Neutron star observations: Prognosis for equation of state constraints

JM Lattimer, M Prakash - Physics reports, 2007 - Elsevier
We investigate how current and proposed observations of neutron stars can lead to an
understanding of the state of their interiors and the key unknowns: the typical neutron star radius …

[HTML][HTML] Effects of dietary fiber and its components on metabolic health

JM Lattimer, MD Haub - Nutrients, 2010 - mdpi.com
Dietary fiber and whole grains contain a unique blend of bioactive components including
resistant starches, vitamins, minerals, phytochemicals and antioxidants. As a result, research …

The nuclear equation of state and neutron star masses

JM Lattimer - Annual Review of Nuclear and Particle Science, 2012 - annualreviews.org
Neutron stars are valuable laboratories for the study of dense matter. Recent observations
have uncovered both massive and low-mass neutron stars and have also set constraints on …

A generalized equation of state for hot, dense matter

JM Lattimer, FD Swesty - Nuclear Physics A, 1991 - Elsevier
… Hartree-Fork method, and by Lattimer') with the LLPR model. … and Baron '2,13) and by
Lattimer and coworkers i4), and both … Much of the following treatment follows the work of Lattimer

Neutron star structure and the equation of state

JM Lattimer, M Prakash - The Astrophysical Journal, 2001 - iopscience.iop.org
The structure of neutron stars is considered from theoretical and observational perspectives.
We demonstrate an important aspect of neutron star structure: the neutron star radius is …

A NICER view of the massive pulsar PSR J0740+ 6620 informed by radio timing and XMM-Newton spectroscopy

…, AK Harding, WCG Ho, JM Lattimer… - The Astrophysical …, 2021 - iopscience.iop.org
We report on Bayesian estimation of the radius, mass, and hot surface regions of the massive
millisecond pulsar PSR J0740+ 6620, conditional on pulse-profile modeling of Neutron …

The radius of PSR J0740+ 6620 from NICER and XMM-Newton data

…, S Guillot, WCG Ho, JM Lattimer… - The Astrophysical …, 2021 - iopscience.iop.org
PSR J0740+ 6620 has a gravitational mass of 2.08±0.07 M⊙, which is the highest reliably
determined mass of any neutron star. As a result, a measurement of its radius will provide …

The physics of neutron stars

JM Lattimer, M Prakash - Science, 2004 - science.org
Neutron stars are some of the densest manifestations of massive objects in the universe.
They are ideal astrophysical laboratories for testing theories of dense matter physics and …

A NICER view of PSR J0030+ 0451: millisecond pulsar parameter estimation

…, AK Harding, WCG Ho, JM Lattimer… - The Astrophysical …, 2019 - iopscience.iop.org
We report on Bayesian parameter estimation of the mass and equatorial radius of the
millisecond pulsar PSR J0030+ 0451, conditional on pulse-profile modeling of Neutron Star …

PSR J0030+ 0451 mass and radius from NICER data and implications for the properties of neutron star matter

…, AK Harding, WCG Ho, JM Lattimer… - The Astrophysical …, 2019 - iopscience.iop.org
Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear
physicists because their attributes can be used to determine the properties of the dense matter …