The Mount Bego
Nice, February 6 - 17, 2006
Programme
Transports
Lecturers
Participants Contacts Nice, February 6 - 17, 2006
The Mount Bego is a sacred mountain, close to Nice, on the Alpes
Maritimes, in the Mercantour Parc, currently being included in the
UNESCO world heritage list. For thousands of years, from the Stone Age
all the way to the Iron Age, the first inhabitants of Europe were
climbing all the way to the top of Mount Bego along the Canyons of the
Valley of the Roya river starting from the Mediterranean Sea. They have
recorded their early expressionsof observing nature in more than thirty
thousand graffiti on the stones of the "Valle des Merveilles". Our
Bego scientific encounters in Nice celebrate this first quest of
knowledge and research of our ancestors. They continue it in the most
advanced research of relativistic astrophysics.
Schedule
BACK SPEAKERS SCHEDULE Program
NICE 6-10 FEBRUARY 2006
MON 6 TUE 7 WED 8 THU 9 FRI 10
8,30-9,30 WELCOME DAMOUR DAMOUR DAMOUR
9,30-10,30 GURZADYAN GURZADYAN KRAMER KRAMER KRAMER
10,30-11,00 BREAK
11,00-12,00 BELINSKI BELINSKI BELINSKI DAMOUR DAMOUR
12,00-13,00 FILIPPI CHERUBINI VERESHCHAGIN TARTAGLIA TITARCHUCK
BREAK
15,30-16,30 PACHECO MIGNARD MIGNARD LATTANZI Mario KLIONER
16,30-17,00 BREAK
17,00-18,00 CIANFRANI KLEINERT KRAMER MERCURI
NICE 13-17 FEBRUARY 2006
MON 13 TUE 14 WED 15 THU 16 FRI 17
8,30-9,30 TITARCHUCK TITARCHUCK TITARCHUCK LAURENT
9,30-10,30 RUFF/BIANCO RUFF/BIANCO RUFF/BIANCO PERON
10,30-11,00 BREAK
11,00-12,00 NOVELLO NOVELLO GERALICO CHARDONNET
12,00-13,00 MATTEI XUE MOSCHELLA MOSCHELLA
BREAK
15,30-16,30 KLIONER KLIONER TEYSSANDIER TEYSSANDIER
16,30-17,00 BREAK
17,00-18,00 LECIAN MEETING WITH MUNICIPALITY and NEIGHBORHOOD OF VILLA
RATTI MIGNARD LATTANZI Massi.
participants list
Program
Back
Lecturers
Participants List - Nice, February 2006
AGNELLO Dario
diddmail@yahoo.it
BATTISTI Marco Valerio
battisti@ICRA.it
BEAUMONT Jean Luc
Jean-Luc.BEAUMONT@unice.fr
BELINSKI Vladimir
belinski@ICRA.it
BELVEDERE Riccardo
ribelwave@libero.it
BERNARDINI Maria Grazia
maria.bernardini@ICRA.it
BIANCO Carlo Luciano
bianco@icra.it
BINI Donato
binid@ICRA.it
BORMANN Celin Hugo
hugo.bormann@ICRA.it
CAITO Letizia
letizia.caito@ICRA.it
CHARDONNET Pascal
chardonnet@lapp.in2p3.fr
CHERUBINI Christian
cherubini@ICRA.it
CIANFRANI Francesco
francesco.cianfrani@ICRA.it
COULLET Pierre
pcoullet@mac.com
DAINOTTI Maria Giovanna
Dainotti@ICRA.it
DAMOUR Thibault
damour@ihes.fr
FILIPPI Simonetta
filippi@icra.it
GERALICO Andrea
Geralico@ICRA.it
GUIDA Roberto
