Q3171924 (Q3171924): Difference between revisions
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(Created claim: summary (P836): OUR WORK FOCUSES ON DYNAMICS AND RADIATION EMITTED DURING THE COLLISION OF NEUTRON STARS. THE RECENT DETECTION OF GRAVITATIONAL WAVES (OG) THROUGH INTERFEROMETRIC OBSERVATORIES OPENS A NEW WINDOW TO STUDY SOME OF THE MOST ENERGETIC PHENOMENA THAT OCCUR IN THE UNIVERSE. ONE OF THE MOST OUTSTANDING CANDIDATES FOR THE GENERATION OF STRONG OG IS THE CLASH OF NEUTRON STARS, WHICH CAN BE CONSIDERED AS AN ASTROPHYSICIC LABORATORY TO STUDY GRAVITY, PLAS...) |
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OUR WORK FOCUSES ON DYNAMICS AND RADIATION EMITTED DURING THE COLLISION OF NEUTRON STARS. THE RECENT DETECTION OF GRAVITATIONAL WAVES (OG) THROUGH INTERFEROMETRIC OBSERVATORIES OPENS A NEW WINDOW TO STUDY SOME OF THE MOST ENERGETIC PHENOMENA THAT OCCUR IN THE UNIVERSE. ONE OF THE MOST OUTSTANDING CANDIDATES FOR THE GENERATION OF STRONG OG IS THE CLASH OF NEUTRON STARS, WHICH CAN BE CONSIDERED AS AN ASTROPHYSICIC LABORATORY TO STUDY GRAVITY, PLASMA PHYSICS AND NUCLEAR PHYSICS IN ITS MOST EXTREME CONDITIONS. SIMULTANEAS OF THE GRAVITACIONAL AND Electromagnetic ONDAS (MS) PRODUCTED by these sources will initiate a MULTI-MESSAGE ASTRONOMY ERA that will improve not only our understanding of the SYSTEM parametres and of the involucrated physical processes, if they do not allow us to demolish our theories and carry out our ASTROPHIC models._x000D_ PROPOSES A PROJECT based on the statistics of the BINARY SYSTEM COLISIONS OF NEUTRONS MEDIANING SYSTEMS Numerical SYSTEMS, the RADIATION that these SYSTEMS emit (EM, OG Y, POSIBLEMENTLY, TRAVES OF neutrinos). WE WILL FOCUS ON DISCOVERING THE MOST RELEVANT PHYSICAL MECHANISMS TO DESCRIBE THIS DYNAMIC, AND IN WHICH CONDITIONS THESE COLLISIONS COULD GIVE RISE TO EM OBSERVABLE SIGNALS, SUCH AS EMISSIONS OF RAYS-GAMMA (RG) AND KILONOVAE. OUR PLAN IS TO INTRODUCE NEW TECHNIQUES AND APPROACHES TO DEAL WITH CHALLENGES RELATED TO THE EVOLUTION OF MAGNETIC FIELDS AND NEUTRINOS, AS WELL AS TO INVESTIGATE THEIR ROLE IN THE PRODUCTION OF PARTICLE JETS (JETS) — WHICH GIVE RISE TO GAMMA RAFFLES (GRB) — AND THE EVOLUTION OF THE MATTER EXPELLED DURING THE COLLISION — WHICH MAY GIVE RISE TO KILONOVAS. THESE NUMERICAL SIMULATIONS ARE COMPUTATIONALLY EXPENSIVE, SO TO COVER ALL POSSIBLE CONFIGURATIONS OF THE PARAMETER SPACE WE WILL NEED TO OPTIMISE OUR CODES AND OVERCOME THE CURRENT LIMITATIONS IN SCALABILITY. WE HOPE THAT THE COMPARISON OF EM AND OG EMISSION MAPS (OBTAINED ON THE ONE HAND FROM THE NUMERICAL CALCULATIONS WE PROPOSE, AND ON THE OTHER HAND FROM FUTURE OBSERVATIONS) WILL SIGNIFICANTLY ADVANCE OUR KNOWLEDGE OF GRAVITATIONAL, NUCLEAR AND PLASMA PHYSICS. It is important to highlight that this multi-digital programme is linked to the first OG DETECTIONS and we will allow the SCIENTIFIC RESULT OF DATA FACILITED BY NEW GRAVITATORY ONDS DETECTORS._x000D_Our numeral SIMULATIONS