ASTROPARTICULAE AND HIGH ENERGY PHYSICS (Q3171083): Difference between revisions

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(‎Changed label, description and/or aliases in en: translated_label)
(‎Removed claim: summary (P836): THE SUCCESS OF THE GREAT HADRON COLLIDER (LHC) AT CERN AND THE RECENT GENERATION OF NEUTRINO EXPERIMENTS HAS LED US TO A GOLDEN AGE OF PARTICLE PHYSICS. IN FACT, BOTH THE RECENT DISCOVERY OF THE HIGGS BOSON AND THE NEUTRINO OSCILLATIONS 15 YEARS AGO HAVE BEEN TWO HISTORIC MILESTONES THAT MARK THE BEGINNING OF A NEW ERA. DRIVEN BY THESE GREAT ACHIEVEMENTS AND THE PROSPECT OF IMPORTANT DISCOVERIES IN THE NEAR FUTURE, THE PARTICLE PHYSICS PREPARE...)
Property / summary
THE SUCCESS OF THE GREAT HADRON COLLIDER (LHC) AT CERN AND THE RECENT GENERATION OF NEUTRINO EXPERIMENTS HAS LED US TO A GOLDEN AGE OF PARTICLE PHYSICS. IN FACT, BOTH THE RECENT DISCOVERY OF THE HIGGS BOSON AND THE NEUTRINO OSCILLATIONS 15 YEARS AGO HAVE BEEN TWO HISTORIC MILESTONES THAT MARK THE BEGINNING OF A NEW ERA. DRIVEN BY THESE GREAT ACHIEVEMENTS AND THE PROSPECT OF IMPORTANT DISCOVERIES IN THE NEAR FUTURE, THE PARTICLE PHYSICS PREPARES THE NEXT STEP. We propose an interdisciplinary research programme for astroparticula and ENERGY ENERGY PHISICATION, CENTRATED IN:_x000D_ _x000D_ 1. PROPERTIES OF NEUTRINOS: Laboratory AND ASTROFISICA_x000D_ the parametres that lead to the oscillations of neutrinos, IN PARTICULARING the CP phase and the heavier hierarchy, shall be determined with the data of the oscillation EXPERIMENTS PROXIMES. We will also analyse subdominant performances due to non-Standard INTERACTIONS, which can provide PISTS ON THE ESCAL OF THE GENERATION OF NEUTRINS MASAS._x000D_ _x000D_ 2. MASSES OF NEUTRINOS: Origin AND CONSEQUENCES_x000D_ we will study THE THEORICAL MODELS OF GENERATION OF THE MOSTS OF the neutrinos, FOR EXAMPLE THAT BASED IN THE SYSTEM OF Discrete SABOR Non-Abelian, as well as their EXPERIMENTAL IMPLICATIONS IN THE LHC AND IN THE VIOLICATION SEARCH OF THE LEPTONIC SABOR AND OF Occupancy MATERIA. We will consider SEE-SAW TYPE schemas as high as low ESCAL, RADIATIVE MODEL ADEMS._x000D_ _x000D_ 3. New PHYSICATE IN THE GREAT Hadron Collider After the DISCOVERMENT OF HIGGS_x000D_ we will investigate the EXTENSIONS OF NEW PHISICAL MORE STANDING, WITH AND WITHOUT supersymetria, with emphasis on the models that can expel observational data on neutrinos. WE WILL STUDY THE SIGNS OF VIOLATION OF THE LEPTONIC NUMBER AND TASTE IN DIFFERENT SCHEMES AND COMPARE THEM WITH FUTURE EXPERIMENTAL DATA. _x000D_ _x000D_ 4. PARTICLE COSMOLOGY: Neutrinos AND MATERIA OSCURA_x000D_ CONSIDERAREMOS ASPECTS OF PARTICULES IN COSMOLOGY, INCLUDING LEPTOGENESIS, MATERIA OSCURA AND INFLACION, IN PARTICULARING their connection with the phisic of neutrinos. WE WILL ANALYSE THE COSMOLOGIC LIMITS TO THE PROPERTIES OF NEUTRINOS, AS THE TOTAL SUM OF THEIR MASSES. With respect to OSCURA MATERIA, we will study the quantities that can be extracted from the DIRECT AND INDIRECTS SEARCHS, as well as LHC DATAs._x000D_ _x000D_ these four lines are interconnected, so that all SENIOR RESEARCHERS will work in more than one TEMA. THE PROPOSED RESEARCH IS MULTIDISCIPLINARY AND COVERS ALL ASPECTS OF THE PHYSICAL SEARCH BEYOND THE STANDARD MODEL, FROM LABORATORY EXPERIMENTS TO MULTIMESSAGE TECHNIQUES IN THE PHYSICS OF ASTROPARTICULA. (English)
 
