https://doi.org/10.1140/epja/s10050-022-00707-9
Letter
Study of the production and decay properties of neutron-deficient nobelium isotopes
1
Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Russia
2
The Institute of Nuclear Physics, 050032, Almaty, Republic of Kazakhstan
3
Dubna State University, Dubna, Russia
4
IJCLAb, IN2P3-CNRS, Université Paris Saclay, 91405, Orsay, France
5
L.N. Gumilyov Eurasian National University, Nur-Sultan, Kazakhstan
6
GANIL, 14076, Caen Cedex 5, France
7
Université de Strasbourg, CNRS, IPHC UMR 7178, 67000, Strasbourg, France
8
Comenius University in Bratislava, 84248, Bratislava, Slovakia
Received:
7
December
2021
Accepted:
14
March
2022
Published online:
24
March
2022
The new neutron-deficient isotope No was synthesized for the first time in the fusion-evaporation reaction
Pb(
Ca,3n)
No. After separation, using the kinematic separator SHELS, the new isotope was identified with the GABRIELA detection system through genetic correlations with the known daughter and granddaughter nuclei
Fm and
Cf. The alpha-decay activity of
No has an energy of 9129(22) keV and half-life 38.3(2.8) ms. An upper limit of 0.2% was measured for the fission branch of
No. Based on the present data and recent information on the decay properties of
Rf and aided by Geant4 simulations, the ground state of
No is assigned the 5/2
[622] neutron configuration and a partial decay scheme from
Rf to
Fm could be established. The production cross-section was found to be
(3n)=0.47(4) nb at a mid-target beam energy of 225.4 MeV, which corresponds to the maximum of the calculated excitation function. Correlations of the
No alpha activity with subsequent alpha decays of energy 7728(20) keV and half-life
min provided a firm measurement of the electron-capture or
branch of
Fm to
Es. The excitation function for the 1n, 2n and 3n evaporation channels was measured. In the case of the 2n-evaporation channel
No, a strong variation of the ground state and isomeric state populations as a function of bombarding energy could be evidenced.
© The Author(s), under exclusive licence to Società Italiana di Fisica and Springer-Verlag GmbH Germany, part of Springer Nature 2022