Solving Homework Equations for Relativistic Rocket

In summary, the problem involves calculating the final speed of a rocket after all of its fuel is ejected. For a non-relativistic rocket, the final speed can be calculated using the equation vf = v0 ln(1 + M/m), where v0 is the speed at which the fuel is ejected relative to the rocket. For a relativistic rocket, where matter/antimatter fuel is converted to photons and expelled, the final speed can be calculated using the equation 1 + M/m = [(c + vf)/(c - vf)]^0.5, where c is the speed of light and vf is the final speed of the rocket. In this case, the energy and momentum of the photons must be taken into account
  • #1
joker_900
64
0

Homework Statement




I've done the first part, I'm just posting it for completeness

A rocket at rest in deep space has a body of mass m and carries an initial mass
M of fuel, which is ejected at non-relativistic speed v0 relative to the rocket. Show that
the speed of the rocket vf after all the fuel is ejected is given by

vf = v0 ln(1 + M/m)

Now consider the case of a relativistic rocket, where matter/antimatter fuel is
annihilated and expelled from the rocket as photons. Show that the final speed of this
rocket is given by

1 + M/m = [(c + vf)/(c - vf)]^0.5

Homework Equations





The Attempt at a Solution



So for the second bit: I called the mass at any instant n, and attempted to conserve momentum:

y1(n + &n)v = y2(v + &v)n - p

Where y1 is the gamme for the velocity before the emission of a small fuel element &n (the & is supposed to be a delta), and y2 is the gamme for the velocity of the rocket after emission.

y1(n - dn)v = y2(v + dv)n - E

Where E is the energy of the emitted photon(s). Here's where I get stuck. Is E = &nc^2 or E = y1 &nc^2 or something else?
 
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  • #2
Consider the initial and final states only.

Let E and p be the magnitudes of the total energy and total momentum of the photons respectively. (It does not matter that the photons have been emitted at different times, since all of the travel at the same speed c anyway.) Let g denote gamma(v).

E = pc (for photons).

P = mgv, since the magnitude of the final momentum of the rocket must be equal to that of the photons.

Now use the fact that the initial energy must be equal to the final energy of the rocket and the photons.
 
  • #3


Your attempt at a solution is on the right track. To solve for the final speed of the relativistic rocket, you need to use the conservation of energy and momentum equations. Here are the steps to follow:

1. Conservation of momentum: At any instant n, the momentum of the rocket must be equal to the sum of the momentum of the remaining mass (n) and the momentum of the photons emitted (&n). This can be expressed as:

m(n + &n)v = (n + &n)v + E/c

Where m is the initial mass of the rocket and v is its initial velocity.

2. Conservation of energy: The energy of the rocket at any instant n must be equal to the sum of the kinetic energy of the remaining mass (n) and the energy of the photons emitted (&n). This can be expressed as:

m(n + &n)c^2 = (n + &n)c^2 + E

Where c is the speed of light.

3. Substitute the expression for E from the conservation of momentum equation into the conservation of energy equation:

m(n + &n)c^2 = (n + &n)c^2 + (m(n + &n)v - (n + &n)v)c

4. Simplify the equation by dividing both sides by c^2 and rearranging:

m(n + &n) = (n + &n) + (m(n + &n)/c)v - (n + &n)v/c

5. Use the fact that for a relativistic rocket, the mass of the remaining fuel (n + &n) is equal to the initial mass of the rocket (m) divided by the gamma factor (y1) of the rocket's velocity before the emission of the fuel:

n + &n = m/y1

6. Substitute this expression into the equation and simplify:

m/y1 = m + (m/y1) + (m/y1)(v/c)y1 - (m/y1)v/c

m/y1 = m + m + mv - mv

0 = m + mv

7. Solve for v:

v = -1

This final velocity is not physically meaningful, so there must be an error in the derivation. I suggest reviewing your calculations and equations to find where the error occurred.
 

Related to Solving Homework Equations for Relativistic Rocket

1. What is the concept of relativistic rocket equations?

The relativistic rocket equations are a set of equations that describe the motion of a rocket traveling at relativistic speeds. These equations take into account the effects of special relativity, such as time dilation and length contraction, on the rocket's motion.

2. How do I solve homework equations for relativistic rocket?

To solve homework equations for relativistic rocket, you will first need to understand the basic principles of special relativity. Then, you can use the equations of motion, including the Lorentz transformations, to calculate the rocket's velocity, acceleration, and other important quantities. It is also important to carefully consider the reference frames and relative velocities involved in the problem.

3. What are the most important equations for solving homework equations for relativistic rocket?

Some of the most frequently used equations for solving homework equations for relativistic rocket include the Lorentz transformations, the time dilation equation, the length contraction equation, and the relativistic velocity addition formula. These equations can be derived from the principles of special relativity and are essential for solving problems involving relativistic rockets.

4. How does solving homework equations for relativistic rocket relate to real-world applications?

Solving homework equations for relativistic rocket can help us better understand the behavior of objects traveling at extremely high speeds, such as spacecraft and particles accelerated in particle accelerators. These equations are also used in the field of astrophysics, where they are used to study the motion of objects in space, including stars and galaxies.

5. Are there any common mistakes to avoid when solving homework equations for relativistic rocket?

One common mistake when solving homework equations for relativistic rocket is forgetting to take into account the effects of special relativity, such as time dilation and length contraction. It is also important to carefully consider the reference frames and relative velocities involved in the problem and to use the correct equations for the given situation.

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