Calculating Mass of Particle A After Decay Using Relativity Equations

In summary, a particle of rest mass Ma decays into two massless particles B and C with energies Eb and Ec respectively. The momenta of particles B and C are separated by an angle \theta. Using 4-momentums, it can be shown that particle A has a mass given by Ma = 1/c^2 . [sqrt(2EbEc(1- cos \theta)]. This equation can be used to easily find the energies of particles B and C using the E^2 formula.
  • #1
alfredbester
40
0
A particle of rest mass Ma, decays into two massles particles of B abd C of energy Eb and Ec respecitvely. The momenta of particles B and C are separated by an angle [tex]\theta[/tex]. Calculate the combinded momentum and combined energy of B and C and hence show that particle A has a mass given by,
Ma = 1/[tex]c^2[/tex] . [sqrt(2EbEc(1- cos [tex]\theta[/tex])]

Pa = 0 = Pb + Pc = [tex]\gamma[/tex]MbVb + [tex]\gamma[/tex]McVc

E = Ea = Eb + Ec
= [tex]\gamma[/tex]Ma[tex]c^2[/tex]

I know that Eb and Ec can be easily found using the [tex]E^2[/tex] formula, but am not sure how to take the equations and find Ma.
 
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  • #2
alfredbester said:
A particle of rest mass Ma, decays into two massles particles of B abd C of energy Eb and Ec respecitvely. The momenta of particles B and C are separated by an angle [tex]\theta[/tex]. Calculate the combinded momentum and combined energy of B and C and hence show that particle A has a mass given by,
Ma = 1/[tex]c^2[/tex] . [sqrt(2EbEc(1- cos [tex]\theta[/tex])]

Pa = 0 = Pb + Pc = [tex]\gamma[/tex]MbVb + [tex]\gamma[/tex]McVc

E = Ea = Eb + Ec
= [tex]\gamma[/tex]Ma[tex]c^2[/tex]

I know that Eb and Ec can be easily found using the [tex]E^2[/tex] formula, but am not sure how to take the equations and find Ma.

The idea here is just what you started. But use 4-momentums I think.

Using 4-momentums (I will use capital P for a 4-momentum and a lower case p for 3 momentums so there is no ambiguity)

Please note I am using units in which c=1
[tex]
(P_A)^2 = (P_B + P_C)^2
[/tex]
From the LHS of the equation:
[tex]
(P_A)^2 = m_A^2
[/tex]
From the RHS of the equation:
[tex]
(P_B + P_C)^2 = m_B^2 + m_C^2 + 2 P_B \cdot P_C
[/tex]


[tex]
p_B = (E_B,\vect{p}_b)
[/tex]
[tex]
p_C = (E_C,\vect{p}_c)
[/tex]

So:
[tex]
(P_B + P_C)^2 = m_B^2 + m_C^2 + 2 (E_B E_C - p_B p_C cos(\theta))
[/tex]

But:
[tex]
m_B = m_C = 0
[/tex]

Which implies that:
[tex]
p_B = \sqrt{E_B^2 + m_B^2} = E_B
[/tex]
[tex]
p_C = \sqrt{E_C^2 + m_C^2} = E_C
[/tex]

So therefore:
[tex]
m_A^2 = (P_B + P_C)^2 = 2 E_B E_C(1-cos(\theta))
[/tex]

Now just go back and put your c's in!
 
Last edited:

1. What are the conservation laws in relativity?

The conservation laws in relativity are the principles that state that certain quantities, such as momentum and energy, remain constant in a closed system even as objects move and interact with each other.

2. How do conservation laws relate to relativity?

Conservation laws are an important part of relativity because they help to explain how energy and momentum are conserved in different reference frames, even as objects move at high speeds.

3. What are the implications of conservation laws in relativity?

The implications of conservation laws in relativity are significant as they allow us to understand how energy and momentum are transferred and conserved in different situations, such as in collisions or when objects are moving at different speeds.

4. How do conservation laws in relativity differ from classical mechanics?

Conservation laws in relativity differ from classical mechanics in that they take into account the effects of high speeds and gravity, which can cause changes in the behavior of objects and the conservation of energy and momentum.

5. Are conservation laws in relativity absolute?

No, conservation laws in relativity are not absolute. They are dependent on the reference frame and can change depending on the relative speeds and positions of objects. However, they still hold true within a specific frame of reference.

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