Neutron Stars and unbinding energy

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SUMMARY

The discussion focuses on calculating the velocity required to unbind two neutron stars using gravitational binding energy. The gravitational binding energy (Ug) is defined as Ug = GM^2/R, where G is the gravitational constant, M is the mass of the stars, and R is their separation distance. Participants suggest equating the kinetic energy of the neutron stars before collision to the total gravitational binding energy, noting that the binding energy can also be expressed as 3GM^2/5R. The discussion acknowledges the unrealistic assumption of neglecting inter-atomic forces.

PREREQUISITES
  • Understanding of gravitational binding energy (Ug)
  • Familiarity with Newton's law of gravitation
  • Knowledge of kinetic energy equations
  • Basic concepts of neutron stars and their properties
NEXT STEPS
  • Research the derivation of gravitational binding energy for different celestial bodies
  • Study the kinetic energy equations in astrophysical contexts
  • Explore the properties and behaviors of neutron stars
  • Investigate the role of inter-atomic forces in astrophysical collisions
USEFUL FOR

Astronomy students, astrophysicists, and anyone interested in the dynamics of neutron star collisions and gravitational interactions.

Minihoudini
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Homework Statement


The Gravitational binding energy of an object consisting of loose material, held together by gravity alone, is the amount of energy required to pull all of the material apart, to infinity. the gravitational binding energy Ug is roughly given by GM^2/R. how fast do you have to smash two neutron stars to get sufficient energy to unbind them?


Homework Equations


I honestly don't know where to start. I believe my teacher is asking for the velocity and then get the energy? also what formula should I use?


The Attempt at a Solution



im thinking we use Ug=Gm^2/R and use Ug= -GMm/r and have r= Tv/2pi
 
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The energy needed to overcome the gravitational forces keeping the neutron star matter together would have to come from the kinetic energy of the stars before collision. When they collide, that energy would have to be converted into kinetic energy of the individual molecules. Although this is thermodynamically not possible, I think that the question assumes that this is the case.

So equate the kinetic energy of two neutron stars of mass M as they are about to collide to the total gravitational binding energy of the two stars.

The question assumes that there are no inter-atomic forces other than gravity, which is not realistic.

Incidentally, the binding energy is 3GM^2/5r. See: http://en.wikipedia.org/wiki/Gravitational_binding_energy

AM
 

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