Stellar Collisions: Modeling Neutron Star & White Dwarf Interactions?

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The discussion centers on the modeling of collisions between neutron stars and white dwarfs, highlighting the complexities and challenges involved. It is established that such collisions are rare due to the tendency of stellar bodies to enter quasi-stable orbits rather than collide directly. The conversation references blue stragglers as potential outcomes of stellar mergers and notes that neutron star-neutron star (NS-NS) collisions are linked to short gamma-ray bursts. The difficulty in simulating these events arises from the lack of comprehensive understanding of neutron star interiors and the necessity of using magnetohydrodynamics codes in a general relativistic framework.

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  • Understanding of neutron star and white dwarf characteristics
  • Familiarity with stellar dynamics and orbital mechanics
  • Knowledge of magnetohydrodynamics in astrophysical contexts
  • Basic principles of general relativity
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  • Study the formation and characteristics of blue stragglers
  • Explore the mechanisms behind short gamma-ray bursts
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alvarogz
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Does it exist an accurate model about what happen when two stellar bodies collide?. I'm referring to the kind of collision between neutron stars, white dwarfs. I was wondering if that collision could produce a new kind of object. For example: a white dwarf into a neutron star, and a neutron star into a black hole.
 
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alvarogz said:
Does it exist an accurate model about what happen when two stellar bodies collide?. I'm referring to the kind of collision between neutron stars, white dwarfs. I was wondering if that collision could produce a new kind of object. For example: a white dwarf into a neutron star, and a neutron star into a black hole.

I believe that type of event is incredibly unlikely (not impossible, of course). As two stellar bodies of comparable mass approach, their v-tangents rarely cross and they usually fall into a quasi-stable mutual orbit. The one becomes the parasite of the other.

As such, I don't think that many people have spent a lot of time trying to simulate an actual impact.

I'm sure it would be interesting to see.
 
Actually, there is a class of stars called "blue stragglers" which may result from stellar collisions and mergers. In the cores of globular clusters, stars are much closer together (~ 10^5 times the density in the vicinity of the sun), so stellar collisions, especially between binary stars, become possible. Here is a starting place:

http://en.wikipedia.org/wiki/Blue_stragglers
 
Stars that are born orbiting one another will eventually collide because of the loss of energy due to tidal effects and the emission of gravitational waves. The collisions of stellar remnants (neutron stars, black holes, and maybe white dwarfs) are thought to power http://en.wikipedia.org/wiki/Gamma-ray_burst#Short_gamma-ray_bursts". These are the some of the most powerful explosions in the universe in which the bulk of x-ray to gamma-ray radiation arrives at Earth in the span of a few seconds or less.
 
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There are plenty of simulations regarding the collision of two compact objects (white dwarf (WD), neutron star (WD), or black hole(BH)) in any combination you wish. NS-NS collisions are thought to be one source of short gamma-ray bursts, as mentioned by bombadil. WD-WD collisions can trigger a type of supernova.

Collisions with black holes will cause total tidal disruption of the companion star. The star will be torn apart by the tides raised by the BH. Some of the material will escape while the rest will simply be accreted into the BH.

But these collisions are tough to simulate. We do not have a very solid understanding of the entire interior structure of NSs, so we must use various approximations. Then, computers are used to numerically solve magnetohydrodynamics codes (charged fluid in a magnetic field) in a full general relativistic setting, due to the very strong gravity of NSs and BHs.
 

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