* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download Document
Canonical quantum gravity wikipedia , lookup
Large Hadron Collider wikipedia , lookup
Higgs boson wikipedia , lookup
Renormalization group wikipedia , lookup
Neutrino oscillation wikipedia , lookup
Theory of everything wikipedia , lookup
Gauge fixing wikipedia , lookup
History of quantum field theory wikipedia , lookup
Search for the Higgs boson wikipedia , lookup
ALICE experiment wikipedia , lookup
Cosmic microwave background wikipedia , lookup
Introduction to gauge theory wikipedia , lookup
Dark matter wikipedia , lookup
Supersymmetry wikipedia , lookup
Higgs mechanism wikipedia , lookup
Future Circular Collider wikipedia , lookup
Weakly-interacting massive particles wikipedia , lookup
Mathematical formulation of the Standard Model wikipedia , lookup
Grand Unified Theory wikipedia , lookup
Elementary particle wikipedia , lookup
Technicolor (physics) wikipedia , lookup
Strangeness production wikipedia , lookup
Quantum chromodynamics wikipedia , lookup
Theoretical Issues in Astro Particle Physics J.W. van Holten April 26, 2004 The solar system is made from quarks (baryons) and leptons, interacting via weak, electro-magnetic and strong color forces. This are the only forms of matter we have been able to create in accelerators at energies up 1 TeV The dominant contribution to the mass of the universe apparently comes from other forms of matter. Neutrino masses See-saw mechanism: large Majorana mass-scale M + Higss-induced Dirac masses m generates large neutrino hierarchy: ( 0 m m M ) with M ~ 10 2 2 m = ½M ± ½(M +4 m ) _ M or m2/M = m m ~ M 6-8 GeV 2 -3 Δm ~ 10 eV 2 (Superkamiokande, SNO) Accelerator physics Extrapolation of running gauge couplings of standard model M Extrapolation of gauge couplings in the MSSM with TeV-scale supersymmetry breaking GUT ~ 10 16 GeV Supersymmetry and MSSM - All gauge and Higgs bosons have spin-1/2 partners - All quarks and leptons have spin-0 partners - The known MSM particles are distinguished from their superpartners by a new quantum number: R-parity - R-parity conservation a lightest superpartner stable - LSP candidate: neutralino χ: partner of photon / Z-boson / Higgs boson gravitino ψ: partner of graviton Rotational velocities of stars in galaxies deviation from Kepler motion Dark matter WMAP survey of Cosmic Microwave Background · flat universe · ~ 5 % baryonic matter · ~ 25 % non-baryonic matter · ~ 70 % dark energy • Neutralinos have standard weak interactions • χ – p cross-sections 10 -11 pb < σ < 10-7 pb for 100 GeV < m χ < 400 GeV (Ellis et al., 2003) • can accumulate in compact objects (stars, planets) • can annihilate to produce neutrinos New phases of matter QCD changes collective behaviour of quarks and gluons at high temperature and/or density: - deconfinement: quarks become free - chiral symmetry restoration: quarks become massless - color superconductivity: • BCS-type quark pairing • massive gluons (M. Alford) New phases of matter · Heavy-ion colliders: QGP, color glass condensate · compact cosmic objects: neutron stars, strange stars, quark stars (?) neutron matter, strange matter, color superconductivity reflected in equation of state (mass-radius relation) Cosmic accelerators 20 Highest-energy cosmics: E = 3 x 10 eV On collision with an oxygen nucleus: 6 s = 3 x 10 GeV · Accelerating mechanism? · Travel through intergalactic space? GKZ cut-off · Dynamics of interaction: quark-gluon plasma? HiSPARC Nijmegen (NAHSA) has recorded the highest-energy event ever observed in the Netherlands: ~ 0.3 J / nucleon Compact and hot early universe: · window on ultra-short distance physics · unification of gauge interactions · long-range scalar fields (inflation, quintessence) · quantum gravity, gravitational waves