Astrophysics- White dwarf collapse

In summary, a white dwarf in a binary system can generate kinetic energy when it accretes enough material to increase its mass beyond the Chandrasekhar limit and collapse to the radius of a neutron star. The difference in gravitational potential energy between the two radii can be used to calculate the amount of kinetic energy generated. This amount is significantly greater than the energy released in a supernova explosion, possibly due to the energy required for atoms to attract to each other. The efficiency of energy conversion in this process is not specified.
  • #1
HawkEye5220
7
0

Homework Statement


Calculate the kinetic energy generated when a white dwarf in a binary system accretes enough material to increase its mass beyond the Chandrasekhar limit (1.4 solar masses) and collapse to the radius of a neutron star.

radius of white dwarf- 5520 km
radius of neutron star- 12 km

Homework Equations


U=−[itex]\frac{3}{5}[/itex] [itex]\frac{GM^{2}}{R}[/itex]


The Attempt at a Solution


It has been a while since I have done a problem like this but I was thinking that if I found the gravitational potential energy at both radii and then found the difference, this difference would be the kinetic energy generated in the collapse. Am I on the right track?
 
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  • #2
Right. You have the right formula there, so you just have to plug in numbers.
 
  • #3
Thank you, it is one of those problems where it seemed too simple.
 
  • #4
Ok, after calculating. I get (-5.6*10^43 Joules) for the white dwarf and (-2.82*10^46 Joules) for the neutron star. This is a difference of 2.814*10^46 Joules, is this the amount of kinetic energy generated? Also, when I compare this number to the 10^44 Joules released by a supernova explosion it is 280 times greater. Why is this? Is it due to the fact that it requires more energy for atoms to attract to each other than it does for them to separate? Also what would the required efficiency of energy conversion be? I can't find a formula for the efficiency in our book anywhere.
 
  • #5
I get slightly different values with WolframAlpha, but that could be a rounding error.

Core collapse supernovae release much more than 10^44 J. Looking at this wikipedia table and reference 101 there the emitted energy is of the order of 10^46 J. Some other fraction of the energy gets used for endothermic fusion reactions. Looks good.
 
  • #6
I should have specified that I am comparing it to the kinetic energy of the supernova explosion which is on the order of 10^44 J. This is where I am confused.
 
  • #7
The kinetic energy of the fragments that get ejected? There is no reason to assume it would be similar to the total energy that gets released in the supernova.
 

1. What is a white dwarf?

A white dwarf is a dense, compact star that is the remnant of a low or medium mass star that has exhausted all of its nuclear fuel.

2. How does a white dwarf collapse?

A white dwarf collapses when it reaches its Chandrasekhar limit, which is the maximum mass that a white dwarf can sustain before it collapses under its own gravity.

3. What happens during the collapse of a white dwarf?

During the collapse, the core of the white dwarf becomes increasingly dense and hot, resulting in a runaway fusion reaction that causes a supernova explosion.

4. What is the significance of white dwarf collapse in astrophysics?

The collapse of white dwarfs is important in understanding the life cycle of stars and the formation of elements in the universe. It also plays a key role in the formation of neutron stars and black holes.

5. How is the collapse of white dwarfs studied?

The collapse of white dwarfs is studied through computer simulations, observations of supernova explosions, and analysis of the remnants of collapsed white dwarfs, such as neutron stars and black holes.

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