How Do You Determine the Four-Vector Quantities for a Moving Particle?

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SUMMARY

The discussion focuses on determining the four-vector quantities for a moving particle, specifically its four-velocity, position as a function of proper time, and the four-force. The four-velocity is expressed as uμ = γ(c, cgt / (1 + g²t²)¹/²), where γ = (1 / (1 + g²t²))⁻¹/². The position x is derived as x = (c/g)(1 + g²t²)¹/², and the relationship between coordinate time t and proper time τ is established through the integral of γ = dt/dτ. The four-force is defined as mass times the derivative of four-velocity, requiring further differentiation with respect to proper time.

PREREQUISITES
  • Understanding of four-vectors in special relativity
  • Familiarity with the concept of proper time (τ) and coordinate time (t)
  • Knowledge of the Lorentz factor (γ) and its derivation
  • Basic calculus skills for integration and differentiation
NEXT STEPS
  • Study the derivation of the Lorentz factor (γ) in detail
  • Learn about hyperbolic functions and their applications in relativity
  • Explore the concept of four-force and its implications in relativistic physics
  • Practice integrating functions involving square roots and trigonometric substitutions
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This discussion is beneficial for first-year physics students, particularly those studying special relativity and looking to understand the mathematical framework behind four-vectors and their applications in particle dynamics.

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Homework Statement


A particle of mass m has a position along the x-axis as a function of time given by the equation

u = cgt / (1 + g2t2)1/2

where g is a constant and c is the speed of light.
(a) Find the 4-velocity of the particle.
(b) Express x and t as a function of the proper time of the particle.
(c) Find the 4-force acting on the particle. Does it ever exceed the speed of light?

Homework Equations



uμ = γ(c, u)

λ = dt / dτ

The Attempt at a Solution



a) Given the first equation, the four-velocity is simply

uμ = γ(c, cgt / (1 + g2t2)1/2

I think.
b) To find the position, we take the integral of dx/dt and find

x = (c/g)(1 + g2t2)1/2

If we let dt = γdτ, then we can easily see t = γτ.

However, this is a problem, as the particle is accelerating (its second time derivative is not zero) and that means γ must change. And, another problem, is that we cannot sub in

γ = (1 - u2/c2)-1/2

because then we have a recursive definition.
c) I know that the four-force is simply mass x second derivative of the four position (or mass x derivative of four-velocity), but I am not too sure how to differentiate it. I also know that the four-force is (F0, F) but I don't know how to find F0 :(
PLEASE BE GENTLE. I am a first-year physics student, and my university decided to put general relativity into a first-year course.
 
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Dakkers said:

Homework Statement


A particle of mass m has a position along the x-axis as a function of time given by the equation

u = cgt / (1 + g2t2)1/2

where g is a constant and c is the speed of light.
You mean velocity, right?

a) Given the first equation, the four-velocity is simply

uμ = γ(c, cgt / (1 + g2t2)1/2

I think.
That's right. Since you know the speed u(t), you can write down an expression for ##\gamma## as a function of t and simplify it a bit.

b) To find the position, we take the integral of dx/dt and find

x = (c/g)(1 + g2t2)1/2

If we let dt = γdτ, then we can easily see t = γτ.

However, this is a problem, as the particle is accelerating (its second time derivative is not zero) and that means γ must change. And, another problem, is that we cannot sub in

γ = (1 - u2/c2)-1/2

because then we have a recursive definition.
Your expression for x(t) is correct, but your reasoning about how t and τ are related isn't. Integrate ##\gamma = \frac{dt}{d\tau}## where you have expressed ##\gamma## as a function of t. (Hint: use the substitution gt = sinh θ.) Then you can write x as a function of the proper time.

c) I know that the four-force is simply mass x second derivative of the four position (or mass x derivative of four-velocity), but I am not too sure how to differentiate it. I also know that the four-force is (F0, F) but I don't know how to find F0 :(
The derivatives are with respect to the proper time τ. It might become clear how to do this after you have expressions for t(τ) and x(τ) from the previous parts of the problem.
 
vela said:
Your expression for x(t) is correct, but your reasoning about how t and τ are related isn't. Integrate ##\gamma = \frac{dt}{d\tau}## where you have expressed ##\gamma## as a function of t. (Hint: use the substitution gt = sinh θ.) Then you can write x as a function of the proper time.


The derivatives are with respect to the proper time τ. It might become clear how to do this after you have expressions for t(τ) and x(τ) from the previous parts of the problem.

Our professor never actually mentioned hyperbolic functions :\
 
I'm not too sure how to integrate γ, either. I am so bad at this.
 
What expression did you get for ##\gamma## in terms of t? You don't have to use hyperbolic functions. You could use a trig substitution, but I think it works out more simply with sinh.
 
I got

γ = (1 / (1 + g2t2))-1/2
 
Good. You can simplify it a bit more:
$$\gamma = \sqrt{1+(gt)^2}.$$So now you have
$$\frac{dt}{d\tau} = \sqrt{1+(gt)^2},$$ which you can solve to find ##t(\tau)##.
 
would it simply be

t = (1 + (gt)2)1/2τ

?
 
No, you can't do that because t varies as τ does. What you have to do is get t on one side and τ on the other:
$$d\tau = \frac{1}{\sqrt{1+(gt)^2}}\,dt$$and then you can integrate both sides to get
$$\tau = \int \frac{1}{\sqrt{1+(gt)^2}}\,dt$$
 

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