roberto.guida@icra.it
GURZADYAN Vahe
gurzadyan@icra.it
KLEINERT Hagen
kleinert@physik.fu-berlin.de
KLIONER Sergei
klioner@rcs.urz.tu-dresden.de
KRAMER Michael
mkramer@jb.man.ac.uk
LATTANZI Mario
lattanzi@to.astro.it
LATTANZI Massimiliano
lattanzi@icra.it
LAURENT Philippe
plaurent@cea.fr
LECIAN Orchidea Maria
lecian@ICRA.it
MARZIN Antoine
antoinemarzin@voila.frt
MATTEI Alvise
Mattei@ICRA.it
MERCURI Simone
Mercuri@ICRA.it
MIGNARD Franois
Francois.Mignard@obs-azur.fr
MOSCHELLA Ugo ugo.moschella@uninsubria.it
NAGAR Alessandro
alessandro.nagar@polito.it
NOVELLO Mario
novello@cbpf.br
PACHECO Jos
pacheco@obs-nice.fr
PERON Roberto
roberto.peron@ifsi.rm.cnr.it
PIZZI Marco
Pizzi@ICRA.it
POMPI Francesca
francesca.pompi@ICRA.it
ROSANO Laura
laura.rosano@icra.it
ROTONDO Michael
michael.rotondo@ICRA.it
ROSQUIT Kjell
kr@physto.se
RUFFINI Remo
ruffini@ICRA.it
TARTAGLIA Angelo
angelo.tartaglia@polito.it
TEYSSANDIER Pierre
Pierre.Teyssandier@obspm.fr
TITARCHUK Lev
ltitarchuk@ssd5.nrl.navy.mil
TRIAY Roland
Roland.Triay@cpt.univ-mrs.fr
VERESHCHAGIN Gregory
Veresh@icra.it
XUE She-Sheng
xue@icra.it
D'ANGELO Veronica veronica.dangelo@icranet.org
DI BERARDINO Federica federica.diberardino@icranet.org
Logistic
SECRETARIAT:
Miss Federica Di Berardino
Piazzale della Repubblica, 10 - 65100 Pescara, Italia
Phone: Secretariat +39-085-23054200
Fax: +39-085-4219252
ACCOMODATION:
NICE La Maison du Seminaire
ST. ETIENNE Le Rabuons (Friday night);
Le Chalet, Le Regalivou et Les Amis (Saturday night)
TRANSPORTATION:
SEMINARS
University of Nice Sophia Antipolis
PROGRAMME
COMPLETE
LECTURES
BACK
"LES RENCONTRES SCIENTIFIQUES DU BEGO"
-BEGO SCIENTIFIC RENCONTRES-
6-17 FEBRUARY
( REGISTRATION FEE: EUR 100,00 )
Back
Detailed programme
Lecturers
Scientific Program
MONDAY 6: 8,30-9,30 Welcome by - A. Marouani (Pres. UNICE) - P.
Coullet
9,30-13,00 Lectures
13,00-15,30 Lunch
15,30- 18,00 Lectures
TUESDAY 7 - FRIDAY 10: 8,30-13,00 Lectures
13,00-15,30 Lunch
15,30- 18,00 Lectures
FRIDAY 10- SUNDAY 12: Week-end to St. Etienne de Tine
MONDAY 13- WEDNESDAY 15: 8,30-13,00 Lectures
13,00-15,30 Lunch
15,30- 18,00 Lectures
THURSDAY 16: 8,30-13,00 Lectures
13,00-15,30 Lunch
15,30- 17,00 Lectures
17,00-18,00 MEETING WITH MUNICIPALITY AND NEIGHBORHOOD
OF VILLA RATTI
FRIDAY 17: 8,30-13,00 Lectures
13,00-15,30 Lunch
15,30- 16,30 Lectures
1
1) *ARRIVAL (Sunday)- AIRPORT-MAISON DU SEMINAIRE*
Airport Terminal 1 or 2: take the bus n. 98 to the Gare Routire
or the line n.500, from the Terminal 1 to the Gare Routire
(Pay attention, please: few trips!)
