Physics book: CRYRING@ESR

Lestinsky, M.; Andrianov, V. A.; Aurand, B.; Bagnoud, V.; Bernhardt, D.; Beyer, H. F.; Bishop, S.; Blaum, Klaus; Bleile, A.; Borovik, A.; Bosch, F.; Bostock, Christopher J.; Brandau, C.; Bräuning‐Demian, A.; Bray, Igor; Davinson, T.; Ebinger, B.; Echler, A.; Egelhof, P.; Ehresmann, A.; Engström, M.; Enss, C.; Ferreira, Natalia; Fischer, Daniel; Fleischmann, A.; Förster, E.; Fritzsche, S.; Geithner, R.; Geyer, Sabrina; Glorius, J.; Göbel, K.; Gorda, O.; Goullon, J.; Grabitz, P.; Grisenti, R. E.; Gumberidze, A.; Hagmann, S.; Heil, M.; Heinz, A.; Herfurth, F.; Heß, R.; Hillenbrand, P.‐M.; Hubele, Renate; Indelicato, P.; Källberg, A.; Kester, O.; Kiselev, O.; Knie, André; Kozhuharov, C.; Kraft‐Bermuth, S.; Kühl, T.; Lane, G. J.; Litvinov, Yu. A.; Liesen, D.; W., X.; Märtin, R.; Moshammer, R.; Müller, Alfred; Namba, S.; Neumeyer, Peter F.; Nilsson, T.; Nörtershäuser, W.; Paulus, Gerhard G.; Petridis, N.; Reed, M. W.; Reifarth, R.; Reiß, Philipp; Rothhardt, Jan; Sánchez, R.; Sanjari, M. S.; Schippers, S.; Schmidt, H. T.; Schneider, Dieter; Scholz, P.; Schuch, R.; Schulz, Michael; Shabaev, V. M.; Simonsson, Ansgar; Sjöholm, Johannes; Skeppstedt, Ö.; Sonnabend, K.; Spillmann, U.; Stiebing, K. E.; Steck, M.; Stöhlker, Th.; Surzhykov, A.; Torilov, S. Yu.; Träbert, E.; Trassinelli, Martino; Trotsenko, S.; Tu, X. L.; Uschmann, I.; Walker, P. M.; Weber, G.; Winters, D.; Woods, P. J.; Zhao, He; Zhang, Y. H.

doi:10.1140/epjst/e2016-02643-6

Cited by 121 publications

(73 citation statements)

References 322 publications

(432 reference statements)

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“…The future scientific programs are rich and include investigations of exotic decay channels such as two-photon and internal pair de-excitation [115], bound electron-positron decays [116], nuclear excitations by electron capture or electron transitions [117], α-decays [118], as well as EC decay of lithium-like ions and forbidden EC decays [82,85]. Last but not least, proton and neutron radioactivity as well as β-delayed particle emission [119] are interesting topics.…”

mentioning

confidence: 99%

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Studies at the border between nuclear and atomic physics: Weak decays of highly charged ions

Atanasov¹,

Blaum²,

Bosch³

et al. 2017

J. Phys.: Conf. Ser.

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confidence: 99%

“…The CRYRING has been installed behind the ESR [117]. HCIs decelerated to energies down to a few hundreds of A keV will be available, thus allowing unique experiments at the interface between nuclear structure, atomic and astrophysics.…”

mentioning

confidence: 99%

Studies at the border between nuclear and atomic physics: Weak decays of highly charged ions

Atanasov¹,

Blaum²,

Bosch³

et al. 2017

J. Phys.: Conf. Ser.

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“…Ions with energies between 0.1 AMeV and 10 AMeV can be efficiently stored in ion storage rings [10,11]. The combination of such a ring with a reactor could open the path to direct measurements of neutron-induced cross sections on short-lived radioactive isotopes in the keV-regime [12].…”

Section: Neutron Capture Cross Sectionsmentioning

confidence: 99%

Reactor neutrons in nuclear astrophysics

et al. 2017

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Abstract. The huge neutron fluxes offer the possibility to use research reactors to produce isotopes of interest, which can be investigated afterwards. An example is the half-lives of long-lived isotopes like 129 I. A direct usage of reactor neutrons in the astrophysical energy regime is only possible, if the corresponding ions are not at rest in the laboratory frame. The combination of an ion storage ring with a reactor and a neutron guide could open the path to direct measurements of neutron-induced cross sections on short-lived radioactive isotopes in the astrophysically interesting energy regime.

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“…Other reactions involved in the particular process are also shown. The expected experimental coverage of the future CRYRING@ESR [7] and the existing ESR storage ring at GSI [1] can be seen.…”

Section: Introductionmentioning

confidence: 96%

Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI

et al. 2017

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Abstract. Ion optical calculations for a storage ring at the present GSI facility for direct proton-induced reactions relevant for different astrophysical processes are presented. As an example case, the 59 Cu(p, γ) and 59 Cu(p, α) reactions are shown. The branching of these two reactions is important in X-ray burst scenarios, since it determines the breakout out of the major 56 Ni waiting point.

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Physics book: CRYRING@ESR

Cited by 121 publications

References 322 publications

Studies at the border between nuclear and atomic physics: Weak decays of highly charged ions

Studies at the border between nuclear and atomic physics: Weak decays of highly charged ions

Reactor neutrons in nuclear astrophysics

Constraining astrophysical reaction rates: using the storage rings at FAIR/GSI

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