This neutron star must have a quadrupole distribution of matter or higher 
order. A neutron star is composed largely of neutron fluid. If this is 
rotating there may be set up by thermal gradients and Coriolis acceleration 
convection flows that would set up such a distribution of matter. It is one 
possible reason the millisecond pulsar is the upper limit on their spin.

LC

On Monday, November 9, 2020 at 8:10:29 AM UTC-6 [email protected] wrote:

> A pulsar is a Neutron Star that is rotating hundreds of times a second and 
> is sending out radio pulses when it does so. If the Neutron Star was 
> perfectly spherical it would not generate any Gravitational Waves no matter 
> how fast it was rotating and neither would it if it was flattened at the 
> poles into a perfect oblate spheroid as long as it was still symmetrical, 
> but if there was any irregularity it would generate Gravitational Waves. 
> The waves would be far weaker than those generated by Black Hole collisions 
> but nevertheless LIGO would still be able to detect them because unlike the 
> Black Hole case the generation of these ways would be continuous and even 
> more important because they know the frequency of the Gravitational waves 
> if they existed because they already know the radio frequency of the 
> pulsar. So they know what frequency to look for. A recent paper looked for 
> these waves that must have been generated by several different pulsars if 
> they were irregular and they didn't find any, they were able to conclude 
> that any variation from being perfectly symmetrical for a Neutron Star 20 
> km across must be smaller than the width of a human hair.
> By the way I've never seen a paper with that many authors.
>
> Gravitational-wave constraints on the equatorial ellipticity of 
> millisecond pulsars <https://arxiv.org/abs/2007.14251>
>
>
>   John K Clark
>
>
>

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