The browser you are using is not supported by this website. All versions of Internet Explorer are no longer supported, either by us or Microsoft (read more here: https://www.microsoft.com/en-us/microsoft-365/windows/end-of-ie-support).

Please use a modern browser to fully experience our website, such as the newest versions of Edge, Chrome, Firefox or Safari etc.

Joakim

Joakim Cederkäll

Professor

Joakim

Nuclear astrophysics with radioactive ions at FAIR

Author

  • R. Reifarthl
  • S. Altstadt
  • K. Goebell
  • T. Heftrich
  • M. Heil
  • A. Koloczek
  • C. Langer
  • R. Plag
  • M. Pohl
  • K. Sonnabend
  • M. Weigand
  • T. Adachi
  • F. Aksouh
  • J. Al-Khalili
  • M. AlGarawi
  • S. AlGhamdi
  • G. Alkhazov
  • N. Alkhomashi
  • H. Alvarez-Pol
  • R. Alvarez-Rodriguez
  • V. Andreev
  • B. Andrei
  • L. Atar
  • T. Aumann
  • Vladimir Avdeichikov
  • C. Bacri
  • S. Bagchi
  • C. Barbieri
  • S. Beceiro
  • C. Beck
  • C. Beinrucker
  • G. Belier
  • D. Bemmerer
  • M. Bendel
  • J. Benlliure
  • G. Benzoni
  • R. Berjillos
  • D. Bertini
  • C. Bertulani
  • S. Bishop
  • N. Blasi
  • T. Bloch
  • Y. Blumenfeld
  • A. Bonaccorso
  • K. Boretzky
  • A. Botvina
  • A. Boudard
  • P. Boutachkov
  • I. Boztosun
  • A. Bracco
  • S. Brambilla
  • J. Briz Monago
  • M. Caamano
  • C. Caesar
  • F. Camera
  • E. Casarejos
  • W. Catford
  • Joakim Cederkäll
  • B. Cederwall
  • M. Chartier
  • A. Chatillon
  • M. Cherciu
  • L. Chulkov
  • P. Coleman-Smith
  • D. Cortina-Gil
  • F. Crespi
  • R. Crespo
  • J. Cresswell
  • M. Csatlos
  • F. Dechery
  • B. Davids
  • T. Davinson
  • V. Derya
  • P. Detistov
  • P. Diaz Fernandez
  • Douglas DiJulio
  • S. Dmitry
  • D. Dore
  • J. Duenas
  • E. Dupont
  • P. Egelhof
  • I. Egorova
  • Z. Elekes
  • J. Enders
  • J. Endres
  • S. Ershov
  • O. Ershova
  • B. Fernandez-Dominguez
  • A. Fetisov
  • E. Fiori
  • A. Fomichev
  • M. Fonseca
  • L. Fraile
  • M. Freer
  • J. Friese
  • M. G. Borge
  • D. Galaviz Redondo
  • S. Gannon
  • U. Garg
  • I. Gasparic
  • L. Gasques
  • B. Gastineau
  • H. Geissel
  • R. Gernhaeuser
  • T. Ghosh
  • M. Gilbert
  • J. Glorius
  • Pavel Golubev
  • A. Gorshkov
  • A. Gourishett
  • L. Grigorenko
  • J. Gulyas
  • M. Haiduc
  • F. Hammache
  • M. Harakeh
  • M. Hass
  • M. Heine
  • A. Hennig
  • A. Henriques
  • R. Herzberg
  • M. Holl
  • A. Ignatov
  • A. Ignatyuk
  • S. Ilieva
  • M. Ivanov
  • N. Iwasa
  • Bo Jakobsson
  • H. Johansson
  • B. Jonson
  • P. Joshi
  • A. Junghans
  • B. Jurado
  • G. Koerner
  • N. Kalantar
  • R. Kanungo
  • A. Kelic-Heil
  • K. Kezzar
  • E. Khan
  • A. Khanzadeev
  • O. Kiselev
  • M. Kogimtzis
  • D. Koerper
  • S. Kraeckmann
  • T. Kroell
  • R. Kruecken
  • A. Krasznahorkay
  • J. Kratz
  • D. Kresan
  • T. Krings
  • A. Krumbholz
  • S. Krupko
  • R. Kulessa
  • S. Kumar
  • N. Kurz
  • E. Kuzmin
  • M. Labiche
  • K. Langanke
  • I. Lazarus
  • T. Le Bleis
  • C. Lederer
  • A. Lemasson
  • R. Lemmon
  • V. Liberati
  • Y. Litvinov
  • B. Loeher
  • J. Lopez Herraiz
  • G. Muenzenberg
  • J. Machado
  • E. Maev
  • K. Mahata
  • D. Mancusi
  • J. Marganiec
  • M. Martinez Perez
  • V. Marusov
  • D. Mengoni
  • B. Million
  • V. Morcelle
  • O. Moreno
  • A. Movsesyan
  • E. Nacher
  • M. Najafi
  • T. Nakamura
  • F. Naqvi
  • E. Nikolski
  • T. Nilsson
  • C. Nociforo
  • P. Nolan
  • B. Novatsky
  • G. Nyman
  • A. Ornelas
  • R. Palit
  • S. Pandit
  • V. Panin
  • C. Paradela
  • V. Parkar
  • S. Paschalis
  • P. Pawlowski
  • A. Perea
  • J. Pereira
  • C. Petrache
  • M. Petri
  • S. Pickstone
  • N. Pietralla
  • S. Pietri
  • Y. Pivovarov
  • P. Potlog
  • A. Prokofiev
  • G. Rastrepina
  • T. Rauscher
  • G. Ribeiro
  • M. Ricciardi
  • A. Richter
  • C. Rigollet
  • K. Riisager
  • A. Rios
  • C. Ritter
  • T. Rodriguez Frutos
  • J. Rodriguez Vignote
  • M. Roeder
  • C. Romig
  • D. Rossi
  • P. Roussel-Chomaz
  • P. Rout
  • S. Roy
  • P. Soederstroem
  • M. Saha Sarkar
  • S. Sakuta
  • M. Salsac
  • J. Sampson
  • J. Sanchez del Rio Saez
  • J. Sanchez Rosado
  • S. Sanjari
  • P. Sarriguren
  • A. Sauerwein
  • D. Savran
  • C. Scheidenberger
  • H. Scheit
  • S. Schmidt
  • C. Schmitt
  • L. Schnorrenberger
  • P. Schrock
  • R. Schwengner
  • D. Seddon
  • B. Sherrill
  • A. Shrivastava
  • S. Sidorchuk
  • J. Silva
  • H. Simon
  • E. Simpson
  • P. Singh
  • D. Slobodan
  • D. Sohler
  • M. Spieker
  • D. Stach
  • E. Stan
  • M. Stanoiu
  • S. Stepantsov
  • P. Stevenson
  • F. Strieder
  • L. Stuhl
  • T. Suda
  • K. Suemmerer
  • B. Streicher
  • J. Taieb
  • M. Takechi
  • I. Tanihata
  • J. Taylor
  • O. Tengblad
  • G. Ter-Akopian
  • S. Terashima
  • P. Teubig
  • R. Thies
  • M. Thoennessen
  • T. Thomas
  • J. Thornhill
  • G. Thungstrom
  • J. Timar
  • Y. Togano
  • U. Tomohiro
  • T. Tornyi
  • J. Tostevin
  • C. Townsley
  • W. Trautmann
  • T. Trivedi
  • S. Typel
  • E. Uberseder
  • J. Udias
  • T. Uesaka
  • L. Uvarov
  • Z. Vajta
  • P. Velho
  • V. Vikhrov
  • M. Volknandt
  • V. Volkov
  • P. von Neumann-Cose
  • M. von Schmid
  • A. Wagner
  • F. Wamers
  • H. Weick
  • D. Wells
  • L. Westerberg
  • O. Wieland
  • M. Wiescher
  • C. Wimmer
  • K. Wimmer
  • J. S. Winfield
  • M. Winkel
  • P. Woods
  • R. Wyss
  • D. Yakorev
  • M. Yavor
  • J. Zamora Cardona
  • I. Zartova
  • T. Zerguerras
  • I. Zgura
  • A. Zhdanov
  • M. Zhukov
  • M. Zieblinski
  • A. Zilges
  • K. Zuber

