Observations show that neutron stars spin very rapidly.
A beta particle is either an electron, or an anti-electron (positron). Both have a spin of 1/2.
Taking a 'particle' as a proton/ neutron, both of these have spin 1/2. So do all leptons (electrons, neutrinos, etc).
They are very hot and they will spin very rapidly - up to a hundred times a second.
A "pulsar" is a rapidly-rotating neutron star, with a core of collapsed matter. The pulsar rotates because the original star rotated. If\\ WHEN a massive star becomes a supernova, the force of the explosion will crush the core of the star into either a neutron star or a black hole, if the original star was massive enough. The angular momentum (the "spin energy") of the original star doesn't disappear; like a figure skater pulling in her arms to spin faster, the neutron star will spin more rapidly because it has collapsed in size. If the neutron star's axis is pointed somewhere close to Earth, we detect the pulsating x-rays and we call it a "pulsar". So to answer the question, all supernova remnants contain either neutron stars or black holes, but they are pulsars only if they spin rapidly.
Observations show that neutron stars spin very rapidly.
Neutron is electrically neutral... But it posses a spin... And when it moves it has a finite kinetic energy...
Neutron is electrically neutral... But it posses a spin... And when it moves it has a finite kinetic energy...
All young neutron stars spin rapidly. You might be confused with a pulsar. See related questions.
If the 3He target has its spin polarized along the axis of the neutron beam, you may consider that the protons' spin will be canceling out and the spin will be more-or-less carried by the one neutron. Thus it will prefer to absorb neutrons polarized in the opposite direction, ie negative helicity.
It is still called a neutron star. Depending on how we observe it, it may also be called a pulsar.
A beta particle is either an electron, or an anti-electron (positron). Both have a spin of 1/2.
Taking a 'particle' as a proton/ neutron, both of these have spin 1/2. So do all leptons (electrons, neutrinos, etc).
The neutron star so affected wouldn't really notice. The mass of the neutron star is huge compared to that of the material in the accretion disk. And that matter, when it falls in, wouldn't really "slow" the spin of the star much unless there was a gigantic quantity of matter falling in and/or it acted over a very long period.
In the Wii version of "I Spy : Spooky Mansion", the ending requires you to keep three plates spinning at the same time. There are two possible keys depending on your play: 1) Spin a plate, pause, spin the second plate, pause, spin the third plate. 2) Spin a plate to maximum, move to the second plate and spin it to maximum. By now the first plate is spinning down, so respin it to maximum, then move to the third plate.
2. Two electrons of opposite spin. This is true of all s, p, d, f g.... orbitals, eah can only contain two electrons of opposite spin.
They are very hot and they will spin very rapidly - up to a hundred times a second.