Quark binding in nuclear particles Radioactive β-decay Celestial mechanics, Structure of the universe Atomic forces, binding, Optics, electricity,... Binding.

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Presentation transcript:

Quark binding in nuclear particles Radioactive β-decay Celestial mechanics, Structure of the universe Atomic forces, binding, Optics, electricity,... Binding between atoms derives from electrical attraction and repulsion Click here for a link to CERN Interatomic Binding

binding total (free) energy of the solid < sum of (free) energy of its individual, separated atoms solid energy free temperature change can change the structure Example: BaTiO 3 Click for information regarding thermodynamic potentials

Weak interaction 0.2 eV/atom typically Van der Waals interaction masked by stronger interactions, always present but solid inert gases* Graphite strong covalent bonding Van der Waals bond Solid lubricant Van der Waals bond *except He remaining liquid at normal pressure down to T->0 due to qm zero point fluctuations

Animation from: Spatulae of gecko feet are small and get so close to the surface that an attractive van der Waals force of around 0.4 µN develops between a single spatula and a surface. Combined force of the millions of spatulae on a single gecko foot produce an adhesion force of around 10 N, or around 2.25 lbs.

d p for Interaction energy: Snapshot at t=t’ +

Repulsive contribution due to Pauli exclusion principle Pauli exclusion principle: Two electrons (identical fermions) can't be in the same quantum state or total wave function of the many electron system has to be antisymmetric Electron has to leave the ground state Energy increase Repulsive interaction Click for more information Wolfgang Pauli