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Pulsars are rotating neutron stars that are renowned for their timingprecision, although glitches can interrupt the regular timing behavior whenthese stars are young. Glitches are thought to be caused by interactionsbetween normal and superfluid matter in the star. We update our recent work ona new technique using pulsar glitch data to constrain superfluid and nuclearequation of state models, demonstrating how current and future astronomytelescopes can probe fundamental physics such as superfluidity near nuclearsaturation and matter at supranuclear densities. Unlike traditional methods ofmeasuring a star's mass by its gravitational effect on another object, ourtechnique relies on nuclear physics knowledge and therefore allows measurementof the mass of pulsars which are in isolation.

Pinning down the superfluid and nuclear equation of state and measuring neutron star mass using pulsar glitches