Innovating Works

FIS2011-24924

Financiado
GRAVEDAD, TEORIAS GAUGE Y SUPERGRAVEDAD, ASTROPARTICULAS Y COSMOLOGIA.
IN THE LAST YEARS, THERE HAS BEEN A GROWING INTERACTION BETWEEN PARTICLE PHYSICS, ASTROPHYSICS AND COSMOLOGY. THE THEORETICAL INTEREST LIES IN THE POTENTIAL FOR PARTICLE PHYSICS IDEAS AND TECHNIQUES TO EXPLAIN SOME OF THE PROBLEMS... IN THE LAST YEARS, THERE HAS BEEN A GROWING INTERACTION BETWEEN PARTICLE PHYSICS, ASTROPHYSICS AND COSMOLOGY. THE THEORETICAL INTEREST LIES IN THE POTENTIAL FOR PARTICLE PHYSICS IDEAS AND TECHNIQUES TO EXPLAIN SOME OF THE PROBLEMS OF COSMOLOGY AND THE POTENTIAL FOR ASTROPHYSICAL AND COSMOLOGICAL OBSERVATIONS TO CONSTRAIN IDEAS IN PARTICLE PHYSICS. IN SOME AREAS, THE CONNECTION BETWEEN PARTICLE PHYSICS, COSMOLOGY AND ASTROPHYSICS HAS BECOME INCREASINGLY PRECISE. GRAVITY MODELS BASED ON SUPERSYMMETRIC MODELS OF PARTICLE PHYSICS HAVE IMPORTANT OBSERVATIONAL CONSEQUENCES BOTH FOR DARK MATTER AND ENERGY. THE PARAMETERS OF THESE MODELS CAN BE CONSTRAINED BY THE CURRENT EXPERIMENTAL AND OBSERVATIONAL DATA. THIS RESEARCH PROJECT WILL EXPLORE AND EXPLOIT THESE CONNECTIONS.THIS PROJECT CONCENTRATES THE RESEARCH IN GRAVITY, HIGH ENERGY AND ASTROPARTICLE PHYSICS, OF THE MEMBERS OF THE RESEARCH GROUP OF THE UNIVERSIDAD DE MURCIA FISPAC (``FISICA DE PARTICULAS, ASTROFISICA Y COSMOLOGIA''). IT HAS THREE MAIN PARTS CORRESPONDING TO THE INDIVIDUAL LINES OF RESEARCH OF THE MEMBERS WITH INTERRELATIONS AMONG THEM. ONE OF THESE LINES OF RESEARCH IS NEW TO OUR GROUP AND CORRESPONDS TO THE ACTIVITIES OF A NEW RAMON Y CAJAL MEMBER. THE MAIN SCIENTIFIC GOALS OF THIS PROJECT ARE THE STUDY OF THE FOLLOWING ASPECTS: A) GRAVITY, SUPERGRAVITY AND DARK ENERGY. THE PROJECT AIMS TO GAIN FURTHER INSIGHTS INTO THE FUNDAMENTAL STRUCTURE OF THE UNIVERSE, NAMELY ITS BASIC CONSTITUENTS, THE FORCES MUTUALLY ACTING AMONG THEM AND THE SYMMETRIES WHICH UNDERLIE ITS THEORETICAL DESCRIPTION. CLASSIFICATION AND SEARCH OF NEW GAUGED SUPERGRAVITY THEORIES AND TO EXPLORE THE RELATION BETWEEN SUPERGRAVITY AND GAUGE FORCES. B) GAMMA RAY ASTROPARTICLE PHYSICS.THE MAIN PHYSICAL OBJECTIVES HERE ARE:(I) STUDY OF SOURCES IN HIGH ENERGY ASTRONOMY: ACTIVE GALACTIC NUCLEI, NEUTRON STARS, OTHER COMPACT OBJECTS ANDASTROPARTICLES.(II) HIGH ENERGY PHYSICS ASTRONOMY: X RAYS AND GAMMA RAYS OF HIGHENERGY (E > 10 GEV). C) NEUTRON STARS AS LABORATORIES OF EXTREME PHYSICS. GRAVITY WAVES. THIS PROPOSAL IS DESIGNED TO MEET SOME MAJOR CHALLENGES ASSOCIATED WITH THE MODELLING OF REALISTIC NEUTRON STAR PHYSICS. IT DRAWS ON EXPERTISE FROM A RANGE OF SPECIALIST DISCIPLINES, INCLUDING HIGH-ENERGY AND NUCLEAR PHYSICS, LOW-TEMPERATURE PHYSICS, GRAVITATIONAL PHYSICS AND TRADITIONAL ASTROPHYSICS. THE OVERALL OBJECTIVE IS TO PROVIDE RELIABLE THEORETICAL MODELS AND FACILITATE QUANTITATIVE COMPARISONS WITH EXISTING AND FUTURE HIGH-QUALITY OBSERVATIONS. RAVITACION\MATERIA OSCURA.\SUPERSIMETRIA\TEORIAS GAUGE ver más
01/01/2011
UM
44K€
Perfil tecnológico estimado

Línea de financiación: concedida

El organismo AGENCIA ESTATAL DE INVESTIGACIÓN notifico la concesión del proyecto el día 2011-01-01
Presupuesto El presupuesto total del proyecto asciende a 44K€
Líder del proyecto
UNIVERSIDAD DE MURCIA No se ha especificado una descripción o un objeto social para esta compañía.
Total investigadores 912