The lambda hyperon and the hyperon puzzle
Wazha German, Dr Jacobus Diener

TL;DR
This paper discusses how hyperons, especially lambda hyperons, influence the equation of state of neutron stars, highlighting the hyperon puzzle where theoretical models conflict with observations of high-mass neutron stars.
Contribution
It provides an analysis of the lambda hyperon's role in neutron star matter using relativistic mean field theory, addressing the hyperon puzzle.
Findings
Inclusion of lambda hyperons softens the neutron star EoS.
Softening EoS reduces maximum neutron star mass.
Observations of high-mass neutron stars challenge hyperon-inclusive models.
Abstract
Neutron stars provide unique conditions to study cold dense nuclear matter at extreme densities. Due to these extreme conditions additional hadronic degrees of freedom are expected to be populated,including hyperons. This talk will focus on the influence of hyperons on the neutron star equation ofstate. In particular the contribution of the lambda hyperon will be discussed, as a first approximation to describing exotic neutron star equations of state. The system under consideration is where the strong nuclear force is described by the exchange of mesons and applying the relativistic mean field theory to study dense nuclear matter. As expected, the inclusion of the lambda hyperon softens the neutron star equation of state (EoS). A softer EoS will reduce the maximum mass attainable by the modeled neutron star with such EoS. While hyperons are certainly not unexpected in high density…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Geophysics and Gravity Measurements · Gamma-ray bursts and supernovae
