Speed of Light Paradox: Neutron Star Rotation Rate

In summary, the conservation of momentum can still hold true for a neutron star rotating at high speeds, as momentum does not increase linearly with speed. Any momentum can be obtained with a speed less than the speed of light. The classical Newtonian approximation only holds for speeds much less than ##c##.
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jflies
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TL;DR Summary
If a neutron star spins fast enough, doesn't it imply that either (1) surface speeds greater than the speed of light are possible or (2) angular momentum is not conserved?
Sorry if this is a stupid question but I couldn't find an answer anywhere. According to 2 scientific papers, the neutron star PSR J1748-2446ad has a rotation rate of 716Hz, which equates to a linear surface speed of 0.24c. What if this star was originally rotating, let's say, 5 times (or more) faster before it collapsed. That would imply that it's surface speed would reach 1.2c. How could the conservation of momentum hold true unless speeds greater than 1c are allowed?
 
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  • #2
Angular momentum does not scale linearly with angular velocity. It approaches infinity as the linear speed approaches ##c##. So any initial angular momentum can be accommodated in the collapsed state without exceeding the speed of light.

Note that neutron stars are extremely complicated objects and you really need to think about their full stress-energy tensor.
 
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Likes Dale and vanhees71
  • #3
Ok thanks for the quick response (and not making fun of my lack of knowledge)!
 
  • #4
jflies said:
Summary: If a neutron star spins fast enough, doesn't it imply that either (1) surface speeds greater than the speed of light are possible or (2) angular momentum is not conserved?

Sorry if this is a stupid question but I couldn't find an answer anywhere. According to 2 scientific papers, the neutron star PSR J1748-2446ad has a rotation rate of 716Hz, which equates to a linear surface speed of 0.24c. What if this star was originally rotating, let's say, 5 times (or more) faster before it collapsed. That would imply that it's surface speed would reach 1.2c. How could the conservation of momentum hold true unless speeds greater than 1c are allowed?

Momentum does not increase linearly with speed. Linear momentum, ##p##, for example is given by:

##p = \frac{mv}{\sqrt{1-v^2/c^2}}##

You can see from this formula that any momentum can be obtained (no matter how large) with a speed of less than ##c##.

When ##v## is small compared to ##c##, then you get the classical, Newtonian approximation:

##p \approx mv##

But that only holds for speeds much less than ##c##.
 
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  • #5
PeroK said:
Momentum does not increase linearly with speed. Linear momentum, ##p##, for example is given by:

##p = \frac{mv}{\sqrt{1-v^2/c^2}}##

You can see from this formula that any momentum can be obtained (no matter how large) with a speed of less than ##c##.

When ##v## is small compared to ##c##, then you get the classical, Newtonian approximation:

##p \approx mv##

But that only holds for speeds much less than ##c##.
Yup, I was only considering the Newtonian approximation. Thanks for the clarification.
 

1. What is the speed of light paradox?

The speed of light paradox refers to the concept that the speed of light is considered to be the fastest speed possible in the universe, yet there are objects, such as neutron stars, that appear to rotate at speeds close to the speed of light.

2. How is the rotation rate of a neutron star measured?

The rotation rate of a neutron star is typically measured by observing the periodic pulses of electromagnetic radiation emitted from its poles. This is known as pulsar timing and can be used to determine the rotation rate of the neutron star.

3. How fast can a neutron star rotate?

Neutron stars can rotate at incredibly fast speeds, with some pulsars rotating hundreds of times per second. The fastest known pulsar, PSR J1748-2446ad, has a rotation rate of 716 times per second.

4. How does the rotation rate of a neutron star relate to the speed of light paradox?

The rotation rate of a neutron star is directly related to the speed of light paradox because the faster the star rotates, the closer it gets to the speed of light. This raises questions about the limitations of the speed of light and how objects can seemingly exceed it.

5. What are the implications of the speed of light paradox for our understanding of physics?

The speed of light paradox challenges our current understanding of physics and the laws of the universe. It raises questions about the nature of time, space, and the limitations of the speed of light. Further research and study of neutron stars and their rotation rates may provide insights into these fundamental questions.

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