Presentation on theme: "The University of Coimbra"— Presentation transcript:
1The University of Coimbra Some highlights ofNuclear Physics atThe University of CoimbraManuel Fiolhais Centre for Computational Physics (CFC-UC) University of Coimbra, PortugalNuPECC meeting, Lisboa, November 2004
2Department of Physics~ 55 staff members~ 10 are nuclear & hadron physicistsOther areas: condensed matter (clusters,X-ray diffraction), high energy, cosmology, instrumentation, electronics, education, etc.
3Centre for Computational Physics Research activity organized in5 Research CentresCentre for Computational Physics(~25% nuclear physics)Centre for Theoretical Physics(~50% nuclear physics)
4Lab for advanced computing of CFC 100 processors interconnected“Centopeia”(centipede)
5Publications in international journals Physical Review CPhysical Review DPhysical Review LettersPhysics Letters BNuclear Physics ANuclear Physics BEuropean Physics JournalEurophysics LettersJournal of Physics G: Particle and Nuclear Physics
6Some keywords (not exhaustive) Relativistic Nuclear PhysicsNuclear Physics at Intermediate energiesEffective models of QCDChiral symmetryPhenomenology of the nucleon and isobarsMeson spectroscopyAstrophysics
7The Ds (2117) meson in a unitarized quark model Eef van BeverenNumber 643 #1, June 26, 2003 by Phil Schewe, James Riordon, and Ben SteinThe Meson Ds(2317)The meson Ds(2317), discovered a couple of months ago in high energy electron-positron collisions at SLAC, possesses a mass of GeV, some 170 MeV lighter than expected, at least according to prevalent theories of quark interactions. Hence physicists need a new explanation of how a charm quark attached to an antistrange quark should have this particular mass. In general, Ds and D mesons are a class of particles, each consisting of a charm quark attached to a light antiquark. (The subscript "s" pertains to all those D's containing a strange antiquark; "ordinary" D mesons consist of a charm quark and a down antiquark.) The Babar detection group at SLAC responsible for the experimental discovery (Aubert et al., Physical Review Letters, 20 June 2003; also see press release) suggests that the Ds(2317) might be a novel particle made of 4 quarks. But a pair of physicists in Portugal claim that in their model, assuming that the meson is indeed a charm/antistrange combination, the mass comes out in the right range if the strong-nuclear-force interactions responsible for the creation and annihilation of extra quark-antiquark pairs are taken into account. Using this model, Eef van Beveren (University of Coimbra) and George Rupp (CFIF Lab, IST, Lisbon) have successfully predicted meson masses in the past (such as the kappa meson, discovered at Fermilab (E791) at a mass of 800 MeV), while in the case of Ds mesons they predict a mass very near the Ds(2317) found already, and another at about 2.9 GeV (yet to be found). As to D mesons, they predict the equivalent of the Ds(2317) at a mass range of GeV (for which preliminary evidence exists), and a heavier one at about 2.8 GeV (still undetected). According to van Beveren and Rupp, both pairs of Ds and D mesons are, in some sense, different aspects of the same underlying quark-antiquark state. (Physical Review Letters, upcoming article, see website or contact George Rupp, )199619971998199920002001200220032004
8Chiral gauge theories and heavy-ions Brigitte Hiller and Alex BlinDynamics of chiral gauge theories in a generalized Schwinger-DeWitt approach: generalization to arbitrary non-degenerate mass matrices.Calculation of the low lying spectrum of pseudoscalarsCalculation of the low lying spectrum of scalarsCalculation of pion-kaon scattering lengthsDescription of resonance production in ultra-relativistic heavy-ion reactions.Invariant mass spectra of various channelsRatios of resonancesAbundances and transverse momentum spectraCorrelations in the invariant mass of decay products.
9(3-flavour) Nambu-Jona Lasínio model Maria da Conceição RuivoPhase transitions, restoration of symmetries and meson properties at finite temperature and density- Phase transitions in hot and dense matter- Pseudoscalar meson properties (masses and quark meson coupling constants)- Two photon decays of the neutral mesons 0 and in vacuum and in medium- Effective restoration of chiral and UA(1) symmetry at finite temperature and density
10EoS and relativistic nuclear matter Constança ProvidênciaEOS for stellar matter:- hadronic matter: non-linear Walecka model (NLWM) with hyperons, quark meson coupling model (QMC) with hyperons and kaon condensate, NLWM with meson- quark matter: su(3) NJL model and MIT Bag model in the normal phase and CFL phase- mixed phase: global charge conservationEOS in hadronic matter, with chiral symmetry.Collective modes in relativistic matter for asymmetric matter- relativistic Vlasov equationAsymmetric matter liquid-gas phase transition in relativistic models- relativistic mean field- NLWM, NLWM with density dependent coupling constants, NLWM with meson, QMC-spinodal, direction of instability, effect of Coulomb interactionCorrelations in relativistic models: EOS for nuclear matterHartree-Fock with correlations (unitary operator)Algebraic models
11Pseudospin symmetry in nuclei Pedro Alberto, MFPseudospin symmetry as a dynamical symmetry in nucleiDependence with potential parameters (radius, thickness,depth)Coulomb effectsDegeneracy between single-particle states
12Nucleon and isobar description: Nucleon properties and NN* transitionsMF et al.The nucleon as a chiral solitonLinear sigma modelChromodielectric modelChiral-quark-soliton model(NJL inspired)Bag models (CBM, etc.)Nucleon and isobar description:Electromagnetic propertiesAxial propertiesStrong properties
13Astroparticle physics MF et al.- Application of quark models to the EOS quark matter and study of compact objects (hybrid stars, quark stars)From NASA press release 02-65, April 10th 2002:“NASA's Chandra X-ray Observatory has found two stars - one too small, one too cold - that reveal cracks in our understanding of the structure of matter. These discoveries open a new window on nuclear physics, offering a link between the vast cosmos and its tiniest constituents. Chandra's observations of RX J and 3C58 suggest that the matter in these stars is even denser than nuclear matter found on Earth. This raises the possibility these stars are composed of pure quarks…”RX JChandra X-ray image
14Programmed activities Axial form factors of N-Electromagnetic NN* transitionsStructure functionsQuark distributionsMedium effects in the nucleonStudies of pseudo-spin symmetries in nucleiEtc.
15Collaborations abroad Bochum (Germany)Ljubljana (Slovenia)Rio de Janeiro, S. Paulo, Florianópolis, Belo Horizonte (Brazil)Cracow (Poland)JINR, Dubna (Russia)