Standard

Mass measurement of neutron-deficient nuclei close to the N = Z line. / Hager, Ulrike; Kankainen, A.; Eronen, T.; Rahaman, S.; Elomaa, V.; Hakala, J.; Rinta-Antila, S.; Jokinen, A.; Moore, I.; Saastamoinen, A.; Penttilä, H.; Sonoda, T.; Äystö, J.; Novikov, Y.; Vorobjev, G.

в: Proceedings of Science, 01.12.2006.

Результаты исследований: Научные публикации в периодических изданиях › статья в журнале по материалам конференции › Рецензирование

Harvard

Hager, U, Kankainen, A, Eronen, T, Rahaman, S, Elomaa, V, Hakala, J, Rinta-Antila, S, Jokinen, A, Moore, I, Saastamoinen, A, Penttilä, H, Sonoda, T, Äystö, J, Novikov, Y & Vorobjev, G 2006, 'Mass measurement of neutron-deficient nuclei close to the N = Z line', Proceedings of Science.

APA

Hager, U., Kankainen, A., Eronen, T., Rahaman, S., Elomaa, V., Hakala, J., Rinta-Antila, S., Jokinen, A., Moore, I., Saastamoinen, A., Penttilä, H., Sonoda, T., Äystö, J., Novikov, Y., & Vorobjev, G. (2006). Mass measurement of neutron-deficient nuclei close to the N = Z line. Proceedings of Science.

Vancouver

Hager U, Kankainen A, Eronen T, Rahaman S, Elomaa V, Hakala J и пр. Mass measurement of neutron-deficient nuclei close to the N = Z line. Proceedings of Science. 2006 Дек. 1.

Author

Hager, Ulrike ; Kankainen, A. ; Eronen, T. ; Rahaman, S. ; Elomaa, V. ; Hakala, J. ; Rinta-Antila, S. ; Jokinen, A. ; Moore, I. ; Saastamoinen, A. ; Penttilä, H. ; Sonoda, T. ; Äystö, J. ; Novikov, Y. ; Vorobjev, G. / Mass measurement of neutron-deficient nuclei close to the N = Z line. в: Proceedings of Science. 2006.

BibTeX

@article{42f15e585122436bb40439eb207f3c90,
title = "Mass measurement of neutron-deficient nuclei close to the N = Z line",
abstract = "The masses of neutron-deficient nuclei close to A=80 are important formodeling the astrophysical rapid proton capture process (rp process) [1]. The rp process occurs as a sequence of β +-decays and proton captures in various astrophysical sites, such as on the surface of an accreting neutron star. The rp process flows close to the N = Z nuclei up to 56Ni. At higher masses, the path will broaden and shift by about one or two units towards stable nuclei. The decay properties of several neutron-deficient nuclei near A=80 have been studied at the IGISOL facility in a series of experiments [2]. These investigations are now extended to precision mass measurements of the nuclei. The masses of 79,80,81,82,83Y, 83,84,85,86,88Zr, 85,86,87,88Nb and 96,98Mo have been measured in the precision trap of the JYFLTRAP Penning trap at IGISOL. The mass of 84Zr has been measured for the first time. The accuracy of the Q EC values and proton separation energies, which are important for the rp process, could be improved significantly for the studied neutron-deficient nuclei.",
author = "Ulrike Hager and A. Kankainen and T. Eronen and S. Rahaman and V. Elomaa and J. Hakala and S. Rinta-Antila and A. Jokinen and I. Moore and A. Saastamoinen and H. Penttil{\"a} and T. Sonoda and J. {\"A}yst{\"o} and Y. Novikov and G. Vorobjev",
year = "2006",
month = dec,
day = "1",
language = "English",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",
note = "9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006 ; Conference date: 25-06-2006 Through 30-06-2006",

}

RIS

TY - JOUR

T1 - Mass measurement of neutron-deficient nuclei close to the N = Z line

AU - Hager, Ulrike

AU - Kankainen, A.

AU - Eronen, T.

AU - Rahaman, S.

AU - Elomaa, V.

AU - Hakala, J.

AU - Rinta-Antila, S.

AU - Jokinen, A.

AU - Moore, I.

AU - Saastamoinen, A.

AU - Penttilä, H.

AU - Sonoda, T.

AU - Äystö, J.

AU - Novikov, Y.

AU - Vorobjev, G.

PY - 2006/12/1

Y1 - 2006/12/1

N2 - The masses of neutron-deficient nuclei close to A=80 are important formodeling the astrophysical rapid proton capture process (rp process) [1]. The rp process occurs as a sequence of β +-decays and proton captures in various astrophysical sites, such as on the surface of an accreting neutron star. The rp process flows close to the N = Z nuclei up to 56Ni. At higher masses, the path will broaden and shift by about one or two units towards stable nuclei. The decay properties of several neutron-deficient nuclei near A=80 have been studied at the IGISOL facility in a series of experiments [2]. These investigations are now extended to precision mass measurements of the nuclei. The masses of 79,80,81,82,83Y, 83,84,85,86,88Zr, 85,86,87,88Nb and 96,98Mo have been measured in the precision trap of the JYFLTRAP Penning trap at IGISOL. The mass of 84Zr has been measured for the first time. The accuracy of the Q EC values and proton separation energies, which are important for the rp process, could be improved significantly for the studied neutron-deficient nuclei.

AB - The masses of neutron-deficient nuclei close to A=80 are important formodeling the astrophysical rapid proton capture process (rp process) [1]. The rp process occurs as a sequence of β +-decays and proton captures in various astrophysical sites, such as on the surface of an accreting neutron star. The rp process flows close to the N = Z nuclei up to 56Ni. At higher masses, the path will broaden and shift by about one or two units towards stable nuclei. The decay properties of several neutron-deficient nuclei near A=80 have been studied at the IGISOL facility in a series of experiments [2]. These investigations are now extended to precision mass measurements of the nuclei. The masses of 79,80,81,82,83Y, 83,84,85,86,88Zr, 85,86,87,88Nb and 96,98Mo have been measured in the precision trap of the JYFLTRAP Penning trap at IGISOL. The mass of 84Zr has been measured for the first time. The accuracy of the Q EC values and proton separation energies, which are important for the rp process, could be improved significantly for the studied neutron-deficient nuclei.

UR - http://www.scopus.com/inward/record.url?scp=84887490373&partnerID=8YFLogxK

M3 - Conference article

AN - SCOPUS:84887490373

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

T2 - 9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006

Y2 - 25 June 2006 through 30 June 2006

ER -

ID: 46104767