Equation of state
Definition: The relation among pressure, density, temperature, and composition of neutron-star matter.
Why it matters here: In Neutron-Star Structure and Equation of State, Equation of state is needed to reason about mass-radius inference, compactness, redshift, and dense-matter constraints rather than merely label the phenomenon.
Relationship: It is interpreted alongside Compactness and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: The spherical, static metric is an approximation; rotation and atmosphere modeling affect inferred radius.
\(1+z=(1-2GM/Rc^2)^{-1/2}\)
Compactness
Definition: The dimensionless strength 2GM/(Rc^2) of relativistic gravity at a stellar surface.
Why it matters here: In Neutron-Star Structure and Equation of State, Compactness is needed to reason about mass-radius inference, compactness, redshift, and dense-matter constraints rather than merely label the phenomenon.
Relationship: It is interpreted alongside Gravitational redshift and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: The spherical, static metric is an approximation; rotation and atmosphere modeling affect inferred radius.
Gravitational redshift
Definition: The increase in photon wavelength between a compact object's surface and a distant observer.
Why it matters here: In Neutron-Star Structure and Equation of State, Gravitational redshift is needed to reason about mass-radius inference, compactness, redshift, and dense-matter constraints rather than merely label the phenomenon.
Relationship: It is interpreted alongside Mass-radius relation and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: The spherical, static metric is an approximation; rotation and atmosphere modeling affect inferred radius.
Mass-radius relation
Definition: The sequence of equilibrium stellar masses and radii predicted by a chosen dense-matter equation of state.
Why it matters here: In Neutron-Star Structure and Equation of State, Mass-radius relation is needed to reason about mass-radius inference, compactness, redshift, and dense-matter constraints rather than merely label the phenomenon.
Relationship: It is interpreted alongside Pulse-profile modeling and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: The spherical, static metric is an approximation; rotation and atmosphere modeling affect inferred radius.
Pulse-profile modeling
Definition: Inference of mass, radius, geometry, and emission properties from relativistically distorted rotational light curves.
Why it matters here: In Neutron-Star Structure and Equation of State, Pulse-profile modeling is needed to reason about mass-radius inference, compactness, redshift, and dense-matter constraints rather than merely label the phenomenon.
Relationship: It is interpreted alongside Equation of state and the lecture relation below; identify which quantities are observed, calibrated, or model-derived.
Limitation or common confusion: The spherical, static metric is an approximation; rotation and atmosphere modeling affect inferred radius.