Ligne : 500 NICE <> GRASSE - Direction : NICE
Dpart : NICE - AEROPORT 1 - Date : 05/02/2006
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Arrive : NICE - Gare Routire - Date : 05/02/2006
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There is a free Shuttle Bus between Terminal 1 et 2.
then, after the arrival to the Gare Routire with the bus n. 98 or
n.500,
take line n. 100, direction MONACO MENTON
Direction : *MONACO MENTON*
Direction : MONACO MENTON
Dpart : NICE - Gare Routire - Date : 05/02/2006
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Stop to LE PORT
Arrival : *NICE - Le port - *Date : *05/02/2006*
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then
- walk to the Maison du S. (300 mt, more or less)
- take line 20 to the Maison du Seminaire (Stop La Rserve)
2) *MdS-CAMPUS VALROSE (UNIV.)-MdS (BUS 30-37)*
Weekdays :
GOING
Arrt de dpart :
LA RESERVE (NICE)
Plan
Arrt d'arrive :
VALROSE (NICE)
Plan
Date du trajet :
06/02/2006
Dpart : 07:44
Dure totale du trajet : 29 mn
Arrive : 08:13
Nombre de changements : 1
Dep. 07:44
Dpart de l'arrt LA RESERVE (NICE)
Dep. 07:44
Arr. 07:58
Ligne : 30 Gare SNCF-Riquier
Direction : GARE SNCF
Dpart : AVENUE DE LA RESERVE [Plan]
Arrive : DESAMBROIS [Plan]
Dep. 08:07
Arr. 08:13
Ligne : 37 Station JC Bermond-Stade Valrose
Direction : STADE VALROSE
Dpart : DESAMBROIS
Arrive : VALROSE [Plan]
Arr. 08:13
Arrive l'arrt VALROSE (NICE)
RETURN
Arrt de dpart :
VALROSE (NICE)
Plan
Arrt d'arrive :
LA RESERVE (NICE)
Plan
Date du trajet :
06/02/2006
Option du trajet :
le plus rapide
Dpart : 18:26
Dure totale du trajet : 35 mn
Arrive : 19:01 ...
ABSTRACTS
BELINSKI Vladimir
1. "Exactly solvable ansatz of Einstein-Maxwell Equations".
An outline of the general theory of integrability of the
Einstein-Maxwell equations will be given.
2. "On the equilibrium state for two charged masses in General
Relativity".
The exact stationary solution of the Einstein-Maxwell equations
representing the equilibrium state of two Reissner-Nordstrom objects
will be described.
3. "On the existence of black hole evaporation"
A new arguments will be presented confirming the point of view that a
Schwarzschild black hole does not radiate.
BIANCO Carlo Luciano
BINI Donato
CHARDONNET Pascal
Univit De Savoie-France
The Dark Matter Universe
Dark matter is a long standing puzzle starting from Le Verrier with his
discovery of Neptune in 1846 as a perturbation of Uranus. Our Galaxy is
surrounded by an extended halo of unseen material. So far undetected,
that dark matter induces a flat rotation curve in the Galactic plane.
Its presence has been noticed since many decades. However, its nature
is still unknown. The dark matter problem consists simply, in the
existence of invisible mass showing its presence by gravitational
effects. Now, it is widely accepted that dark matter exists. In fact,
there is evidence for dark matter on scales from galaxy to the cluster
of galaxies and to the whole Universe itself. Zwicky measured the
dispersion velocity in the Coma cluster and found that the dynamical
mass was hundred times more than the luminosity mass. Moreover, the
dark matter seems essential: the growth of structure in the Universe by
hierachical merging of the dark matter halo is a master piece of moderm
cosmology.
Recently, WMAP has established the presence of non baryonic dark matter
with the density reported in terms of critical density of order 23%.
This is now the standard value of the modern cosmology for dark matter
density.
CHERUBINI Christian
Scattering problems in rotating astrophysical and acoustic black holes:
general theory and numerical techniques
In this lecture the problem of scattering of fields of different
helicity on black holes on Nature is presented.
After a rapid review of Teukolsky formalism applied to rotating Kerr ...
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