collapse, and the surface rebounds, blowing out as fast as it collpased down. As
the surface collides with the outer portions of the star an explosion occurs and the
star is destroyed in a bright flash. The material blown out from the star is
dispersed into space as a nebula. The remnants of the core becomes
• If the mass of the star is less than 3 sun's mass, star becomes a neutron star
{neutron star}. The core collapses further, pressing the protons and electrons
together to form neutrons, until neutron degeneracy stablilises it against further
collapse. Neutron stars have been detected because of their strange emission
characteristics. From the Earth, we see then a pulse of light, which gives the
neutron star its other name, a pulsar {pulsar}.
• If the mass of the star is greater than 3 sun's mass, star becomes a black hole
{black hole}. When stars of very large mass explode in a supernova, they leave
behind a core which is so massive (greater than about 3 solar masses) that it
cannot be stabilized against gravitational collapse by an known means, not even
neutron degeneracy. Such a core is detined to collapse indefinitely until it forms a
black hole, and object so dense that nothing can escape its gravitational pull, ot
even light.
Let us now start the listing of matter forms observed at a super nuclear scale (sacle larger
than the nuclear s
cale).
Atoms
Atoms are elementary bricks of matter. {atom} Atoms themselves are
compound by a set of electrons in interaction with a nucleus. This
system can be described by a planetary model fig figatome), but it
should be rigorously described by using the quantum mechanics formalism
section secatomemq). The nucleus is itself a N body problem: it is
compound by nucleons, themselves compound by quarks
Molecules
A molecule is an arrangement of some atoms {molecule}(from two to some
hundreds). Properties of molecules can be described by quantum
mechanics section secmolecmq). The knowledge of the geometry of a
molecule is sometimes enough to understand its properties. Figure
figc60fig represents fullerene molecule C60 at the origin of chemistry
Nobel price 1996 of Profs Curl, Kroto, et Smalley.
Existence of such a molecule had been predicted by the study of the adsorption spectrum
of some distant stars. Curl, Kroto, et Smalley succeeded in constructing it on the earth.
C60 molecule is compound by 12 pentagons and 20 hexagons. It is the smallest spherical
structure that can be construct using polygons{fullerene}. Polymers ) are another
example of large molecules.