Property / summary: THE SUCCESS OF THE GREAT HADRON COLLIDER (LHC) AT CERN AND THE RECENT GENERATION OF NEUTRINO EXPERIMENTS HAS LED US TO A GOLDEN AGE OF PARTICLE PHYSICS. IN FACT, BOTH THE RECENT DISCOVERY OF THE HIGGS BOSON AND THE NEUTRINO OSCILLATIONS 15 YEARS AGO HAVE BEEN TWO HISTORIC MILESTONES THAT MARK THE BEGINNING OF A NEW ERA. DRIVEN BY THESE GREAT ACHIEVEMENTS AND THE PROSPECT OF IMPORTANT DISCOVERIES IN THE NEAR FUTURE, THE PARTICLE PHYSICS PREPARES THE NEXT STEP. We propose an interdisciplinary research programme for astroparticula and ENERGY ENERGY PHISICATION, CENTRATED IN:_x000D_ _x000D_ 1. PROPERTIES OF NEUTRINOS: Laboratory AND ASTROFISICA_x000D_ the parametres that lead to the oscillations of neutrinos, IN PARTICULARING the CP phase and the heavier hierarchy, shall be determined with the data of the oscillation EXPERIMENTS PROXIMES. We will also analyse subdominant performances due to non-Standard INTERACTIONS, which can provide PISTS ON THE ESCAL OF THE GENERATION OF NEUTRINS MASAS._x000D_ _x000D_ 2. MASSES OF NEUTRINOS: Origin AND CONSEQUENCES_x000D_ we will study THE THEORICAL MODELS OF GENERATION OF THE MOSTS OF the neutrinos, FOR EXAMPLE THAT BASED IN THE SYSTEM OF Discrete SABOR Non-Abelian, as well as their EXPERIMENTAL IMPLICATIONS IN THE LHC AND IN THE VIOLICATION SEARCH OF THE LEPTONIC SABOR AND OF Occupancy MATERIA. We will consider SEE-SAW TYPE schemas as high as low ESCAL, RADIATIVE MODEL ADEMS._x000D_ _x000D_ 3. New PHYSICATE IN THE GREAT Hadron Collider After the DISCOVERMENT OF HIGGS_x000D_ we will investigate the EXTENSIONS OF NEW PHISICAL MORE STANDING, WITH AND WITHOUT supersymetria, with emphasis on the models that can expel observational data on neutrinos. WE WILL STUDY THE SIGNS OF VIOLATION OF THE LEPTONIC NUMBER AND TASTE IN DIFFERENT SCHEMES AND COMPARE THEM WITH FUTURE EXPERIMENTAL DATA. _x000D_ _x000D_ 4. PARTICLE COSMOLOGY: Neutrinos AND MATERIA OSCURA_x000D_ CONSIDERAREMOS ASPECTS OF PARTICULES IN COSMOLOGY, INCLUDING LEPTOGENESIS, MATERIA OSCURA AND INFLACION, IN PARTICULARING their connection with the phisic of neutrinos. WE WILL ANALYSE THE COSMOLOGIC LIMITS TO THE PROPERTIES OF NEUTRINOS, AS THE TOTAL SUM OF THEIR MASSES. With respect to OSCURA MATERIA, we will study the quantities that can be extracted from the DIRECT AND INDIRECTS SEARCHS, as well as LHC DATAs._x000D_ _x000D_ these four lines are interconnected, so that all SENIOR RESEARCHERS will work in more than one TEMA. THE PROPOSED RESEARCH IS MULTIDISCIPLINARY AND COVERS ALL ASPECTS OF THE PHYSICAL SEARCH BEYOND THE STANDARD MODEL, FROM LABORATORY EXPERIMENTS TO MULTIMESSAGE TECHNIQUES IN THE PHYSICS OF ASTROPARTICULA. (English) / rank
Normal rank
 
