Magnetic Fields of Neutron Stars

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Discussion Overview

The discussion revolves around the magnetic fields of neutron stars and pulsars, exploring their origins, stability, and the underlying physics. Participants examine theoretical models, particle interactions, and the structural composition of neutron stars, with a focus on the implications for their strong magnetic fields.

Discussion Character

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

Main Points Raised

  • Some participants note that neutron stars and pulsars have extremely strong magnetic fields, amplified during the core collapse of their progenitors.
  • There is speculation regarding the role of other particles, such as W or Z bosons, in mediating electromagnetic forces within neutron stars, as neutrons alone may not account for the observed magnetic fields.
  • One participant highlights the non-uniform structure of neutron stars, suggesting that layers, including an atmosphere of iron nuclei, contribute to the magnetic field's characteristics.
  • Another participant proposes that quantum-statistical Fermi-Dirac effects and the spin rate of neutron stars may play a role in maintaining their magnetic fields, comparing them to magnetars and white dwarfs.
  • It is mentioned that neutrons possess a small magnetic field, which could contribute to the overall strength of the magnetic field in neutron stars.
  • A question is raised about the numerical values of the electric moments of neutrons versus protons, indicating a curiosity about their relative magnitudes.
  • A participant introduces the concept of "Magnestars," suggesting it as a related but less commonly discussed topic in the context of neutron stars.

Areas of Agreement / Disagreement

Participants express various hypotheses and models regarding the magnetic fields of neutron stars, with no consensus reached on the mechanisms involved or the significance of different contributing factors.

Contextual Notes

Some claims rely on specific assumptions about particle interactions and the structure of neutron stars, which may not be universally accepted or fully resolved within the discussion.

Nebula
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It is a known fact that neutron stars and pulsars, remnants of super nova explosions, have very strong magnetic fields. It is said that the collapse of the core amplifies the magnetic field of the progenitor. This is due to the fact that the magnetic fields lines are drawn closer together during the collapse by the contracting material. The magnetic fields of neutron stars and pulsars are millions, even trillions of times stronger than the Earth’s magnetic field. The current http://www.physicspost.com/imageview.php?imageId=34 model for a pulsar describes two hotspots on the surface of the star that lie along the magnetic axis generating beams of out going radiation that produce the characteristic pulses of these stars.

How is it that the magnetic field of these stars is able to retain its stability for so long if the star is essentially made up of neutral matter (neutrons)? My current speculation is that there must be some sort of other particle mediating the electromagnetic force within the neutron stars, perhaps the W or Z boson; which are weak nuclear force carriers that are produced in various nuclear processes such as beta decay. Moving charge, variable electric fields and other phenomena can generate magnetic fields, but neutrons alone cannot generate these fields unless something else is going on or there are other particles involved. How are the high magnetic fields of neutron stars and pulsars sustained?
 
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Originally posted by Nebula
It is a known fact that neutron stars and pulsars, remnants of super nova explosions, have very strong magnetic fields. It is said that the collapse of the core amplifies the magnetic field of the progenitor. This is due to the fact that the magnetic fields lines are drawn closer together during the collapse by the contracting material. The magnetic fields of neutron stars and pulsars are millions, even trillions of times stronger than the Earth’s magnetic field. The current http://www.physicspost.com/imageview.php?imageId=34 model for a pulsar describes two hotspots on the surface of the star that lie along the magnetic axis generating beams of out going radiation that produce the characteristic pulses of these stars.

How is it that the magnetic field of these stars is able to retain its stability for so long if the star is essentially made up of neutral matter (neutrons)? My current speculation is that there must be some sort of other particle mediating the electromagnetic force within the neutron stars, perhaps the W or Z boson; which are weak nuclear force carriers that are produced in various nuclear processes such as beta decay. Moving charge, variable electric fields and other phenomena can generate magnetic fields, but neutrons alone cannot generate these fields unless something else is going on or there are other particles involved. How are the high magnetic fields of neutron stars and pulsars sustained?
Because Neutron stars are not of a consistent structure or uniformity throughout. See the info at:

http://www.astro.umd.edu/~miller/nstar.html#formation
It explains at several places on the page the workings of a neutron star that give rise to the huge magnetic fields.
 
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Thanks for the link Labguy. So essentially a neutron star isn’t made up entirely of neutrons. I completely overlooked the fact that the star might have various stratified layers particularly the “atmosphere” consisting primarily of iron nuclei. Thanks again for the info. :smile:
 
Nebula-

Try also Scientific American February 2003, "Magnetars," page 34. I believe the maintenance of the magnetic field is due to quantum-statistical Fermi-Dirac effects as well as the rate of spin of that neutron star. The latter I liken to blue giants (magnetars) burning out more rapidly than white dwarves (conventional pulsar). The greater the spin and thus field, the shorter its duration.
 
Uhmm, and

It should also be noted that neutrons are known to have their own magnetic field, small, exceedingly small, but it is there.

Coalesence, and amplification, could easily lead to this being an aspect of the entire magnetic fields strength, and origin.

After all, a neutrons composition is a positron (positive) and an electron (negative) within, what had been a proton, and those are the two energies of magnets. (when contained within one object)
 
What is the neutron vs proton electric moment numerically? Exceedingly small?
 
What you are asking about, and talking about is a Magnestar, do a search for them, they are a fringe topic and don't get a lot of coverage.
 

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