Raphaël Raynaud
7
Documents
Identifiants chercheurs
- raphael-raynaud
- Arxiv : raynaud_r_1
- 0000-0001-6815-7109
- IdRef : 188243488
Présentation
#### **Physics Lecturer**
Université de Paris
CEA Saclay - UMR AIM
Orme des Merisiers, Bât. 709
91191 Gif-sur-Yvette - France
Email: *firstname.lastname\_AT\_cea.fr*
#### **Research Interests**
I am primarily interested in astrophysical fluid dynamics and nonlinear phenomena, with particular focus on thermal convection and magnetohydrodynamics (MHD). This branch of fluid dynamics describes the interaction of magnetic fields with electrically conducting fluid and is particularly important in explaining the magnetic properties of planets and stars, like the Earth or the Sun.
#### **Publications**
- **[ADS](http://adsabs.harvard.edu/cgi-bin/nph-abs_connect?db_key=AST&db_key=PHY&db_key=PRE&qform=AST&arxiv_sel=astro-ph&arxiv_sel=cond-mat&arxiv_sel=cs&arxiv_sel=gr-qc&arxiv_sel=hep-ex&arxiv_sel=hep-lat&arxiv_sel=hep-ph&arxiv_sel=hep-th&arxiv_sel=math&arxiv_sel=math-ph&arxiv_sel=nlin&arxiv_sel=nucl-ex&arxiv_sel=nucl-th&arxiv_sel=physics&arxiv_sel=quant-ph&arxiv_sel=q-bio&sim_query=YES&ned_query=YES&adsobj_query=YES&aut_logic=OR&obj_logic=OR&author=raynaud%2C+r&object=&start_mon=&start_year=&end_mon=&end_year=&ttl_logic=OR&title=&txt_logic=OR&text=&nr_to_return=200&start_nr=1&jou_pick=ALL&ref_stems=&data_and=ALL&group_and=ALL&start_entry_day=&start_entry_mon=&start_entry_year=&end_entry_day=&end_entry_mon=&end_entry_year=&min_score=&sort=SCORE&data_type=SHORT&aut_syn=YES&ttl_syn=YES&txt_syn=YES&aut_wt=1.0&obj_wt=1.0&ttl_wt=0.3&txt_wt=3.0&aut_wgt=YES&obj_wgt=YES&ttl_wgt=YES&txt_wgt=YES&ttl_sco=YES&txt_sco=YES&version=1)**
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Magnetar formation through a convective dynamo in protoneutron starsScience Advances , 2020, 6 (eaay2732), ⟨10.1126/sciadv.aay2732⟩
Article dans une revue
hal-02428428v1
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Gravity darkening in late-type stars. I. The Coriolis effectAstronomy and Astrophysics - A&A, 2018, 609 (A124), ⟨10.1051/0004-6361/201731729⟩
Article dans une revue
hal-01706693v1
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Magnetar formation through convective dynamos in protoneutron starsMulti-Messenger Astrophysics in the Gravitational Wave Era, Yukawa Institute for Theoretical Physics, Sep 2019, Kyoto, Japan
Communication dans un congrès
hal-02428460v1
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Magnetar formation through convective dynamos in protoneutron starsJournées de la SF2A 2019, Société Francaise d’Astronomie et d’Astrophysique, May 2019, Nice, France
Communication dans un congrès
hal-02429004v1
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Gravity darkening in late-type stars7th BCool meeting, Apr 2018, Dublin, Ireland
Communication dans un congrès
hal-02428464v1
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Convective dynamos in protoneutron starsMagnetic field formation and evolution in neutron stars, PHAROS WG4+WG5 meeting and CoCoNuT Meeting, Nov 2018, Saclay, France
Communication dans un congrès
hal-02429015v1
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Latitudinal flux variations of thermal anelastic convection in a rotating spherical shellCompressible Convection Conference, Sep 2017, Lyon, France
Communication dans un congrès
hal-02428465v1
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