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Quenching of the SnSbTe cycle in the rp process. / Elomaa, V. V.; Vorobjev, G. K.; Kankainen, A.; Batist, L.; Eronen, T.; Hakala, J.; Jokinen, A.; Moore, I. D.; Novikov, Yu N.; Penttilä, H.; Rahaman, S.; Rissanen, J.; Saastamoinen, A.; Schatz, H.; Seliverstov, D. M.; Weber, C.; Äystö, J.

In: Physical Review Letters, Vol. 102, No. 25, 252501, 25.06.2009.

Research output: Contribution to journal › Article › peer-review

Harvard

Elomaa, VV, Vorobjev, GK, Kankainen, A, Batist, L, Eronen, T, Hakala, J, Jokinen, A, Moore, ID, Novikov, YN, Penttilä, H, Rahaman, S, Rissanen, J, Saastamoinen, A, Schatz, H, Seliverstov, DM, Weber, C & Äystö, J 2009, 'Quenching of the SnSbTe cycle in the rp process', Physical Review Letters, vol. 102, no. 25, 252501. https://doi.org/10.1103/PhysRevLett.102.252501

APA

Elomaa, V. V., Vorobjev, G. K., Kankainen, A., Batist, L., Eronen, T., Hakala, J., Jokinen, A., Moore, I. D., Novikov, Y. N., Penttilä, H., Rahaman, S., Rissanen, J., Saastamoinen, A., Schatz, H., Seliverstov, D. M., Weber, C., & Äystö, J. (2009). Quenching of the SnSbTe cycle in the rp process. Physical Review Letters, 102(25), [252501]. https://doi.org/10.1103/PhysRevLett.102.252501

Vancouver

Elomaa VV, Vorobjev GK, Kankainen A, Batist L, Eronen T, Hakala J et al. Quenching of the SnSbTe cycle in the rp process. Physical Review Letters. 2009 Jun 25;102(25). 252501. https://doi.org/10.1103/PhysRevLett.102.252501

Author

Elomaa, V. V. ; Vorobjev, G. K. ; Kankainen, A. ; Batist, L. ; Eronen, T. ; Hakala, J. ; Jokinen, A. ; Moore, I. D. ; Novikov, Yu N. ; Penttilä, H. ; Rahaman, S. ; Rissanen, J. ; Saastamoinen, A. ; Schatz, H. ; Seliverstov, D. M. ; Weber, C. ; Äystö, J. / Quenching of the SnSbTe cycle in the rp process. In: Physical Review Letters. 2009 ; Vol. 102, No. 25.

BibTeX

@article{c1956525805e4e06a425093cfb6d5ee0,
title = "Quenching of the SnSbTe cycle in the rp process",
abstract = "The nuclides Sn104-108, Sb106-110, Te108,109, and I111 at the expected endpoint of the astrophysical rp process have been produced in Ni58+Ninat fusion-evaporation reactions at IGISOL and their mass values were precisely measured with the JYFLTRAP Penning trap mass spectrometer. For Sb106, Sb108, and Sb110 these are the first direct experimental mass results obtained. The related one-proton separation energies have been derived and the value for Sb106, Sp=424(8)keV, shows that the branching into the closed SnSbTe cycle in the astrophysical rp process is weaker than expected.",
author = "Elomaa, {V. V.} and Vorobjev, {G. K.} and A. Kankainen and L. Batist and T. Eronen and J. Hakala and A. Jokinen and Moore, {I. D.} and Novikov, {Yu N.} and H. Penttil{\"a} and S. Rahaman and J. Rissanen and A. Saastamoinen and H. Schatz and Seliverstov, {D. M.} and C. Weber and J. {\"A}yst{\"o}",
year = "2009",
month = jun,
day = "25",
doi = "10.1103/PhysRevLett.102.252501",
language = "English",
volume = "102",
journal = "Physical Review Letters",
issn = "0031-9007",
publisher = "American Physical Society",
number = "25",

}

RIS

TY - JOUR

T1 - Quenching of the SnSbTe cycle in the rp process

AU - Elomaa, V. V.

AU - Vorobjev, G. K.

AU - Kankainen, A.

AU - Batist, L.

AU - Eronen, T.

AU - Hakala, J.

AU - Jokinen, A.

AU - Moore, I. D.

AU - Novikov, Yu N.

AU - Penttilä, H.

AU - Rahaman, S.

AU - Rissanen, J.

AU - Saastamoinen, A.

AU - Schatz, H.

AU - Seliverstov, D. M.

AU - Weber, C.

AU - Äystö, J.

PY - 2009/6/25

Y1 - 2009/6/25

N2 - The nuclides Sn104-108, Sb106-110, Te108,109, and I111 at the expected endpoint of the astrophysical rp process have been produced in Ni58+Ninat fusion-evaporation reactions at IGISOL and their mass values were precisely measured with the JYFLTRAP Penning trap mass spectrometer. For Sb106, Sb108, and Sb110 these are the first direct experimental mass results obtained. The related one-proton separation energies have been derived and the value for Sb106, Sp=424(8)keV, shows that the branching into the closed SnSbTe cycle in the astrophysical rp process is weaker than expected.

AB - The nuclides Sn104-108, Sb106-110, Te108,109, and I111 at the expected endpoint of the astrophysical rp process have been produced in Ni58+Ninat fusion-evaporation reactions at IGISOL and their mass values were precisely measured with the JYFLTRAP Penning trap mass spectrometer. For Sb106, Sb108, and Sb110 these are the first direct experimental mass results obtained. The related one-proton separation energies have been derived and the value for Sb106, Sp=424(8)keV, shows that the branching into the closed SnSbTe cycle in the astrophysical rp process is weaker than expected.

UR - http://www.scopus.com/inward/record.url?scp=67649427442&partnerID=8YFLogxK

U2 - 10.1103/PhysRevLett.102.252501

DO - 10.1103/PhysRevLett.102.252501

M3 - Article

AN - SCOPUS:67649427442

VL - 102

JO - Physical Review Letters

JF - Physical Review Letters

SN - 0031-9007

IS - 25

M1 - 252501

ER -

ID: 46103500