nature of time.

5. How has Einstein's solution for the PDE for Tau impacted modern physics?

Einstein's solution for the PDE for Tau has had a profound impact on modern physics. It led to the development of the theory of General Relativity, which revolutionized our understanding of gravity and the structure of the universe. It also paved the way for advancements in fields such as cosmology, quantum mechanics, and particle physics.

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