Hola,
¿eres nuevo aquí?

Regístrate gratis y conecta tu empresa con financiación pública, partners y proyectos.

Tengo cuenta

Regístrate

Ver video

PWNtori

Financiado

Cerrado

MHD modeling of wind tori and particle acceleration in pulsar wind nebulae

The proposed research aims to constrain the energy spectrum of accelerated particles in pulsar wind nebulae (PWNe), and their contribution to the recently measured primary cosmic-ray positron spectrum. To this end, observations o... ver más

31/08/2014

INAF

125K€

Presupuesto del proyecto: 125K€

Líder del proyecto

ISTITUTO NAZIONALE DI ASTROFISICA No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Fecha límite participación Sin fecha límite de participación.

Financiación concedida El organismo FP7 notifico la concesión del proyecto el día 2014-08-31 No tenemos la información de la convocatoria

0% 100% 100%

Información adicional privada

No hay información privada compartida para este proyecto. Habla con el coordinador.

1 Participantes

INAF

0.00€ | Lider

Conecta tu I+D

¿Tienes un proyecto y buscas un partner? Gracias a nuestro motor inteligente podemos recomendarte los mejores socios y ponerte en contacto con ellos. Te lo explicamos en este video

Proyectos interesantes

CMR Cosmic ray acceleration magnetic field and radiation hydrod... 900K€ Cerrado

COMPLEX Cosmological magnetic fields and plasma physics in extended... 2M€ Cerrado

AYA2017-92402-EXP LA BESTIA INTERIOR Y EXTERIOR: ACELERACION Y EMISION EN GAPS... 42K€ Cerrado

GammaRayCascades Probing the origin of intergalactic magnetic fields and cosm... 175K€ Cerrado

PICOGAL Mind the Gap from Plasma Kinetics to Cosmological Galaxy Fo... 3M€ Cerrado

GRBS Gamma Ray Bursts as a Focal Point of High Energy Astrophysic... 2M€ Cerrado

Líder del proyecto

ISTITUTO NAZIONALE DI ASTROFISICA No se ha especificado una descripción o un objeto social para esta compañía.

TRL 4-5

Presupuesto del proyecto 125K€

Fecha límite de participación Sin fecha límite de participación.

Descripción del proyecto The proposed research aims to constrain the energy spectrum of accelerated particles in pulsar wind nebulae (PWNe), and their contribution to the recently measured primary cosmic-ray positron spectrum. To this end, observations of synchrotron emission from the inner wind tori of young PWNe, in particular in the infrared domain, will be modeled using relativistic magnetohydrodynamic (MHD) numerical simulations developed at the host institute (Arcetri). The radiative and adiabatic energy losses of the accelerated electrons and positrons prior to their escape into the interstellar medium will be computed using relativistic MHD simulations of PWNe in their later, bow-shock phase, when they are most likely to contribute to the leptonic cosmic ray spectrum. The combination of these two parts of the project will allow more precise predictions of the contribution of PWNe to the primary cosmic-ray positron spectrum, and help quantify the potential necessity for additional, alternative sources of positrons such as the annihilation of dark matter particles. The proposed mobility will give Dr. Gallant the opportunity to reach higher levels and a greater balance of theoretical and observational expertise, through collaboration in state-of-the-art theoretical research, as well as interaction with experts in infrared observation, at Arcetri. The skills acquired, and the longer-term collaborations at the European level which his mobility will foster, will allow Dr. Gallant to continue to play a leading role in the scientific exploitation of future high-energy astrophysical experiments, and in particular the planned ground-based gamma-ray observatory CTA, in which European groups are deeply invested.

Conecta tu I+D

Entra hoy

¿Olvidé mi contraseña?

Financiación

Empresas

CTIs/Universidades

Proyectos

Investigadores