PDF-Baryon Spectrum in Neutrinoinduced Reactions

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Luis Alvarez Ruso NSTAR 2019 L AlvarezRusoIFIC NSTAR2019 IntroductionNeutrinointe

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Baryon Spectrum in Neutrinoinduced Reactions: Transcript


Luis Alvarez Ruso NSTAR 2019 L AlvarezRusoIFIC NSTAR2019 IntroductionNeutrinointe. in heavy baryons. Atsushi . Hosaka.  . (RCNP, Osaka U.. ). 9/10-13, 2013. Charmed baryons. 1. Practical questions of hadron physics. • How ground and excited states are described?. • Are there simple language for it . Nucleosynthesis. :. The Primordial Lithium Problem. Matthew von Hippel. 1. Outline. What is Big Bang . Nucleosyntheis. ?. How does it work?. How can we check it?. The Primordial Lithium Problem. Problem or problem?. Baryon Number Fluctuations. in Heavy Ion Collisions. Masakiyo. Kitazawa. (Osaka U.). MK, M. . Asakawa. , arXiv:1107.2755[. nucl-th. ]. Energy Scan Program @ RHIC. . T. 0. Hadrons. Color SC. m. high. . . Bao-Xi SUN. (. 孙宝玺. ). Beijing University of Technology. . . Hirschegg 2014. Hadrons from Quarks and Gluons,. Jan. 12-18, 2014 . from Continuum-QCD. Craig . D. Roberts. Physics Division. Argonne National . Laboratory. &. School . of Physics. Peking . University. Q. C. D. ’s Challenges. Dynamical . Chiral. Symmetry Breaking. Radiation-Dominated Jet?. Kunihito. . Ioka. (KEK). T. Inoue, Asano & KI, . arXiv. : 1011.6350. KI. , . arXiv. : 1006.3073. Suwa. & KI, . arXiv. : 1009.6001. KI+, in . preparation (. GeV. Photon Delay. Kunihito. . Ioka. (KEK). Contents. Very High Lorentz Factor (VHLF). G. max. can be up to ~10. 6. (> . G. max,. conv. ~10. 3. ). Internal Shock Synchrotron. ⇒ Power-law component over >7 decades. Elementary Particles 4. 1.6 STRANGE PARTICLES (1 947-1 960). For a brief period in 1947 it was possible to believe that the major problems . of elementary . particle physics were solved.. . After a . keyparameter:baryon-to-photonratiolithiumproblem miguelpato(tumunich)prl109,021102(2012) 1.thelithiumproblembigbangnucleosynthesissynthesisoflightelementsintheearlyuniverse keyparameter:baryon-to-pho Ming Sun . (University of Virginia). ‏. M. . Voit, M. Donahue . (. MSU. ). . A. Vikhlinin, W. . Forman, . C. . . Jones (. CfA. ) . N. Sehgal (. KIPAC. ) . C. . Sarazin (. Virginia. ). Groups? Why . FIRE . Tracing . Cosmic Inflows, Galactic Outflows, and . Gas . Recycling in Realistic Environments. Daniel . Anglés-Alcázar. CIERA Postdoctoral Fellow. C. enter for . I. nterdisciplinary. . E. xploration and . Robert Edwards . Jefferson Lab. N. *. @ high . Q. 2. , 2011. TexPoint. fonts used in EMF. . Read the TexPoint manual before you delete this box.: . A. A. A. A. A. A. A. A. A. A. A. A. A. A. A. Collaborators:. INFN-LNS. Modelli. . Idrodinamici. e . di . Ricombinazione. . con . p. T. . spettri. e v. 2. at LHC. ?. V. . Minissale. F. . Scardina. S. . Plumari. . Brief Introduction to basic idea of coalescence. Chen . Chen. University of Giessen. Diquark. Correlations in . Hadron. Physics: . Origin, Impact and Evidence. 23-27 September 2019. ECT*. Hadrons, as bound states, are dominated by non-. perturbative.

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