OF BINARY SYSTEMS the CODIGO HAD, an open INFRASTRUCTURE that in the current situation may be able to resolve re-examination of magnetohidrodinemic effluents with funds repressed by REALIST ECUACIONES and with a staiming of the effectiveness of the neutrinos, and (2) SIMFLOWNY, a body based on the roof for scientific dynamic models with small multiples, composing for a specific semantic language and an integrated development environment for use, which automatically manages the parallel code for SIMULACION frameworks. THE RESULTING CODE WILL INCLUDE ALL THE MAIN BASIC INGREDIENTS (I.E. STRONG GRAVITY, MAGNETIC FIELDS AND NEUTRINOS) TO SYSTEMATICALLY STUDY THE PRODUCTION OF JETS IN THESE SCENARIOS AND THE EVOLUTION OF THE MATERIAL EXPELLED DURING THE COLLISION. (English) | |||||||||||||||
| Property / summary: OUR WORK FOCUSES ON DYNAMICS AND RADIATION EMITTED DURING THE COLLISION OF NEUTRON STARS. THE RECENT DETECTION OF GRAVITATIONAL WAVES (OG) THROUGH INTERFEROMETRIC OBSERVATORIES OPENS A NEW WINDOW TO STUDY SOME OF THE MOST ENERGETIC PHENOMENA THAT OCCUR IN THE UNIVERSE. ONE OF THE MOST OUTSTANDING CANDIDATES FOR THE GENERATION OF STRONG OG IS THE CLASH OF NEUTRON STARS, WHICH CAN BE CONSIDERED AS AN ASTROPHYSICIC LABORATORY TO STUDY GRAVITY, PLASMA PHYSICS AND NUCLEAR PHYSICS IN ITS MOST EXTREME CONDITIONS. SIMULTANEAS OF THE GRAVITACIONAL AND Electromagnetic ONDAS (MS) PRODUCTED by these sources will initiate a MULTI-MESSAGE ASTRONOMY ERA that will improve not only our understanding of the SYSTEM parametres and of the involucrated physical processes, if they do not allow us to demolish our theories and carry out our ASTROPHIC models._x000D_ PROPOSES A PROJECT based on the statistics of the BINARY SYSTEM COLISIONS OF NEUTRONS MEDIANING SYSTEMS Numerical SYSTEMS, the RADIATION that these SYSTEMS emit (EM, OG Y, POSIBLEMENTLY, TRAVES OF neutrinos). WE WILL FOCUS ON DISCOVERING THE MOST RELEVANT PHYSICAL MECHANISMS TO DESCRIBE THIS DYNAMIC, AND IN WHICH CONDITIONS THESE COLLISIONS COULD GIVE RISE TO EM OBSERVABLE SIGNALS, SUCH AS EMISSIONS OF RAYS-GAMMA (RG) AND KILONOVAE. OUR PLAN IS TO INTRODUCE NEW TECHNIQUES AND APPROACHES TO DEAL WITH CHALLENGES RELATED TO THE EVOLUTION OF MAGNETIC FIELDS AND NEUTRINOS, AS WELL AS TO INVESTIGATE THEIR ROLE IN THE PRODUCTION OF PARTICLE JETS (JETS) — WHICH GIVE RISE TO GAMMA RAFFLES (GRB) — AND THE EVOLUTION OF THE MATTER EXPELLED DURING THE COLLISION — WHICH MAY GIVE RISE TO KILONOVAS. THESE NUMERICAL SIMULATIONS ARE COMPUTATIONALLY EXPENSIVE, SO TO COVER ALL POSSIBLE CONFIGURATIONS OF THE PARAMETER SPACE WE WILL NEED TO OPTIMISE OUR CODES AND OVERCOME THE CURRENT LIMITATIONS IN SCALABILITY. WE HOPE THAT THE COMPARISON OF EM AND OG EMISSION MAPS (OBTAINED ON THE ONE HAND FROM THE NUMERICAL CALCULATIONS WE PROPOSE, AND ON THE OTHER HAND FROM FUTURE OBSERVATIONS) WILL SIGNIFICANTLY ADVANCE OUR KNOWLEDGE OF GRAVITATIONAL, NUCLEAR AND PLASMA PHYSICS. It is important to highlight that this