This means that for a given mass, a stiffer equation of state will predict a larger, fluffier neutron star, while a softer equation of state will predict a more compact, denser neutron star. In this paper, we assume that GW170817’s source is a binary neutron star system, where both neut...
Neutron radiography measurements of a Siemens star pattern were performed in event mode acquisition comparing two common high-resolution neutron scintillators, crystalline Gadolinium Gallium Garnet (GGG) and powdered Gadolinium Oxysulfide (GOS). An analysis of the light signature caused by neutron ...
The significant detection or exclusion of a gamma-ray eclipse provides a constraint on the binary inclination angle that depends on the angular size of the companion star as seen from the pulsar. The angular size of the companion star’s Roche lobe only depends on the binary mass ratio,q, a...
There is also a discreet (possible) Star Wars reference which I noticed when I was a kid that I'm still convinced is there.The animation, I was a bit surprised about. Being a CG animated film from 2001 that wasn't coming from Pixar or Dreamworks, you don't expect animation quality ...
Passamonti A and Andersson N 2012 Towards real neutron star seismology: accounting for elasticity and superfluidity Mon. Not. R. Astron. Soc. 419 638A. Passamonti and N. Andersson, Towards real neutron star seismology: accounting for elasticity and superfluidity, MNRAS 419 (2012) 638-655, [...
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mergers. In Evacuate Earth, a neutron star tiny and incredibly dense- is flying straight toward our solar system. Possible massive 'kilonova' explosion creates an epic afterglow. A Neutron star has very, very large feet. The biggest difference in brightness was in infrared light, measured by ...
has found signatures of strontium formed in a neutron-star merger. This artist’s impression shows two tiny but very dense neutron stars at the point at which they merge and explode as a kilonova. In the foreground, we see a representation of freshly created strontium. Image Credit:...
Solid lines in the corresponding colors are fitted error functions to the data. Full size image Small field-of-view imaging (4 × 4 cm2 active area) For high spatial resolution measurements, the chopper was removed and a white-beam radiograph of a test pattern (Siemens star made from ...
Probable frequency of real-space distances p(r) (Otherwise known as pair-distance distribution function). The inverse Fourier transform of the form factor that converts the reciprocal space scattering I(q) versus q into a frequency distribution, p, of real-space distances, r; that is, p(r)...