Energy conservation in particle decay

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Discussion Overview

The discussion revolves around the implications of energy conservation in the context of particle decay, particularly focusing on how the decay of a massive particle affects the energy of other particles in its vicinity. Participants explore theoretical scenarios involving gravitational interactions and the behavior of photons emitted during decay processes.

Discussion Character

  • Exploratory
  • Debate/contested
  • Conceptual clarification
  • Mathematical reasoning

Main Points Raised

  • Some participants propose that when a massive particle decays into a less massive particle and emits energy (e.g., a gamma ray), the energy of another gravitationally bound particle would be altered, raising questions about conservation of mass-energy.
  • Others argue that the center of mass of the system remains unchanged during decay, and the total energy is conserved when considering the energy-momentum tensor of the decay products.
  • A participant describes a hypothetical scenario involving a pion decaying into photons, suggesting that the photons would lose energy as they escape the gravitational potential of another particle, such as a proton.
  • Another participant introduces a thought experiment involving a particle decaying into photons that travel against a gravitational field, asserting that if photons were unaffected by gravity, it would lead to violations of energy conservation.
  • Concerns are raised about how the energy lost by the emitted photons relates to the energy of the other particle in the system after the decay event.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between particle decay, gravitational effects, and energy conservation. There is no consensus on how these factors interact, and the discussion remains unresolved.

Contextual Notes

Participants highlight the complexities of gravitational interactions and energy conservation in particle decay, with some assumptions about the scale of effects and the nature of gravitational potential remaining unaddressed.

nolanp2
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two massive particles a finite distance from each other are bound to each other gravitationally, so if one disappeared the other one would have its energy altered, and the conservation of mass-energy would be broken.

so what happens when a massive particle decays to a less massive particle with the emission of say a gamma ray? how would the energy of another particle in the vicinity be altered?
 
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nolanp2 said:
two massive particles a finite distance from each other are bound to each other gravitationally, so if one disappeared the other one would have its energy altered, and the conservation of mass-energy would be broken.

so what happens when a massive particle decays to a less massive particle with the emission of say a gamma ray? how would the energy of another particle in the vicinity be altered?

Consider two heavenly bodies, say the Earth and the moon. Now, consider that the moon breaks up into two pieces in an explosion. What do you think would happen gravitationally ?
 
eh the center of mass would still be at the same point so not much i would guess? but there's still the same amount of mass, it's just been separated. I'm tsalking about when the net mass of the system is reduced after the event, i don't see how the two relate.
 
nolanp2 said:
eh the center of mass would still be at the same point so not much i would guess? but there's still the same amount of mass, it's just been separated. I'm tsalking about when the net mass of the system is reduced after the event, i don't see how the two relate.

Well, the center of mass, even in the decay of a particle, will still remain the same, and the total energy also. That is to say, if you add the 4-vectors (E,px,py,pz) of the decay products, you will obtain the original (E,px,py,pz) of the original particle before decay. Now, what counts gravitationally is the E (in fact, the energy-momentum tensor, but we can do with the E here).

So imagine that you have a pi-0, gravitationally bound to, say, a proton (quite hypothetic, I know). If the pi-0 decays into two photons (each initially of energy about the mass of the pi-0 divided by 2), then those two photons will have to "climb out of the gravitational potential well" of the proton, and loose energy (shift to red). In the end, the two photons will have a total energy which is less than the energy of the pi-0, with exactly the amount of gravitational energy they needed to overcome the gravitational potential energy.

Of course, in practice this is ridiculous, because the gravitational energy of a proton and a pion are so terribly tiny as compared to the mass-energy of a pion, that you will never be able to measure this.
 
nolanp2 said:
two massive particles a finite distance from each other are bound to each other gravitationally, so if one disappeared the other one would have its energy altered, and the conservation of mass-energy would be broken.

so what happens when a massive particle decays to a less massive particle with the emission of say a gamma ray? how would the energy of another particle in the vicinity be altered?
If photons could travel against the gravitational field without loosing energy, then energy conservation would be violated. We can use this to calculate the effect of gravity on the energy (frequency) of photons.
Imagine this experiment:

A particle with mass m decays into two photons, which travel upwards for a height z in gravitational field g. Then they assemble back to original particle, which travels back to the original location. If gravity did not affect photons, then this (cyclical) proces would be a perpetuum mobile, since we would get out work done by gravitational force on every cycle.
For energy to be conserved, a photon traveling in gravitational field must loose exactly as much energy as a massive particle with m=E/c^2=h*f/c^2 (f=photon frequency).

This must also be true for infinitezimal height dz:

m*g*dz=h*df
E*g*dz/c^2=h*df
f*g*dz/c^2=h*df

Consequence:

df/dz=f*g/c^2
 
ok so the photons are still affected by the gravitational potential of the other particle after decay, but what happens to the other particle after this? is the energy lost by the photons making up for the energy gained by the other particle by losing its original graitational well?
 

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