Probe into the interior of compact stars
Nana Pan, Miao Kang
TL;DR
This paper reviews methods, especially r-mode instability, to investigate the dense nuclear matter inside neutron stars, highlighting potential insights from observations like the XTE J1739-285 pulsar.
Contribution
It summarizes current probing techniques for neutron star interiors and presents new results related to r-mode instability implications.
Findings
R-mode instability can provide insights into neutron star interior composition.
The KHz pulsar XTE J1739-285 offers significant observational implications.
Proposed methods can help confirm the presence of various subatomic particles inside neutron stars.
Abstract
The interior of neutron stars contains nuclear matter at very high density for numerous subatomic particles compete with each other. Therefore, confirming the components and properties there is our significant task. Here we summarize the possible methods especial the way of r-mode instability to probe into the neutron star and show our some results. The KHz pulsar in XTE J1739-285 may give a significant implication
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Taxonomy
TopicsHistory and Developments in Astronomy