multi-digital programme is linked to the first OG DETECTIONS and we will allow the SCIENTIFIC RESULT OF DATA FACILITED BY NEW GRAVITATORY ONDS DETECTORS._x000D_Our numeral SIMULATIONS OF BINARY SYSTEMS the CODIGO HAD, an open INFRASTRUCTURE that in the current situation may be able to resolve re-examination of magnetohidrodinemic effluents with funds repressed by REALIST ECUACIONES and with a staiming of the effectiveness of the neutrinos, and (2) SIMFLOWNY, a body based on the roof for scientific dynamic models with small multiples, composing for a specific semantic language and an integrated development environment for use, which automatically manages the parallel code for SIMULACION frameworks. THE RESULTING CODE WILL INCLUDE ALL THE MAIN BASIC INGREDIENTS (I.E. STRONG GRAVITY, MAGNETIC FIELDS AND NEUTRINOS) TO SYSTEMATICALLY STUDY THE PRODUCTION OF JETS IN THESE SCENARIOS AND THE EVOLUTION OF THE MATERIAL EXPELLED DURING THE COLLISION. (English) / rank | |||||||||||||||
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| Property / summary: OUR WORK FOCUSES ON DYNAMICS AND RADIATION EMITTED DURING THE COLLISION OF NEUTRON STARS. THE RECENT DETECTION OF GRAVITATIONAL WAVES (OG) THROUGH INTERFEROMETRIC OBSERVATORIES OPENS A NEW WINDOW TO STUDY SOME OF THE MOST ENERGETIC PHENOMENA THAT OCCUR IN THE UNIVERSE. ONE OF THE MOST OUTSTANDING CANDIDATES FOR THE GENERATION OF STRONG OG IS THE CLASH OF NEUTRON STARS, WHICH CAN BE CONSIDERED AS AN ASTROPHYSICIC LABORATORY TO STUDY GRAVITY, PLASMA PHYSICS AND NUCLEAR PHYSICS IN ITS MOST EXTREME CONDITIONS. SIMULTANEAS OF THE GRAVITACIONAL AND Electromagnetic ONDAS (MS) PRODUCTED by these sources will initiate a MULTI-MESSAGE ASTRONOMY ERA that will improve not only our understanding of the SYSTEM parametres and of the involucrated physical processes, if they do not allow us to demolish our theories and carry out our ASTROPHIC models._x000D_ PROPOSES A PROJECT based on the statistics of the BINARY SYSTEM COLISIONS OF NEUTRONS MEDIANING SYSTEMS Numerical SYSTEMS, the RADIATION that these SYSTEMS emit (EM, OG Y, POSIBLEMENTLY, TRAVES OF neutrinos). WE WILL FOCUS ON DISCOVERING THE MOST RELEVANT PHYSICAL MECHANISMS TO DESCRIBE THIS DYNAMIC, AND IN WHICH CONDITIONS THESE COLLISIONS COULD GIVE RISE TO EM OBSERVABLE SIGNALS, SUCH AS EMISSIONS OF RAYS-GAMMA (RG) AND KILONOVAE. OUR PLAN IS TO INTRODUCE NEW TECHNIQUES AND APPROACHES TO DEAL WITH CHALLENGES RELATED TO THE EVOLUTION OF MAGNETIC FIELDS AND NEUTRINOS, AS WELL AS TO INVESTIGATE THEIR ROLE IN THE PRODUCTION OF PARTICLE JETS (JETS) — WHICH GIVE RISE TO GAMMA RAFFLES (GRB) — AND THE EVOLUTION OF THE MATTER EXPELLED DURING THE COLLISION — WHICH MAY GIVE RISE TO KILONOVAS. THESE NUMERICAL SIMULATIONS ARE COMPUTATIONALLY EXPENSIVE, SO TO COVER ALL POSSIBLE CONFIGURATIONS OF THE PARAMETER SPACE WE WILL NEED TO OPTIMISE OUR CODES AND OVERCOME THE CURRENT LIMITATIONS IN SCALABILITY. WE HOPE THAT THE COMPARISON OF EM AND OG EMISSION MAPS (OBTAINED ON