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Neutron Degeneracy

Neutron Degeneracy

Neutron degeneracy is a stellar application of the Pauli Exclusion Principle, as is electron degeneracy. No two neutrons can occupy identical states, even under the pressure of a collapsing star of ...

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http://hyperphysics.phy-astr.gsu.edu/hbase/astro/pulsar.html#c3
Neutron Stars - Introduction

Neutron Stars - Introduction

Brief introduction from NASA on the nature of neutron stars, the most dense objects known, created in the cores of massive stars during supernova explosions. Includes links to related topics.

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http://imagine.gsfc.nasa.gov/docs/science/know_l1/neutron_stars.html
ISIS Pulsed Neutron & Muon Source

ISIS Pulsed Neutron & Muon Source

The homepage of the world's leading pulsed neutron source

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http://www.isis.rl.ac.uk/
Autobiography of Bertram N. Brockhouse

Autobiography of Bertram N. Brockhouse

Bertram N. Brockhouse (1918 - ) received the Nobel Prize for Physics in 1994 for pioneering contributions to the development of neutron scattering techniques for studies of condensed matter. In ...

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http://nobelprize.org/nobel_prizes/physics/laureates/1994/brockhouse-autobio.html
Event Horizon

Event Horizon

After collapse to the neutron star stage, stars with masses less than 1-3 solar masses should remain neutron stars. Those of masses greater than 1 to 3 collapse toward zero spatial extent - toward a ...

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http://hyperphysics.phy-astr.gsu.edu/hbase/astro/blkhol.html#c1
Hyperphysics - Neutrons

Hyperphysics - Neutrons

Structure and stability of the neutron with good links to other relevant parts of the site.

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http://hyperphysics.phy-astr.gsu.edu/hbase/particles/proton.html#c3
Nuclear Isotope Half-Lifes

Nuclear Isotope Half-Lifes

The site demonstrates the half-life of ten basic nuclei and you can add or subtract a proton or a neutron to the current isotope.

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http://lectureonline.cl.msu.edu/~mmp//kap30/Nuclear/nuc.htm
Cygnus X-1

Cygnus X-1

Doppler studies of this blue supergiant in Cygnus indicate a period of 5.6 days in orbit around an unseen companion. The mass of the companion is calculated to be 8-10 solar masses, much too large to ...

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http://hyperphysics.phy-astr.gsu.edu/hbase/astro/blkbin.html#c1
Neutron Star

Neutron Star

For a sufficiently massive star, an iron core is formed and still the gravitational collapse has enough energy to heat it up to a high enough temperature to either fuse or fission iron. Either in the ...

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http://hyperphysics.phy-astr.gsu.edu/hbase/astro/pulsar.html#c1
Autobiograpy of Clifford G. Shull

Autobiograpy of Clifford G. Shull

Clifford G. Shull (1915 - 2001) received the Nobel Prize for Physics in 1994 for pioneering contributions to the development of neutron scattering techniques for studies of condensed matter.

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http://nobelprize.org/nobel_prizes/physics/laureates/1994/shull-autobio.html
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