Conservation of relativistic energy

In summary: In this case, that's E1:\begin{align*}m_0c^2 &= E_1 + E_2 \\0 &= p_1c + p_2c\\m_0(c-1) &= E_1 - E_2 \\0 &= p_1(-c+1) + p_2c\end{align*}Once you have that, solving for c leaves you withc=\frac{p_1c}{2}So, in summary, the particles of rest mass m_0 disintegrate into two particles of rest masses m_1 and m_2
  • #1
stepheng123
3
0
A particle of rest mass m_0 disintegrates into two particles of rest masses m_1 and m_2.
Use conservation of relativistic energy and relativistic 3-momentum to find the energies E1 and E2 of the particles in the rest fram of the original particle.

Relevant equations:
E0 = E1 + E2
p0 = p1+ p2

?
 
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  • #2
stepheng123 said:
A particle of rest mass m_0 disintegrates into two particles of rest masses m_1 and m_2.
Use conservation of relativistic energy and relativistic 3-momentum to find the energies E1 and E2 of the particles in the rest fram of the original particle.

Relevant equations:
E0 = E1 + E2
p0 = p1+ p2

?
put values in p0 = p1+ p2

you will have m1v1 = m2v2
 
  • #3
cupid.callin said:
you will have m1v1 = m2v2

Would it not be m1v1 = -m2v2 as p0 = 0 ?
And how would this lead to me obtaining the energies of the particles?
 
  • #4
no ... v1 will be opposit to v2

so m_o(0) = m1v1-m2v2 => m1v1 = m2v2

but i don't think that Eo = E1 + E2 will be valid ... if by E you mean mechanical energy
 
  • #5
Stick with E's and p's instead of using velocities. So far you have

[tex]\begin{align*}
E_0 &= E_1 + E_2 \\
0 &= p_1 + p_2
\end{align*}[/tex]

What equations do you have relating energy, momentum, and mass?
 
  • #6
vela said:
What equations do you have relating energy, momentum, and mass?

I have E[tex]^{2}[/tex] = p[tex]^{2}[/tex]c[tex]^{2}[/tex] + m[tex]^{2}[/tex]c[tex]^{4}[/tex]

I need E1 and E2 in terms of c, m0, m1 and m2..
 
  • #7
Good. Since p0=0, you know E0=m0c2, and you can multiply the second equation by c, which leaves you with

[tex]
\begin{align*}
m_0c^2 &= E_1 + E_2 \\
0 &= p_1c + p_2c
\end{align*}
[/tex]

You're going to want to square the equations, subtract the second from the first, and use the relation you have to replace combinations of E2 and (pc)2 with (mc2)2. The trick is to first arrange the equations so that the cross term you get from squaring conveniently let's you solve for one of the energies.
 

FAQ: Conservation of relativistic energy

What is the conservation of relativistic energy?

The conservation of relativistic energy is a fundamental principle in physics which states that the total energy of a closed system remains constant over time, regardless of any changes that may occur within the system. This means that energy can neither be created nor destroyed, but can only be transformed from one form to another.

How is relativistic energy different from classical energy?

Relativistic energy is based on the theory of special relativity, which takes into account the effects of high speeds and large masses on energy. In contrast, classical energy is based on Newtonian physics and does not consider these effects. Relativistic energy also includes the concept of mass-energy equivalence, which means that mass and energy are different forms of the same underlying quantity.

3. How is relativistic energy calculated?

The equation for relativistic energy is E = mc^2, where E is energy, m is mass, and c is the speed of light. This equation shows that energy is directly proportional to mass, and as an object's speed approaches the speed of light, its energy increases significantly.

4. What does the conservation of relativistic energy mean for the behavior of particles?

The conservation of relativistic energy has important implications for the behavior of particles, particularly at high speeds. As particles approach the speed of light, their mass and energy increase, making it more difficult to accelerate them further. This is why it is impossible for an object with mass to reach the speed of light.

5. How does the conservation of relativistic energy impact our daily lives?

The conservation of relativistic energy is a fundamental principle that governs the behavior of matter and energy in our universe. It has led to groundbreaking discoveries and technologies, such as nuclear power and medical imaging. This principle also helps us understand the behavior of particles in high-energy environments, such as particle accelerators, and has implications for space travel and the study of the universe.

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