LEADER 05372nam 2200709Ia 450 001 9910826679403321 005 20200520144314.0 010 $a981-277-624-9 035 $a(CKB)1000000000412951 035 $a(EBL)1681061 035 $a(OCoLC)879074375 035 $a(SSID)ssj0000277073 035 $a(PQKBManifestationID)12087162 035 $a(PQKBTitleCode)TC0000277073 035 $a(PQKBWorkID)10232857 035 $a(PQKB)10699627 035 $a(MiAaPQ)EBC1681061 035 $a(WSP)00005176 035 $a(Au-PeEL)EBL1681061 035 $a(CaPaEBR)ebr10201298 035 $a(CaONFJC)MIL505377 035 $a(EXLCZ)991000000000412951 100 $a20030424d2002 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 10$aASAP 2002 $eastrophysics, symmetries, and applied physics at spallation neutron sources /$feditors, Paul E. Koehler ... [et al.] 205 $a1st ed. 210 $aSingapore ;$aRiver Edge, N.J. $cWorld Scientific$dc2002 215 $a1 online resource (264 p.) 300 $aThe Workshop on Astrophysics, Symmetries, and Applied Physics at Spallation Neutron Sources was held at the Oak Ridge National Laboratory, Mar. 2002. 311 $a981-238-249-6 320 $aIncludes bibliographical references and index. 327 $aContents ; Preface ; Schedule for the Workshop on ASAP ; Participant List ; Neutron Capture Nucleosynthesis: Astrophysical Processes and Laboratory Approaches ; 1 Introduction ; 2 The Observed Abundances ; 3 Neutron Capture Scenarios ; 4 The Case of the s Process 327 $a5 s Process Models 6 s-Process Branchings ; 7 Neutron Data for Astrophysics: Status and Needs ; 8 Summary ; References ; The Detector for Advanced Neutron Capture Experiments at LANSCE ; 1 Introduction ; 2 Neutron Source ; 3 Preliminary Data with C6D6 Scintillators 327 $a4 DANCE Design 5 Summary and Future Plans ; References ; Astrophysics Program at the CERN n_TOF Facility ; 1 Introduction ; 2 Priority measurements for nuclear astrophysics ; 3 Conclusion and perspectives ; Acknowledgments ; References 327 $aRecent Astrophysics Results from ORELA and Possible Future Experiments at ORELA and SNS 1 Introduction ; 2 Recent ORELA Results and the Need for New Measurements ; 3 The Need for the SNS ; Acknowledgements ; References 327 $aSensitivity of Isotope Yields to Reaction Rates in the Alpha Rich Freezeout 1 Introduction ; 2 The calculations ; 3 Web-based data display ; 4 Examples ; 5 Conclusion ; Acknowledgements ; References ; Neutron Reactions of Light Nuclei from Astrophysics & Nuclear Physics Interest 327 $a1 Introduction 330 $a The spallation neutron source (SNS) being built at the Oak Ridge National Laboratory (ORNL) will be by far the highest flux pulsed source of epithermal neutrons in the world when it comes on line in 2006. Although the main thrust of the science program at the SNS will be materials science, the facility could provide outstanding opportunities for research in nuclear astrophysics, fundamental symmetries, and applied nuclear physics. To review the current status of these fields and to begin to assemble the scientific case and the community of researchers for future experiments at the SNS, a work 517 3 $aAstrophysics, symmetries, and applied physics at spallation neutron sources 606 $aNuclear astrophysics$vCongresses 606 $aNuclear physics$vCongresses 606 $aSpallation (Nuclear physics)$vCongresses 606 $aNeutron sources$vCongresses 615 0$aNuclear astrophysics 615 0$aNuclear physics 615 0$aSpallation (Nuclear physics) 615 0$aNeutron sources 676 $a539.7213 701 $aKoehler$b Paul E$g(Paul Edward)$01638893 712 02$aOak Ridge National Laboratory. 712 12$aWorkshop on Astrophysics, Symmetries, and Applied Physics at Spallation Neutron Sources 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910826679403321 996 $aASAP 2002$93981566 997 $aUNINA