Summary, in English

The nucleosynthesis of elements beyond iron is dominated by neutron captures in the s and r processes. However, 32 stable, proton-rich isotopes cannot be formed during those processes, because they are shielded from the s-process flow and r-process beta-decay chains. These nuclei are attributed to the p and rp process. For all those processes, current research in nuclear astrophysics addresses the need for more precise reaction data involving radioactive isotopes. Depending on the particular reaction, direct or inverse kinematics, forward or time-reversed direction are investigated to determine or at least to constrain the desired reaction cross sections. The Facility for Antiproton and Ion Research (FAIR) will offer unique, unprecedented opportunities to investigate many of the important reactions. The high yield of radioactive isotopes, even far away from the valley of stability, allows the investigation of isotopes involved in processes as exotic as the r or rp processes.

Department/s

  • Nuclear physics

Publishing year

2016

Language

English

Pages

012044-012044

Publication/Series

Journal of Physics: Conference Series

Volume

665

Document type

Conference paper

Publisher

IOP Publishing

Topic

  • Astronomy, Astrophysics and Cosmology
  • Subatomic Physics

Conference name

6th Nuclear Physics in Astrophysics Conference (NPA)

Conference date

2013-05-19 - 2013-05-24

Conference place

Lisbon, Portugal

Status

Published

ISBN/ISSN/Other

  • ISSN: 1742-6588
  • ISSN: 1742-6596