Stellar Collisions: Modeling Neutron Star & White Dwarf Interactions?

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Discussion Overview

The discussion revolves around the modeling of collisions between stellar bodies, specifically neutron stars and white dwarfs. Participants explore the potential outcomes of such collisions, including the formation of new astronomical objects and the implications for astrophysical phenomena like gamma-ray bursts.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants question the existence of accurate models for collisions between neutron stars and white dwarfs, suggesting that such events may lead to the formation of new objects like neutron stars or black holes.
  • One participant argues that collisions are unlikely due to the tendency of stellar bodies to enter quasi-stable orbits rather than collide directly, indicating a lack of extensive simulation efforts on actual impacts.
  • Another participant introduces the concept of "blue stragglers," which may arise from stellar collisions, particularly in dense environments like globular clusters.
  • It is noted that stars in mutual orbits may eventually collide due to energy loss from tidal effects and gravitational waves, which could lead to significant astrophysical events.
  • Participants mention existing simulations of compact object collisions, highlighting that neutron star-neutron star collisions are linked to short gamma-ray bursts, while white dwarf-white dwarf collisions can trigger supernovae.
  • Challenges in simulating these collisions are acknowledged, particularly due to uncertainties in the interior structure of neutron stars and the complexities of magnetohydrodynamics in strong gravitational fields.

Areas of Agreement / Disagreement

Participants express a mix of viewpoints, with some agreeing on the potential for stellar collisions to produce significant astrophysical phenomena, while others emphasize the challenges and uncertainties in modeling these events. No consensus is reached regarding the likelihood or outcomes of such collisions.

Contextual Notes

Limitations include the dependence on approximations for neutron star structures and the complexities involved in simulating interactions under extreme gravitational conditions.

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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