Hola,
¿eres nuevo aquí?

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

Tengo cuenta

Regístrate

Ver video

NSMAG

Financiado

Cerrado

Magnetic Fields in Neutron Stars via Numerical Simulations

Neutron Stars (NSs) are what is left after a massive stars terminates its life in a Supernova Explosion. It was immediately evident the role of rotation and magnetic fields in characterizing their phenomenology. We now know severa... ver más

31/07/2016

INAF

100K€

Presupuesto del proyecto: 100K€

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 2016-07-31 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

DYNACOR From the Sun to stars Interplay between dynamo and corona 162K€ Cerrado

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

AYA2015-66899-C2-1-P ASTROFISICA RELATIVISTA COMPUTACIONAL 344K€ Cerrado

ExCEED Explaining Common Envelope Evolution and Dynamics in binary... 3M€ Cerrado

COSMOLAB Laboratory simulation of cosmological magnetic fields 1M€ Cerrado

MAGMIST From the magnetized diffuse interstellar medium to the stars 1M€ 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 100K€

Fecha límite de participación Sin fecha límite de participación.

Descripción del proyecto Neutron Stars (NSs) are what is left after a massive stars terminates its life in a Supernova Explosion. It was immediately evident the role of rotation and magnetic fields in characterizing their phenomenology. We now know several different class of NSs, whose peculiarities we think are due to their intrinsic magnetic properties. Strong magnetic fields play a crucial role in many high-energy astrophysical systems containing compact objects. Understanding, the role of magnetic field in NS, developing the tools necessary for its correct modeling, and being able to follow its dynamics, has important consequences in other astrophysical fields. This proposal aims to develop a research line on the physics involving strong magnetic fields in compact objects, and their role in powering high-energy astrophysical engines, through the use of state-of-the-art computational techniques for relativistic MHD. The planned research has a strong numerical focus, which should complement, and enhance the existing theoretical and observational strength points already in place, both within the host institution and its national and international partners. We also plan to make all tools and numerical algorithms that will be developed, available on-line with a dedicated web-site The complexity of the physics involved makes the study of magnetized NS both challenging for its complexity and interesting for its possible outcomes. Numerical tools and techniques are now mature enough thanks to the recent development of robust and reliable multidimensional numerical schemes for general relativistic MHD, to be applied to the investigation of these systems. I plan to construct fully consistent magnetized models of NS in General Relativity; to investigate the role of the Equation of State in conjunction with the magnetic field; to investigate the role of magnetic dissipation ad turbulent dynamo ; nd to the magnetosphere-interior relation.

Conecta tu I+D

Entra hoy

¿Olvidé mi contraseña?

Financiación

Empresas

CTIs/Universidades

Proyectos

Investigadores