What is Einstein's equation used for?

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Discussion Overview

The discussion revolves around the applications of Einstein's equation E² = (mc²)² + (pc)², particularly in contexts beyond nuclear reactions. Participants explore various scenarios where this equation might be relevant, including theoretical and experimental applications.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants note that the equation is primarily applicable in nuclear reactions, where E = mc² can be simplified under conditions of zero momentum.
  • Others argue that the equation can also be used to calculate binding energies in atoms and is relevant in particle physics for computing mass, energy, or momentum of particles.
  • A participant mentions that the particle experiments at CERN demonstrate the mass-energy relationship and relativistic kinetic energy, suggesting practical applications in high-energy physics.
  • Another participant highlights the theoretical applications of the equation in contexts such as the thrust of a relativistic rocket engine.
  • One contribution discusses the specific case of positron emission tomography (PET), where the energy of emitted photons relates to the equation, illustrating a medical application.
  • There is a mention of the total loss of rest mass in the Sun due to nuclear fusion, with a clarification that the fusion process itself does not affect the Sun's mass directly.

Areas of Agreement / Disagreement

Participants express a range of views on the applications of the equation, with no clear consensus on specific practical applications beyond those mentioned. Some focus on theoretical implications, while others emphasize experimental contexts.

Contextual Notes

Limitations include the equation's applicability primarily under relativistic conditions, which may restrict its practical use in everyday scenarios. Additionally, some assumptions about the contexts in which the equation is applied remain unresolved.

Ashley Warnes
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I've been doing some research into Einstein's equation E2=(mc2)2 +(pc)2 but apart from in nuclear reactions, where you can use the simpler E=mc2 as momentum=0, I have been unable to find any applications.

Thank you in advance
 
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Ashley Warnes said:
I've been doing some research into Einstein's equation E2=(mc2)2 +(pc)2 but apart from in nuclear reactions, where you can use the simpler E=mc2 as momentum=0, I have been unable to find any applications.

Thank you in advance

It depends what you mean by an application. Beyond the atomic level rest mass is generally conserved. That said, the total of all the nuclear fusion in the Sun amounts to a huge loss of rest mass per second.
 
Thank you for your response.
Obviously it can be used to calculate the energy for a change of mass taking into account momentum, but I was hoping to find applications like in nuclear fusion where the equation can be demonstrated if that makes sense.
 
Ashley Warnes said:
Thank you for your response.
Obviously it can be used to calculate the energy for a change of mass taking into account momentum, but I was hoping to find applications like in nuclear fusion where the equation can be demonstrated if that makes sense.

The particle experiments at CERN, for example, are continual demonstrations of special relativity, including the mass/energy relationship and the definition of relativistic KE and momentum.
 
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https://www.google.com/search?q=pet+scan+photon+energy

The 511 keV photon energy (E) comes from Einstein's famous equation E = mc2 , where m is the mass of the electron or positron (a very small number) and c is the speed of light (a very large number - squared) This annihilation radiation is what is detected in PET and what is used to form images of tracer concentration ...
Physics of PET - University of Washington
http://depts.washington.edu/imreslab/education/Physics of PET.pdf
https://en.wikipedia.org/wiki/Positron_emission_tomography
 
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Ashley Warnes said:
I have been unable to find any applications.

Of course it's hard to find practical aplication because the formula makes sense under relativistic conditions only. But there are a lot of theoretical applications, e.g. for the thrust of a relativistic rocket engine.

PeroK said:
That said, the total of all the nuclear fusion in the Sun amounts to a huge loss of rest mass per second.

Just to be more precise: It’s the emission of particles and radiation that results in the loss of mass. The fusion itself has no effect on the mass of the Sun.
 
Particle physicists use that equation when they need to compute the mass, energy, or momentum of a particle from the other two quantitles.

Example: accelerate an electron (mc2 = 511 keV) from rest through a potential difference of 1 million volts (1000 kV). What is its momentum? (which determines e.g. the radius of curvature of its path when it travels through a given magnetic field)

Solution: From ##\Delta K = q \Delta V##, the kinetic energy is 1000 keV. The total energy (kinetic plus rest energy) is E = 1000 keV + 511 keV = 1511 keV. Therefore, the momentum (in energy units) is ##pc = \sqrt {E^2 - (mc^2)^2} = \sqrt {(1511~\rm{keV})^2 - (511~\rm{keV})^2} = 1422~\rm{keV}##.
 

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