Maxiumum magnetic field strength

In summary, the maximum theoretical field strength for a neutron star, and therefore for any known phenomenon is 1013 T. Why is there a maximum?Unqualified guess follows. Because, big and energetic as they are, neutron stars have a finite amount of energy too?I would guess that it's because there's a maximum possible for a normal star of particular mass. When it collapses, the field is concentrated, but there's also a maximum mass which will halt at being a neutron star. A larger one will continue to black hole status.
  • #1
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The maximum theoretical field strength for a neutron star, and therefore for any known phenomenon is 1013 T. Why is there a maximum?
 
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  • #2
Unqualified guess follows.
Because, big and energetic as they are, neutron stars have a finite amount of energy too?
 
  • #3
I would guess that it's because there's a maximum possible for a normal star of particular mass. When it collapses, the field is concentrated, but there's also a maximum mass which will halt at being a neutron star. A larger one will continue to black hole status.
 
  • #4
using the cgs version of Maxwell's equations ([itex] \mathbf{E} [/itex] and [itex] \mathbf{B} [/itex] field are dimensionally identical and [itex] \mathbf{v} [/itex] is normalized by [itex] c [/itex] in Lorentz force eq.):
[tex] \nabla \cdot \mathbf{E} = 4 \pi \rho \ </math>
[tex] \nabla \cdot \left( \frac{1}{2} \mathbf{B} \right) = 0 \ </math>
[tex] \nabla \times \mathbf{E} = -\frac{1}{c} \frac{\partial \left( \frac{1}{2} \mathbf{B} \right)} {\partial t} \ </math>
[tex] \nabla \times \left( \frac{1}{2} \mathbf{B} \right) = \frac{1}{c} \left( -4 \pi G \mathbf{J} + \frac{\partial \mathbf{E}} {\partial t} \right) = \frac{1}{c} \left( 4 \pi \rho \mathbf{v}_{\rho} + \frac{\partial \mathbf{E}} {\partial t} \right) \ [/tex]
i guess the magnitude of the [itex] \mathbf{B} [/itex] is limited by the magnitude of [itex] \rho [/itex] or [itex] \mathbf{v} [/itex] in the neutron star. [itex] |\mathbf{v}| [/itex] is limited by [itex] c [/itex] and i suppose there is a limit to [itex] \rho [/itex] in the neutron star.
(just guessing.)
 
  • #5
There is a limit because nothing can exceed the speed of light.
 
  • #6
rbj, you make my head hurt.
Tide, could you explain that please?
 
  • #7
Danger said:
rbj, you make my head hurt.
Tide, could you explain that please?

Magnetic fields arise from the flow of current or the intrinsic magnetic moment of a spinning particle (which is essentially a current). The speed of light limits the flow of current and charge is invariant under Einstein-Lorentz transformation. Assuming finite charge density, magnetic fields due to electrical current are therefore bounded by the speed of light.
 
  • #8
Well... you learn somethin' new every day. Thanks, Tide.
 
  • #9
geez, i cannot get the "Edit" button to work on the previous post. can some admin make that previous post go away? i can't even delete it. (sheesh! make a mistake with tex and it kills you.) r b-j
using the cgs version of Maxwell's equations ([itex] \mathbf{E} [/itex] and [itex] \mathbf{B} [/itex] field are dimensionally identical and [itex] \mathbf{v} [/itex] is normalized by [itex] c [/itex] in Lorentz force eq.):
[tex] \nabla \cdot \mathbf{E} = 4 \pi \rho \ [/tex]
[tex] \nabla \cdot \left( \mathbf{B} \right) = 0 \ [/tex]
[tex] \nabla \times \mathbf{E} = -\frac{1}{c} \frac{\partial \left( \mathbf{B} \right)} {\partial t} \ [/tex]
[tex] \nabla \times \left( \mathbf{B} \right) = \frac{1}{c} \left( 4 \pi \mathbf{J} + \frac{\partial \mathbf{E}} {\partial t} \right) = \frac{1}{c} \left( 4 \pi \rho \mathbf{v}_{\rho} + \frac{\partial \mathbf{E}} {\partial t} \right) \ [/tex]
i guess the magnitude of the [itex] \mathbf{B} [/itex] is limited by the magnitude of [itex] \rho [/itex] or [itex] \mathbf{v} [/itex] in the neutron star. [itex] |\mathbf{v}| [/itex] is limited by [itex] c [/itex] and i suppose there is a limit to [itex] \rho [/itex] in the neutron star.
(just guessing.)
 
  • #10
Tide said:
Magnetic fields arise from the flow of current or the intrinsic magnetic moment of a spinning particle (which is essentially a current). The speed of light limits the flow of current and charge is invariant under Einstein-Lorentz transformation. Assuming finite charge density, magnetic fields due to electrical current are therefore bounded by the speed of light.
Ah yes, thank you very much.
 
  • #11
Originally Posted by Tide
Magnetic fields arise from the flow of current or the intrinsic magnetic moment of a spinning particle (which is essentially a current).

