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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
El momento de la verdad para la materia oscura WIMP
1Institut d'Astrophysique de Paris, UMR 7095-CNRS, Université Pierre et Marie Curie, 98 bis Boulevard Arago, 75014 Paris, France. bertone@iap.fr
Nature
|November 19, 2010
Resumen
Las partículas masivas de interacción débil (WIMP) son las principales candidatas a la materia oscura. Los experimentos en el Gran Colisionador de Hadrones y más allá pronto confirmarán o refutarán su existencia.
Área de la Ciencia:
- Cosmología y Física de Partículas.
- Física de las astropartículas Física de las astropartículas
Sus antecedentes:
- La materia oscura comprende el 85% del contenido de materia del universo.
- La composición de la materia oscura sigue siendo desconocida.
- Las partículas masivas de interacción débil (WIMP) son un prominente candidato teórico para la materia oscura.
Objetivo del estudio:
- Para resaltar la importancia de las WIMP como candidatos a la materia oscura.
- Para discutir la coyuntura crítica para las teorías WIMP debido a los próximos resultados experimentales.
Principales métodos:
- Las extensiones teóricas del Modelo Estándar de la física de partículas predicen naturalmente los WIMPs.
- Las búsquedas de WIMPs se están llevando a cabo utilizando el Gran Colisionador de Hadrones (LHC).
- Las nuevas generaciones de experimentos de astropartículas también están investigando la existencia de WIMP.
Principales resultados:
- El estudio no presenta nuevos resultados experimentales, sino que enmarca el estado actual de la investigación WIMP.
- Los próximos experimentos están listos para proporcionar evidencia definitiva a favor o en contra de las WIMPs.
Conclusiones:
- Los próximos cinco a diez años representan un período crucial para la investigación WIMP.
- Los resultados experimentales confirmarán WIMPs como la solución al rompecabezas de la materia oscura o llevarán a su menor prominencia.
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