Property / summary: THE SUCCESS OF THE GREAT HADRON COLLIDER (LHC) AT CERN AND THE RECENT GENERATION OF NEUTRINO EXPERIMENTS HAS LED US TO A GOLDEN AGE OF PARTICLE PHYSICS. IN FACT, BOTH THE RECENT DISCOVERY OF THE HIGGS BOSON AND THE NEUTRINO OSCILLATIONS 15 YEARS AGO HAVE BEEN TWO HISTORIC MILESTONES THAT MARK THE BEGINNING OF A NEW ERA. DRIVEN BY THESE GREAT ACHIEVEMENTS AND THE PROSPECT OF IMPORTANT DISCOVERIES IN THE NEAR FUTURE, THE PARTICLE PHYSICS PREPARES THE NEXT STEP. We propose an interdisciplinary research programme for astroparticula and ENERGY ENERGY PHISICATION, CENTRATED IN:_x000D_ _x000D_ 1. PROPERTIES OF NEUTRINOS: Laboratory AND ASTROFISICA_x000D_ the parametres that lead to the oscillations of neutrinos, IN PARTICULARING the CP phase and the heavier hierarchy, shall be determined with the data of the oscillation EXPERIMENTS PROXIMES. We will also analyse subdominant performances due to non-Standard INTERACTIONS, which can provide PISTS ON THE ESCAL OF THE GENERATION OF NEUTRINS MASAS._x000D_ _x000D_ 2. MASSES OF NEUTRINOS: Origin AND CONSEQUENCES_x000D_ we will study THE THEORICAL MODELS OF GENERATION OF THE MOSTS OF the neutrinos, FOR EXAMPLE THAT BASED IN THE SYSTEM OF Discrete SABOR Non-Abelian, as well as their EXPERIMENTAL IMPLICATIONS IN THE LHC AND IN THE VIOLICATION SEARCH OF THE LEPTONIC SABOR AND OF Occupancy MATERIA. We will consider SEE-SAW TYPE schemas as high as low ESCAL, RADIATIVE MODEL ADEMS._x000D_ _x000D_ 3. New PHYSICATE IN THE GREAT Hadron Collider After the DISCOVERMENT OF HIGGS_x000D_ we will investigate the EXTENSIONS OF NEW PHISICAL MORE STANDING, WITH AND WITHOUT supersymetria, with emphasis on the models that can expel observational data on neutrinos. WE WILL STUDY THE SIGNS OF VIOLATION OF THE LEPTONIC NUMBER AND TASTE IN DIFFERENT SCHEMES AND COMPARE THEM WITH FUTURE EXPERIMENTAL DATA. _x000D_ _x000D_ 4. PARTICLE COSMOLOGY: Neutrinos AND MATERIA OSCURA_x000D_ CONSIDERAREMOS ASPECTS OF PARTICULES IN COSMOLOGY, INCLUDING LEPTOGENESIS, MATERIA OSCURA AND INFLACION, IN PARTICULARING their connection with the phisic of neutrinos. WE WILL ANALYSE THE COSMOLOGIC LIMITS TO THE PROPERTIES OF NEUTRINOS, AS THE TOTAL SUM OF THEIR MASSES. With respect to OSCURA MATERIA, we will study the quantities that can be extracted from the DIRECT AND INDIRECTS SEARCHS, as well as LHC DATAs._x000D_ _x000D_ these four lines are interconnected, so that all SENIOR RESEARCHERS will work in more than one TEMA. THE PROPOSED RESEARCH IS MULTIDISCIPLINARY AND COVERS ALL ASPECTS OF THE PHYSICAL SEARCH BEYOND THE STANDARD MODEL, FROM LABORATORY EXPERIMENTS TO MULTIMESSAGE TECHNIQUES IN THE PHYSICS OF ASTROPARTICULA. (English) / qualifier
point in time: 12 October 2021
Timestamp+2021-10-12T00:00:00Z
Timezone+00:00
CalendarGregorian
Precision1 day
Before0
After0
 

Revision as of 18:58, 12 October 2021

Project Q3171083 in Spain
Language Label Description Also known as
English
ASTROPARTICULAE AND HIGH ENERGY PHYSICS
Project Q3171083 in Spain

    Statements

    country
    Spain
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    EU contribution
    108,900.0 Euro
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    budget
    217,800.0 Euro
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    co-financing rate
    50.0 percent
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    start time
    1 January 2015
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    end time
    31 December 2017
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    beneficiary name (string)
    AGENCIA CONSEJO SUPERIOR DE INVESTIGACIONES CIENTIFICAS
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    beneficiary
    Q3132561
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    coordinate location

