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PHENOMENOLOGY at the LHC,COSMIC RAYS and their COSMOLOGICAL IMPLICATIONS

PHENOMENOLOGY at the LHC,COSMIC RAYS and their COSMOLOGICAL IMPLICATIONS. High Density matter Cosmic Rays showers and   Flux Non linear field theory and cosmological implications. High Density Matter.

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PHENOMENOLOGY at the LHC,COSMIC RAYS and their COSMOLOGICAL IMPLICATIONS

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  1. PHENOMENOLOGY at theLHC,COSMIC RAYS and theirCOSMOLOGICALIMPLICATIONS High Density matter Cosmic Rays showers and Flux Non linear field theory and cosmological implications

  2. High Density Matter • _Supression of high pt in AA,and the dissapearence of back to back jet correlations.Detailed study of heavy flavour supression(predicted less supression due to dead cone).Modification of jet properties (momentum,and multiplicity distributions) due to medium.Properties of the medium(collaboration with Frascati group of ALICE)

  3. Discussion onincoming LHC data on AA and pp and predictions of CGC and string percolation(multiplicity,elliptical flow,B/M, Cronin effect,heavy flavour).J supression Study of strong color fields and saturation of partons(new QCD scale,Qs )Interplay between pQCD and npQCD Correlations(rapidity long range correlations,SB,) critical point,FAIR

  4. COSMIC RAYS SHOWERS and  FLUX Parton saturation effects in atmospheric showers,studying the distribution of the shower depth of maximum and the number of muons(an excess is seen in Auger) Behaviour of F2 at low x due to saturation and its consequences on the detection of the  flux due toτ energy loss produced by photonuclear interactions and to the charged current V-Across section

  5. Non linear field theory and phenomenological implications Application of integrability methods for the description of the gluon sector.Glueballs Analysis of field theories with non standard kinetic terms,useful to describe cosmological scenarios,at AA collisions at LHC(negative pressure,elliptical flow). Relevance of the special kinetic terms in the presence of intense black holes of AGN.

  6. Researchers • High density matter. Cu C.Pajares;Tu C.Merino;RyC N.Armesto,E.G.Ferreiro C.A.Salgado Doct P.Quiroga Otras Instituciones:M.A.Braun,J.Dias de Deus,J.G.Milhano J.Lopez Albacete,J.Casalderrey,Y.Shabelski Cosmic Rays Showers and  Flux Cu E.Zas Tu G.Parente,R.Vazquez;RyCJ.Alvarez Muñiz Cu C.Pajares;Tu C.Merino;RyC N.Armesto;O.I J.Dias Deus Non Linear Field Theory and Cosm Impl Cu J.Sanchez Guillen,J.L.MiramontesTu R.Vazquez,RyC(equivalent) C.Adam,O.I L.A.Ferreira,P.Klimas

  7. REQUIREMENTS • Personal 448250eu 3 postdocx24 months =228000eu visitors(4x1monthx5years) =32000eu administration(13500x5y) = 67500eu complements(2100x11.5x5)=120750eu ---------------------------------------------------------- Equipement(Pc,software,…) = 18500eu Travels 140000eu Various 30000eu --------------- 188500eu TOTAL 636750eu

  8. SUMMARY Cosmic Rays Showers Showers at UHE (Alvarez, Pajares) Low x,  Flux (Zas, Parente, Vazquez, Merino, Armesto) 1 postdoc, visitor, computer resources Supression of high pT (Armesto, Salgado, Ferreiro, Quiroga, Pajares) Correlations, J supression Ferreiro, Pajares, Armesto 1 postdoc, visitors, computer resources Integrability methods in gluon sector Sánchez Guillen, Miramontes Special Kinetic Terms and cosmology Sánchez Guillén, Vázquez, Adam 1 postdoc, visitors

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