neutron stars

One of the best possible sources for gravitational waves would be a merger between compact binary neutron stars.

A third topic is that of the high-density colour superconductive state of matter, which may be present in the core of neutron stars.

He said the neutron stars can be no larger than about 20. 5 miles (33 kilometers) across.

To find out how strong the crusts of neutron stars really are, Horowitz and a colleague created a computer simulation of a star's surface.

Strong gravitational waves are thought to be produced by the collision of two neutron stars.

One of the neutron stars is a pulsar; it emits radio pulses at regular intervals as it spins 45 times per second.

however , it is now proposed that the conversion of neutron stars to strange stars is another possible origin of gamma - ray bursts.

Due to the existence of high viscosity in strange matter, strange stars can reach much shorter period than neutron stars.

People who believe in astrology or aliens may look for hidden meaning in this model of a black hole sucking neutron stars into its maw.

The most likely explanation for GRB050709 is that it was produced by a collision of two neutron stars, or a neutron star and a black hole.

For M15, the HST astronomers relied on an earlier estimate of the number of neutron stars in the cluster.

Carbon Earths might be especially prevalent in more bizarre settings, such as the environs of white dwarfs and neutron stars.

Pulsars are widely thought to be rapidly rotating, magnetized neutron stars.

There is a positive observational and theoretical basis for believing that neutron stars and black holes follow as a result of supernovae.

The pair calculated what would happen if dark matter particles like these were attracted by the intense gravity of neutron stars.

We discuss the observational masses, redshifts and rotation frequencies constraints on the equations of state in the cores of neutron stars.

Pictured above is an artist's illustration depicting two neutron stars spiraling in toward each other, just before they collide.

Also shown are huge clouds of multimillion degree gas and bright point like sources due to neutron stars and black holes.

Pulsars are rotating neutron stars that are observable as sources of electromagnetic radiation.

Since neutron stars have solid crusts and are born in violent supernova explosions, they probably will have mountains.

However, we should be aware that pulsars may not be neutron stars at all, they may be Strange Stars!

Neutron stars are created when massive stars run out of fuel and collapse.

Not just any old relics, neutron stars are the leftover cores of huge stars that exploded in supernovae.

Radio pulsars are neutron stars with an immensely strong magnetic field.

Their new findings suggest these positrons originate mainly from stars getting devoured by black holes and neutron stars.

Searching for X- ray sources in the sky becomes the most important ways to locate neutron stars and black holes among binary system .

These systems likely contain neutron stars or stellar mass black holes that represent final stages in stellar evolution.

"We could look for evidence that neutron stars don't live very long in regions with a lot of dark matter, " he says.

We adopt a new train of thought to constrain the equations of state of neutron stars.

Einstein's predicted warping of space-time has been discovered around neutron stars, the most dense observable matter in the universe.

The relatively low figure allowed them to state with confidence that neutron stars alone could not explain the star motions they saw.

In particular, a new study suggests that neutron stars can spin only so fast before they begin to emit gravity waves.

This requires even more detectors because these waves are even weaker than the waves from binary stars and neutron stars.

So instead of looking at many neutron stars, researchers needed to look at only this one.

Some neutron stars become pulsars , stars that send off pulses of radio waves. These can also cause gravitational waves.

Neutron superfluid vertex in neutron stars is discussed in this paper.

The neutron stars rotate around, - we discussed that earlier-- - conservation of angular momentum-- and they have strong magnetic fields.

Likewise, it can't go on forever because Cas A would get far colder than neutron stars generally do.

The nuclear force can maintain the stability of a nuclei so that it can also maintain the stability of the neutron stars.

Pulsars: Neutron Stars or Strange Stars?

With the results from this pulsar search, we improve our understanding of how many binaries with neutron stars may be out there in total.

Neutron stars contain the densest known matter that is directly observable.

For example, spinning neutron stars called pulsars emit clocklike streams of electromagnetic pulses.

So, scientists can add neutron stars to their list of cosmic things they can test in the lab.

Are some known neutron stars actually strange stars?

Angular Momentum - Torques - Conservation of Angular Momentum - Spinning Neutron Stars - Stellar Collapse

Comparison of Two Methods for Calculating Properties of Rotating Neutron Stars

Neutron Superfluid Vortex in Neutron Stars and Its Astronomical Effects

Study of the Gravitational Energy in Neutron Stars

Description of Nuclear Matter and Neutron Stars in Density-dependent Relativistic Mean Field Theory

Describing Neutron Stars with the Relativistic Mean Field Theory

Two relevant models are introduced: (1) The neutrino rocket model for neutron stars with high velocities;

Electron capture of strong magnetic field in the outer crusts of neutron stars

Density Dependence of Proton Fraction in Neutron Stars

Equation of State and Proton Ratio on the Inner Shell Layer of Neutron Stars

Much more dense than neutron stars

In-Medium Effects on Neutron Stars