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Pulsar glitches from quantum vortex networks.

Giacomo Marmorini1,2, Shigehiro Yasui3,4, Muneto Nitta5,6

  • 1Department of Physics, Nihon University, Tokyo, Japan.

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Researchers analyzed pulsar glitch data, revealing a scaling law related to their energy. A new model explains these glitches using quantum vortex networks in neutron stars, specifically at the interface of inner and outer core superfluids.

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Area of Science:

  • * Astrophysics
  • * Nuclear Physics
  • * Condensed Matter Physics

Background:

  • * Neutron stars, or pulsars, are extremely dense, rapidly rotating celestial objects.
  • * Pulsar glitches, sudden reductions in rotation speed, remain a long-standing mystery.
  • * The scaling law of glitch energy distribution is a key characteristic.

Purpose of the Study:

  • * To reanalyze observational data for the pulsar glitch energy scaling law exponent.
  • * To propose a novel microscopic model for pulsar glitches.
  • * To explain the origin of glitches without free parameters.

Main Methods:

  • * Reanalysis of accumulated observational data on pulsar glitches.
  • * Development of a simple microscopic model based on superfluid interfaces.
  • * Theoretical deduction of the observed scaling law.

Main Results:

  • * Determination of the exponent for the pulsar glitch energy scaling law.
  • * Proposal of a model linking glitches to quantum vortex networks.
  • * Explanation of the scaling law derived from superfluid interactions.

Conclusions:

  • * Pulsar glitches can be explained by quantum vortex dynamics at superfluid interfaces.
  • * The model successfully deduces the observed scaling law without free parameters.
  • * The findings offer a new perspective on the internal structure and dynamics of neutron stars.