Rotation speed of a neutron star

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Discussion Overview

The discussion centers on the rotation speed of neutron stars, exploring their rapid rotation, the mechanisms behind their spin, and the characteristics of specific types of neutron stars, such as magnetars. Participants inquire about the nature of neutron star rotation and its implications, including the processes that lead to changes in speed over time.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants propose that neutron stars retain the angular momentum of their progenitor stars, leading to rapid rotation to conserve this momentum.
  • It is noted that neutron stars can rotate at speeds up to 50,000 rpm, with variations among individual stars.
  • A common pattern discussed is the magnetar, a type of neutron star that converts rotational speed into a powerful magnetic field, with some estimates suggesting that about 15% of neutron stars are magnetars.
  • Another perspective mentions that neutron stars can "spin up" by accreting matter from a companion star, potentially leading to extreme rotation rates.
  • Participants mention that isolated neutron stars will eventually slow down over a very long time, but the mechanisms for shedding angular momentum are not straightforward.
  • Clarifications about magnetars include their exceptionally strong magnetic fields, which are much greater than those of ordinary neutron stars, and the potential for these fields to alter atomic structures.
  • One participant raises a question about the type of radiation associated with particle production in magnetars, linking it to ongoing studies in particle physics.

Areas of Agreement / Disagreement

The discussion includes multiple competing views regarding the characteristics and behaviors of neutron stars, particularly in relation to their rotation and magnetic properties. No consensus is reached on specific mechanisms or the implications of these characteristics.

Contextual Notes

Participants express uncertainty about the exact processes involved in angular momentum loss and the conditions under which neutron stars exhibit extreme rotation. There are also unresolved questions regarding the nature of particle production in the context of magnetars.

Who May Find This Useful

This discussion may be of interest to those studying astrophysics, particularly in the areas of stellar evolution, neutron star characteristics, and the interplay between rotation and magnetic fields in compact objects.

shounakbhatta
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Hello,

Can somebody please tell me in details about the rotation speed of a neutron star? Does it rotate very fast and then slows down?

Thanks.
 
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Thats the prevailing opinion. A neutron star retains the angular momentum of the star from which it formed. Because it is so much smaller than its mama, it must spin rapidly to conserve angular momentum. This is where millisecond pulsars come from. Eventually, they will spin down, but this is a very, very slow process. It is not easy to shed angular momentum without invoking unusual circumstances.
 
shounakbhatta said:
Hello,

Can somebody please tell me in details about the rotation speed of a neutron star? Does it rotate very fast and then slows down?

Thanks.

Neutron star rotation ranges up to 50000 rpm. Each star is different. A common pattern is the magnetar, in which a very young neutron star sets up a dynamo that converts most of its rotational speed to a magnetic field. Something like 15% (I forget) of neutron stars are magnetars.

Another common pattern is a star that pulls in matter from a companion. This causes the star to "spin up' and reach extreme rotations. The limit is that at superhigh rotation the star becomes asymmetrical and emits gravitational waves. Maybe 5% of neutron stars are like this.

Isolated neutron stars will eventually slow down, but this takes a very, very long time.
 
Hello,

What is meant by a magnetar?
 
A magnetar is a neutron star, generally believed to be relatively young, with an incredibly powerful magnetic field. Most neutron stars are believed to have strong magnetic fields, a magnetar has an unusually powerful magnetic field.
 
Chronos said:
A magnetar is a neutron star, generally believed to be relatively young, with an incredibly powerful magnetic field. Most neutron stars are believed to have strong magnetic fields, a magnetar has an unusually powerful magnetic field.

The Earth has a magnetic field of about half a gauss. An ordinary neutron star is about a billion gauss, which I find inconceivable. A magnetar has maybe a quadrillion gauss, and is limited to that only because electron-positron pairs start to form spontaneously in the vacuum and carry off the energy. Inside the magnetar the pairs are inhibited by the matter, so it is thought that a quintillion gauss is possible. The magnetic field can be so strong that it changes the shape of atomic nuclei, polymerizes them, and noticeably changes the shape of the star.

The highest magnetic field ever generated on Earth was about ten million gauss, produced momentarily via an explosion. A hundred thousand gauss is enough to levitate a frog.
 
ImaLooser said:
The Earth has a magnetic field of about half a gauss. An ordinary neutron star is about a billion gauss, which I find inconceivable. A magnetar has maybe a quadrillion gauss, and is limited to that only because electron-positron pairs start to form spontaneously in the vacuum and carry off the energy. Inside the magnetar the pairs are inhibited by the matter, so it is thought that a quintillion gauss is possible. The magnetic field can be so strong that it changes the shape of atomic nuclei, polymerizes them, and noticeably changes the shape of the star.

The highest magnetic field ever generated on Earth was about ten million gauss, produced momentarily via an explosion. A hundred thousand gauss is enough to levitate a frog.

I don't suppose you know what type of radiation/perturbation that particle production would fall under. I'm currently studying Hawking, Unruh, Parker and false vacuum particle production so I am curious which this form of particle production this one would best fall under.
 
That would be the Schwinger pair production mechanism.
 
  • #10
Thanks Chronos
 

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