THE ONE HAND FROM THE NUMERICAL CALCULATIONS WE PROPOSE, AND ON THE OTHER HAND FROM FUTURE OBSERVATIONS) WILL SIGNIFICANTLY ADVANCE OUR KNOWLEDGE OF GRAVITATIONAL, NUCLEAR AND PLASMA PHYSICS. It is important to highlight that this multi-digital programme is linked to the first OG DETECTIONS and we will allow the SCIENTIFIC RESULT OF DATA FACILITED BY NEW GRAVITATORY ONDS DETECTORS._x000D_Our numeral SIMULATIONS OF BINARY SYSTEMS the CODIGO HAD, an open INFRASTRUCTURE that in the current situation may be able to resolve re-examination of magnetohidrodinemic effluents with funds repressed by REALIST ECUACIONES and with a staiming of the effectiveness of the neutrinos, and (2) SIMFLOWNY, a body based on the roof for scientific dynamic models with small multiples, composing for a specific semantic language and an integrated development environment for use, which automatically manages the parallel code for SIMULACION frameworks. THE RESULTING CODE WILL INCLUDE ALL THE MAIN BASIC INGREDIENTS (I.E. STRONG GRAVITY, MAGNETIC FIELDS AND NEUTRINOS) TO SYSTEMATICALLY STUDY THE PRODUCTION OF JETS IN THESE SCENARIOS AND THE EVOLUTION OF THE MATERIAL EXPELLED DURING THE COLLISION. (English) / qualifier | |||||||||||||||
point in time: 12 October 2021
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Revision as of 18:28, 12 October 2021
Project Q3171924 in Spain
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | No label defined |
Project Q3171924 in Spain |
Statements
68,970.0 Euro
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137,940.0 Euro
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50.0 percent
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30 December 2016
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31 December 2020
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UNIVERSIDAD DE LAS ISLAS BALEARES
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39°34'10.49"N, 2°39'0.25"E
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07040
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NUESTRO TRABAJO SE CENTRA EN LA DINAMICA Y LA RADIACION EMITIDA DURANTE LA COLISION DE ESTRELLAS DE NEUTRONES. LA RECIENTE DETECCION DE ONDAS GRAVITACIONALES (OG) A TRAVES DE LOS OBSERVATORIOS INTERFEROMETRICOS ABRE UNA NUEVA VENTANA PARA ESTUDIAR ALGUNOS DE LOS FENOMENOS MAS ENERGETICOS QUE OCURREN EN EL UNIVERSO. UNO DE LOS CANDIDATOS MAS DESTACADOS PARA LA GENERACION DE FUERTES OG ES EL CHOQUE DE ESTRELLAS DE NEUTRONES, QUE SE PUEDE CONSIDERAR COMO UN LABORATORIO ASTROFISICO PARA ESTUDIAR GRAVEDAD, FISICA DE PLASMAS Y FISICA NUCLEAR EN SUS CONDICIONES MAS EXTREMAS. OBSERVACIONES SIMULTANEAS DE LAS ONDAS GRAVITACIONALES Y ELECTROMAGNETICAS (EM) PRODUCIDAS POR ESTAS FUENTES INICIARAN UNA ERA DE ASTRONOMIA DE MULTI-MENSAJEROS QUE MEJORARA NO SOLO NUESTRA COMPRENSION DE LOS PARAMETROS DEL SISTEMA Y DE LOS PROCESOS FISICOS INVOLUCRADOS, SINO QUE TAMBIEN NOS PERMITIRA DEMOSTRAR NUESTRAS TEORIAS Y VALIDAR NUESTROS MODELOS