LEADER 05441nam 2200625Ia 450 001 9910782390603321 005 20230422045416.0 010 $a1-281-95615-5 010 $a9786611956158 010 $a981-281-043-9 035 $a(CKB)1000000000538079 035 $a(EBL)1679411 035 $a(MiAaPQ)EBC1679411 035 $a(WSP)00004553 035 $a(Au-PeEL)EBL1679411 035 $a(CaPaEBR)ebr10255633 035 $a(CaONFJC)MIL195615 035 $a(OCoLC)320955556 035 $a(EXLCZ)991000000000538079 100 $a20000607d2000 uy 0 101 0 $aeng 135 $aur|n|---||||| 200 10$aParticle physics and the universe$b[electronic resource] $eproceedings of Nobel Symposium 109 : Haga, Slott, Enko?ping, Sweden, August 20-25, 1998 /$feditors, L. Bergstro?m, P. Carlson, C. Fransson 210 $aStockholm, Sweden $cRoyal Swedish Academy of Science$dc2000 215 $a1 online resource (276 p.) 225 1 $aPhysica scripta ;$vv. T85 300 $aDescription based upon print version of record. 311 $a981-02-4459-2 320 $aIncludes bibliographical references. 327 $aContents; Committees; List of participants; Preface; Remembering David N. Schramm; References; Review of Big Bang Nucleosynthesis and Primordial Abundances; Abstract; 1. Introduction; 2. Physics of BBN; 3. Measurement of primordial abundances; 4. Deuterium in quasar spectra; 5. Helium; 6. 3He; 7. Lithium; 8. Beryllium; 9. Are the different nuclei concordant or is there a crisis?; 10. Non-standard BBN; 11. Cosmological baryon density; 12. The achievements of BBN; Acknowledgements; References; Cosmology with Clusters of Galaxies; Abstract; 1. Introduction 327 $a2. Cluster dynamics and the mass-to-light ratio4. Evolution of cluster abundance; 5. Summary; Acknowledgements; References; Determination of Cosmological Parameters; Abstract; 1. Introduction and brief historical overview; 2. Determination of Qm; 3. Determination of QA; 4. Determination of H0; 5. Determination of t0; 6. The cosmic microwave background radiation and cosmological parameters; 7. Discussion and summary; Acknowledgments; References; The Acceleration of the Universe: Measurements of Cosmological Parameters from Type la Supernovae; Abstract 327 $a1. Cosmological parameters from ""standard candles""2. Type la supernovae as ""standard candles""; 3. High-redshift supernova data; 4. Fits to QM and QA; 5. Systematic uncertainties and cross-checks; 6. Results and error budget; 7. Conclusions and discussion; References; Bias is Complicated; Abstract; 1. Introduction; 2. Ruling out simple biasing; 3. Measuring r(k); 4. Conclusions; Acknowledgements; References; Solar Neutrinos: an Overview; Abstract; 1. Introduction; 2. Standard model predictions; 3. Three solar neutrino problems; 4. Uncertainties in the flux calculations 327 $a5. How large an uncertainty does helioseismology suggest?6. Fits without solar models; 7. Neutrino oscillations; 8. Discussion and conclusion; Acknowledgements; References; Radiochemical Solar Neutrino Experiments and Implications; Abstract; 1. Introduction; 2. General considerations about radiochemical experiments; 3. Homestake chlorine experiment; 4. Gallium for pp-neutrino detection; 5. Gallex; 6. Sage; 7. Interpretation and implications; 8. Outlook; References; Evidence for Neutrino Oscillation Observed in Super-Kamiokande; Abstract; 1. Introduction; 2. Super-Kamiokande detector 327 $a3. Atmospheric Neutrinos4. Conclusion; Acknowledgements; References; Neutrino Oscillations; Abstract; 1. Introduction; 2. Atmospheric neutrinos; 3. Solar neutrinos; 4. Accelerator neutrinos; 5. Neutrino mass-mixing patterns; 6. Conclusions and prospects; Acknowledgements; References; Primary Cosmic Rays Antiprotons and Atmospheric Neutrinos; Abstract; 1. Introduction; 2. Primary spectra; 3. Atmospheric neutrinos; 4. Antiprotons; Acknowledgement; References; High Energy Cosmic Neutrinos; Abstracts; 1. Introduction; 2. Science goals; 3. High energy neutrino observatories 327 $a4. Future arrays with kilometer dimensions 330 $aIt is generally felt in the cosmology and particle astrophysics community that we have just entered an era which later can only be looked back upon as a golden age. Thanks to the rapid technical development, with powerful new telescopes and other detectors taken into operation at an impressive rate, and the accompanying advancement of theoretical ideas, the picture of the past, present and future Universe is getting ever clearer. Some of the most exciting new findings and expected future developments are discussed in this invaluable volume. The topics covered include the physics of the early U 410 0$aPhysica scripta (Stockholm, Sweden : 1982) ;$vv. T85. 606 $aParticles (Nuclear physics)$vCongresses 606 $aCosmology$vCongresses 606 $aNuclear astrophysics$vCongresses 615 0$aParticles (Nuclear physics) 615 0$aCosmology 615 0$aNuclear astrophysics 676 $a523.01972 676 $a539.7 701 $aBergstro?m$b L$g(Lars)$01508177 701 $aCarlson$b Per$01508178 701 $aFransson$b C$g(Claes)$01508179 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910782390603321 996 $aParticle physics and the universe$93739453 997 $aUNINA