So, what is happening in a magnet?

How does it maintain a current strong enough to generate a repulsive force?
 
  • #12
That's the cumulative field from the magnetic moment of atoms which align themselves in bunches (domains). I'm not sure what you mean by "maintain" since the magnetic moment is a permanent property of the atom.

The domains are held in place by the lattice but they (the domains) aren't necessarily permanent since they can be altered, e.g., by heating the magnet, mechanical shock or when the magnet does work.
 
  • #13
I'm not sure what you mean by "maintain" since the magnetic moment is a permanent property of the atom.

In this context I meant generate.

I was just reading an article about a problem with a machine at 3M. It was producing a static field in excess of 200Mv and at a certain time of the day, an invisible wall could be felt.

I was wondering if the same/similar principle was involved.

SESSION 7: SPECIAL SESSION, 17th Annual EOS/ESD Symposium
THURSDAY, SEPTEMBER 14, 1995, 8:00 am

SESSION 7: SPECIAL SESSION: ELECTROSTATIC CONSIDERATIONS IN INDUSTRY

MODERATOR: D. Swenson, 3M

7.7 CASE STUDY - LARGE PLASTIC WEB ELECTROSTATIC PROBLEMS, RESULTS AND CURE,

D. Swenson, 3M Company

Tremendous static charge generation on a plastic web causes unique physical phenomena and special problems. Solution was simple and cost effective.

David Swenson of 3M Corporation describes an anomaly where workers encountered a strange "invisible wall" in the area under a fast-moving sheet of electrically charged polypropelene film in a factory. This "invisible wall" was strong enough to prevent humans from passing through. A person near this "wall" was unable to turn, and so had to walk backwards to retreat from it.

http://www.amasci.com/weird/unusual/e-wall.html1
 
  • #14
On wikipedia they say that the magnetic force F is given by:
F = qv X B
Where q is the electric charge, v is the velocity of the electric charge q and B is the magnetic flux density.
Is there a different equation that relates the pull of the magnetic field with the mass of the magnetic body? Suppose i have 2 magnetized bodies A and B where B is twice the size of A, then is B's magnetic field twice as large as A's or is there a different non-linear relationship between the two.

Another question, with these neutron stars having huge magnetic fields, and seeing as a magnetic force is so much stronger than a gravitational force for objects of similar mass, why does light escape such a magnetic field? And what would such a powerfull magnetic field be ablt to pull in? I assume all objects have a slightly inbalanced magnetic distribution, or is it only some metals that have the ability to have poles? Would a neutron star's magnetic field be able to pull on a piece of wood?
 
  • #15
Aha! Back to something that I know a little bit about. The magnetic field of a neutron star (or black hole, or whatever) is the same strength as that of the original star (allowing for some mass loss during collapse). It's just a lot more concentrated, the same as the mass. It accelerates charged particles to very high velocity (hence the 'pulsar' radio signals and X-ray emissions), but has no attractive effect on normal matter. Light escapes just as it does from any other magnetic source, although it will be distorted by the gravity.

That's a fascinating quote, Moo. I don't have time to check the link right now, but am looking forward to it later.
 
  • #16
That's a fascinating quote, Moo. I don't have time to check the link right now, but am looking forward to it later.

Cheers. I found a lot of weird effects that have been studied and it would be great to obliterate the urban myths that have developed around them.

There is another link I have about people who demonstrate a magnetic like ability. Metal objects stick to them. I think, if the reports are accurate, that they are generating a localised cumulative field from the magnetic moment of atoms (thanks Tide :)). My question would be how?

Perhaps, if anyone else feels it is good idea, a section could be created to store the real scientific information behind these events. It would serve as the primary location to obtain accurate information and assist greatly in reducing the junk science across the web. In time, it would be referenced across the Internet extensively.

Due to the subject content, it would also prove to be one of the more fascinating aspects of the web.

I'll let all of you get back to the topic at hand. Thanks.
 

1. What is maximum magnetic field strength?

The maximum magnetic field strength, also known as the saturation magnetization, is the maximum amount of magnetic field that a material can hold before it becomes magnetically saturated.

2. How is maximum magnetic field strength measured?

The maximum magnetic field strength is typically measured in units of Tesla (T) or Gauss (G) using a magnetometer.

3. What factors affect the maximum magnetic field strength?

The maximum magnetic field strength of a material is affected by its composition, temperature, and external magnetic field. It also varies depending on the type of material, such as ferromagnetic, paramagnetic, or diamagnetic.

4. Why is maximum magnetic field strength important?

Maximum magnetic field strength is important in various industrial and scientific applications. It determines the strength of magnetic materials and their ability to be magnetized, which is crucial in the development of technologies such as magnetic storage devices and electromagnets.

5. Is there a limit to the maximum magnetic field strength?

Yes, there is a theoretical limit to the maximum magnetic field strength. This limit is known as the Curie temperature, and it is the temperature at which a material loses its magnetization and becomes paramagnetic.

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