PPT-Baryon content of galaxy groups

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 . mode of . accretion. in . simulations. of . galaxy. . formation. G. Murante – INAF . OATo. P. Monaco – . Univ. . . Ts. M. Calabrese – SISSA . Ts. G. De Lucia - INAF . OATs. S. . Borgani. – . 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. D.J. Pisano. (West Virginia University). Why study galaxy environment?. Nature vs. Nurture. Can they be distinguished?. What does the environment do to a galaxy?. What would a galaxy look like without any environmental influence?. . . Bao-Xi SUN. (. 孙宝玺. ). Beijing University of Technology. . . Hirschegg 2014. Hadrons from Quarks and Gluons,. Jan. 12-18, 2014 . 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. galaxy group, Stephan 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 Eleonora Babayants, MLS. Information Overload and How to Deal With It. Galaxy Consulting . www.galaxyconsulting.net. Information is the oxygen of the modern age. It seeps through the walls topped by barbed wire, it wafts across the electrified borders. - . 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. in . simulations. of . galaxy. . formation. G. Murante – INAF . OATo. P. Monaco – . Univ. . . Ts. M. Calabrese – SISSA . Ts. G. De Lucia - INAF . OATs. S. . Borgani. – . Univ. . . Ts. K. .