ASTROFISICOS._x000D_ PROPONEMOS UN PROYECTO BASADO EN EL ESTUDIO DE LAS COLISIONES DE SISTEMAS BINARIOS DE ESTRELLAS DE NEUTRONES MEDIANTE SIMULACIONES NUMERICAS, ESTIMANDO ADEMAS LA RADIACION QUE EMITEN ESTOS SISTEMAS (EM, OG Y, POSIBLEMENTE, A TRAVES DE NEUTRINOS). NOS CENTRAREMOS EN DESCUBRIR LOS MECANISMOS FISICOS MAS RELEVANTES PARA DESCRIBIR DICHA DINAMICA, Y EN QUE CONDICIONES ESTAS COLISIONES PODRIAN DAR LUGAR A SEÑALES EM OBSERVABLES, COMO EMISIONES DE RAYOS-GAMMA (RG) Y KILONOVAS. NUESTRO PLAN ES INTRODUCIR NUEVAS TECNICAS Y ENFOQUES PARA HACER FRENTE A LOS DESAFIOS RELACIONADOS CON LA EVOLUCION DE LOS CAMPOS MAGNETICOS Y LOS NEUTRINOS, ASI COMO PARA INVESTIGAR SU PAPEL EN LA PRODUCCION DE CHORROS DE PARTICULAS (JETS) -QUE DAN LUGAR A RAFAGAS DE RAYOS GAMMA (GRB)- Y LA EVOLUCION DE LA MATERIA EXPULSADA DURANTE LA COLISION -QUE PUEDE DAR LUGAR A KILONOVAS-. ESTAS SIMULACIONES NUMERICAS SON COMPUTACIONALMENTE COSTOSAS, POR LO QUE PARA CUBRIR TODAS LAS POSIBLES CONFIGURACIONES DEL ESPACIO DE PARAMETROS NECESITAREMOS OPTIMIZAR NUESTROS CODIGOS Y SUPERAR LAS LIMITACIONES ACTUALES EN LA ESCALABILIDAD. ESPERAMOS QUE LA COMPARACION DE LOS MAPAS DE EMISIONES DE EM Y OG (OBTENIDOS POR UN LADO A PARTIR DE LOS CALCULOS NUMERICOS QUE PROPONEMOS, Y POR EL OTRO DE FUTURAS OBSERVACIONES) AVANZARA SIGNIFICATIVAMENTE NUESTRO CONOCIMIENTO DE LA FISICA GRAVITACIONAL, NUCLEAR Y DE PLASMAS. ES IMPORTANTE RESALTAR QUE ESTE PROGRAMA MULTIDISCIPLINARIO COINCIDE CON LAS PRIMERAS DETECCIONES DE OG Y NOS PERMITIRA MAXIMIZAR EL RESULTADO CIENTIFICO DE LOS DATOS FACILITADOS POR LOS NUEVOS DETECTORES DE ONDAS GRAVITATORIAS._x000D_ NUESTRAS SIMULACIONES NUMERICAS DE SISTEMAS BINARIOS DE ESTRELLA DE NEUTRONES SE LLEVARAN A CABO MEDIANTE EL ACOPLAMIENTO DE FORMA SINERGICA (1) EL CODIGO HAD, UNA INFRAESTRUCTURA ABIERTA QUE EN LA ACTUALIDAD PUEDE RESOLVER ECUACIONES DE MAGNETOHIDRODINAMICA RELATIVISTA CON FLUIDOS REPRESENTADOS POR ECUACIONES DE ESTADO REALISTAS Y CON UNA ESTIMACION DEL EFECTO DE LOS NEUTRINOS, Y (2) SIMFLOWNY, UN ENTORNO BASADO EN LA NUBE PARA MODELOS DINAMICOS CIENTIFICOS CON MULTIPLES ESCALAS, COMPUESTA POR UN LENGUAJE SEMANTICO ESPECIFICO Y UN ENTORNO DE DESARROLLO INTEGRADO FACIL DE USAR, QUE GENERA AUTOMATICAMENTE EL CODIGO PARALELO PARA MARCOS DE SIMULACION. EL CODIGO RESULTANTE INCLUIRA TODOS LOS PRINCIPALES INGREDIENTES BASICOS (ES DECIR, GRAVEDAD FUERTE, CAMPOS MAGNETICOS Y NEUTRINOS) PARA ESTUDIAR SISTEMATICAMENTE LA PRODUCCION DE JETS EN ESTOS ESCENARIOS Y LA EVOLUCION DEL MATERIAL EXPULSADO DURANTE LA COLISION. (Spanish)