    39°30'14.11"N, 0°26'31.56"W
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    postal code
    46190
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    summary
    EL EXITO DEL GRAN COLISIONADOR DE HADRONES (LHC) EN EL CERN Y DE LA RECIENTE GENERACION DE EXPERIMENTOS DE NEUTRINOS NOS HA CONDUCIDO A UNA EDAD DE ORO DE LA FISICA DE PARTICULAS. DE HECHO, TANTO EL RECIENTE DESCUBRIMIENTO DEL BOSON DE HIGGS COMO EL DE LAS OSCILACIONES DE NEUTRINOS, HACE 15 AÑOS, HAN SIDO DOS HITOS HISTORICOS QUE MARCAN EL PRINCIPIO DE UNA NUEVA ERA. IMPULSADA POR ESTOS GRANDES LOGROS Y POR LA PERSPECTIVA DE IMPORTANTES DESCUBRIMIENTOS EN UN FUTURO PROXIMO, LA FISICA DE PARTICULAS PREPARA EL SIGUIENTE PASO. PROPONEMOS UN PROGRAMA DE INVESTIGACION QUE ABARCA DIVERSOS ASPECTOS INTERDISCIPLINARIOS DE ASTROPARTICULAS Y FISICA DE ALTAS ENERGIAS, CENTRADO EN:_x000D_ _x000D_ 1. PROPIEDADES DE LOS NEUTRINOS: LABORATORIO Y ASTROFISICA_x000D_ LOS PARAMETROS QUE RIGEN LAS OSCILACIONES DE NEUTRINOS, EN PARTICULAR LA FASE CP Y LA JERARQUIA DE MASAS, SE DETERMINARAN CON LOS DATOS DE LOS PROXIMOS EXPERIMENTOS DE OSCILACIONES. ANALIZAREMOS TAMBIEN EFECTOS SUBDOMINANTES DEBIDOS A INTERACCIONES NO ESTANDAR, QUE PUEDEN PROPORCIONAR PISTAS SOBRE LA ESCALA DE LA GENERACION DE LAS MASAS DE LOS NEUTRINOS._x000D_ _x000D_ 2. MASAS DE LOS NEUTRINOS: ORIGEN Y CONSECUENCIAS_x000D_ ESTUDIAREMOS LOS MODELOS TEORICOS DE GENERACION DE LAS MASAS DE LOS NEUTRINOS, POR EJEMPLO AQUELLOS BASADOS EN LAS SIMETRIAS DE SABOR DISCRETAS NO ABELIANAS, ASI COMO SUS IMPLICACIONES EXPERIMENTALES EN EL LHC Y EN LA BUSQUEDA DE VIOLACION DEL SABOR LEPTONICO Y DE MATERIA OSCURA. CONSIDERAREMOS LOS ESQUEMAS DE TIPO SEE-SAW TANTO A ALTA COMO A BAJA ESCALA, ADEMAS DE MODELOS RADIATIVOS._x000D_ _x000D_ 3. NUEVA FISICA EN EL GRAN COLISIONADOR DE HADRONES TRAS EL DESCUBRIMIENTO DEL HIGGS_x000D_ INVESTIGAREMOS LAS EXTENSIONES DE NUEVA FISICA MAS ALLA DEL MODELO ESTANDAR, CON Y SIN SUPERSIMETRIA, CON ENFASIS EN LOS MODELOS QUE PUEDEN EXPLICAR LOS DATOS OBSERVACIONALES SOBRE NEUTRINOS. ESTUDIAREMOS LAS SEÑALES DE VIOLACION DEL NUMERO Y SABOR LEPTONICO EN DIFERENTES ESQUEMAS Y LAS COMPARAREMOS CON FUTUROS DATOS EXPERIMENTALES. _x000D_ _x000D_ 4. COSMOLOGIA DE PARTICULAS: NEUTRINOS Y MATERIA OSCURA_x000D_ CONSIDERAREMOS ASPECTOS DE LA FISICA DE PARTICULAS EN COSMOLOGIA, INCLUYENDO LEPTOGENESIS, MATERIA OSCURA E INFLACION, EN PARTICULAR SU CONEXION CON LA FISICA DE NEUTRINOS. ANALIZAREMOS LOS LIMITES COSMOLOGICOS A LAS PROPIEDADES DE LOS NEUTRINOS, COMO LA SUMA TOTAL DE SUS MASAS. RESPECTO A LA MATERIA OSCURA, ESTUDIAREMOS LAS COTAS QUE PUEDEN EXTRAERSE DE LAS BUSQUEDAS DIRECTAS E INDIRECTAS, ASI COMO DE DATOS DEL LHC._x000D_ _x000D_ ESTAS CUATRO LINEAS ESTAN INTERCONECTADAS, POR LO QUE TODOS LOS INVESTIGADORES SENIOR TRABAJARAN EN MAS DE UN TEMA. LA INVESTIGACION PROPUESTA ES PLURIDISCIPLINAR Y ABARCA TODOS LOS ASPECTOS DE LA BUSQUEDA DE FISICA MAS ALLA DEL MODELO ESTANDAR, DESDE EXPERIMENTOS DE LABORATORIO HASTA TECNICAS DE MULTIMENSAJEROS EN LA FISICA DE ASTROPARTICULAS. (Spanish)
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    location (string)
    Paterna
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    Identifiers

    Spanish Kohesio ID
    FPA2014-58183-P
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