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SUMMARY:Training school: "R-matrix calculations for nuclear astrophysics"
DTSTART;VALUE=DATE:20170913
DTEND;VALUE=DATE:20170916
DTSTAMP;VALUE=DATE-TIME:20201230T131450Z
UID:6218c426e41548bc98d94c09adde096d
ATTENDEE;CN="- ADSLEY Philip, IPN Orsay (France)                   ";ROLE=
 REQ-PARTICIPANT:- ADSLEY Philip, IPN Orsay (France)                   
ATTENDEE;CN="- ALCINDOR Valérian, GANIL-Caen  (France)                 ";
 ROLE=REQ-PARTICIPANT:- ALCINDOR Valérian, GANIL-Caen  (France)           
       
ATTENDEE;CN="- BOWEN Jiang, TU Darmstadt (Germany)                    ";RO
 LE=REQ-PARTICIPANT:- BOWEN Jiang, TU Darmstadt (Germany)                  
   
ATTENDEE;CN="- FRUET Guillaume	, IPHC/CNRS Strasbourg  (France)         ";
 ROLE=REQ-PARTICIPANT:- FRUET Guillaume	, IPHC/CNRS Strasbourg  (France)   
       
ATTENDEE;CN="- GNECH Alex,  Gran Sasso Science Institute (Italy)";ROLE=REQ
 -PARTICIPANT:- GNECH Alex,  Gran Sasso Science Institute (Italy)
ATTENDEE;CN="- HUBBARD Nicolas, University of York	 (United Kingdom)      
         ";ROLE=REQ-PARTICIPANT:- HUBBARD Nicolas, University of York	 (Uni
 ted Kingdom)              
ATTENDEE;CN="- HORNYAK István, University of Debrecen  (Hungary)       ";
 ROLE=REQ-PARTICIPANT:- HORNYAK István, University of Debrecen  (Hungary) 
       
ATTENDEE;CN="- MAUSS	Benoît, GANIL-Caen (France)                 ";ROLE=R
 EQ-PARTICIPANT:- MAUSS	Benoît, GANIL-Caen (France)                 
ATTENDEE;CN="- MEYER Anne, IPN-Orsay (France)                         ";RO
 LE=REQ-PARTICIPANT:- MEYER Anne, IPN-Orsay (France)                       
   
ATTENDEE;CN="- MRAZEK Jaromir,	 ASCR Rez  (Czech Republic)            	";R
 OLE=REQ-PARTICIPANT:- MRAZEK Jaromir,	 ASCR Rez  (Czech Republic)         
    	
ATTENDEE;CN="- STOECKEL Klaus, HZDR (Germany)";ROLE=REQ-PARTICIPANT:- STOE
 CKEL Klaus, HZDR (Germany)
ATTENDEE;CN="- STUART	 Perrie, University of Birmingham (United kingdom)  
                     ";ROLE=REQ-PARTICIPANT:- STUART	 Perrie, University of
  Birmingham (United kingdom)                      
ATTENDEE;CN="- SWARTZ Jacobus Andreas, Aarhus University (Denmark)";ROLE=R
 EQ-PARTICIPANT:- SWARTZ Jacobus Andreas, Aarhus University (Denmark)
ATTENDEE;CN="- THÖER Rémy, CSNSM-Orsay (France)                         
  ";ROLE=REQ-PARTICIPANT:- THÖER Rémy, CSNSM-Orsay (France)              
             
ATTENDEE;CN="- VUKMAN Nikola, Ruđer Bošković Institute (Croatia)";ROLE=
 REQ-PARTICIPANT:- VUKMAN Nikola, Ruđer Bošković Institute (Croatia)
CONTACT:Fairouz Hammache\, hammache _AT_ ipno.in2p3.fr
CREATED;VALUE=DATE-TIME:20170627T153432Z
DESCRIPTION:The main goal of the R-matrix method\, which was developed by 
 Lane and Thomas in the fifties\, is to parametrize known experimental obse
 rvables  such as cross-sections of nuclear reactions of astrophysical inte
 rest or phase shifts with a small number of parameters\, and then use thes
 e parameters to extrapolate data measured  at higher energies down to stel
 lar energies. R-matrix codes\, easy to use\, were developed these last 20 
 years such as DREAM of P. Descouvemont et al.  and AZURE of Azuma et al.. 
 These codes allow to analyze complex cases including multiple resonances w
 hich can interfere and non-resonant contributions.  In this training schoo
 l\,  the lecturers Pierre Descouvemont (Universiy ULB of Brussels) and Edw
 ard Simpson (University of Canberra) will show the participants how to use
  the two R-matrix codes after giving an introduction on the R-matrix forma
 lism.
LAST-MODIFIED;VALUE=DATE-TIME:20170824T085943Z
LOCATION:IPN\, Orsay\, France
URL:http://www.chetec.eu/activities/training-schools/training-school-r-mat
 rix-calculations-for-nuclear-astrophysics
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