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OUR WORK FOCUSES ON DYNAMICS AND RADIATION EMITTED DURING THE COLLISION OF NEUTRON STARS. THE RECENT DETECTION OF GRAVITATIONAL WAVES (OG) THROUGH INTERFEROMETRIC OBSERVATORIES OPENS A NEW WINDOW TO STUDY SOME OF THE MOST ENERGETIC PHENOMENA THAT OCCUR IN THE UNIVERSE. ONE OF THE MOST OUTSTANDING CANDIDATES FOR THE GENERATION OF STRONG OG IS THE CLASH OF NEUTRON STARS, WHICH CAN BE CONSIDERED AS AN ASTROPHYSICIC LABORATORY TO STUDY GRAVITY, PLASMA PHYSICS AND NUCLEAR PHYSICS IN ITS MOST EXTREME CONDITIONS. SIMULTANEAS OF THE GRAVITACIONAL AND Electromagnetic ONDAS (MS) PRODUCTED by these sources will initiate a MULTI-MESSAGE ASTRONOMY ERA that will improve not only our understanding of the SYSTEM parametres and of the involucrated physical processes, if they do not allow us to demolish our theories and carry out our ASTROPHIC models._x000D_ PROPOSES A PROJECT based on the statistics of the BINARY SYSTEM COLISIONS OF NEUTRONS MEDIANING SYSTEMS Numerical SYSTEMS, the RADIATION that these SYSTEMS emit (EM, OG Y, POSIBLEMENTLY, TRAVES OF neutrinos). WE WILL FOCUS ON DISCOVERING THE MOST RELEVANT PHYSICAL MECHANISMS TO DESCRIBE THIS DYNAMIC, AND IN WHICH CONDITIONS THESE COLLISIONS COULD GIVE RISE TO EM OBSERVABLE SIGNALS, SUCH AS EMISSIONS OF RAYS-GAMMA (RG) AND KILONOVAE. OUR PLAN IS TO INTRODUCE NEW TECHNIQUES AND APPROACHES TO DEAL WITH CHALLENGES RELATED TO THE EVOLUTION OF MAGNETIC FIELDS AND NEUTRINOS, AS WELL AS TO INVESTIGATE THEIR ROLE IN THE PRODUCTION OF PARTICLE JETS (JETS) — WHICH GIVE RISE TO GAMMA RAFFLES (GRB) — AND THE EVOLUTION OF THE MATTER EXPELLED DURING THE COLLISION — WHICH MAY GIVE RISE TO KILONOVAS. THESE NUMERICAL SIMULATIONS ARE COMPUTATIONALLY EXPENSIVE, SO TO COVER ALL POSSIBLE CONFIGURATIONS OF THE PARAMETER SPACE WE WILL NEED TO OPTIMISE OUR CODES AND OVERCOME THE CURRENT LIMITATIONS IN SCALABILITY. WE HOPE THAT THE COMPARISON OF EM AND OG EMISSION MAPS (OBTAINED ON THE ONE HAND FROM THE NUMERICAL CALCULATIONS WE PROPOSE, AND ON THE OTHER HAND FROM FUTURE OBSERVATIONS) WILL SIGNIFICANTLY ADVANCE OUR KNOWLEDGE OF GRAVITATIONAL, NUCLEAR AND PLASMA PHYSICS. It is important to highlight that this multi-digital programme is linked to the first OG DETECTIONS and we will allow the SCIENTIFIC RESULT OF DATA FACILITED BY NEW GRAVITATORY ONDS DETECTORS._x000D_Our numeral SIMULATIONS OF BINARY SYSTEMS the CODIGO HAD, an open INFRASTRUCTURE that in the current situation may be able to resolve re-examination of magnetohidrodinemic effluents with funds repressed by REALIST ECUACIONES and with a staiming of the effectiveness of the neutrinos, and (2) SIMFLOWNY, a body based on the roof for scientific dynamic models with small multiples, composing for a specific semantic language and an integrated development environment for use, which automatically manages the parallel code for SIMULACION frameworks. THE RESULTING CODE WILL INCLUDE ALL THE MAIN BASIC INGREDIENTS (I.E. STRONG GRAVITY, MAGNETIC FIELDS AND NEUTRINOS) TO SYSTEMATICALLY STUDY THE PRODUCTION OF JETS IN THESE SCENARIOS AND THE EVOLUTION OF THE MATERIAL EXPELLED DURING THE COLLISION. (English)
12 October 2021
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Palma de Mallorca
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Identifiers
AYA2016-80289-P
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