title: Nuclear isomers in superheavy elements as stepping stones towards the island of stability.
abstract: A long-standing prediction of nuclear models is the emergence of a region of long-lived, or even stable, superheavy elements beyond the actinides. These nuclei owe their enhanced stability to closed shells in the structure of both protons and neutrons. However, theoretical approaches to date do not yield consistent predictions of the precise limits of the 'island of stability'; experimental studies are therefore crucial. The bulk of experimental effort so far has been focused on the direct creation of superheavy elements in heavy ion fusion reactions, leading to the production of elements up to proton number Z = 118 (refs 4, 5). Recently, it has become possible to make detailed spectroscopic studies of nuclei beyond fermium (Z = 100), with the aim of understanding the underlying single-particle structure of superheavy elements. Here we report such a study of the nobelium isotope 254No, with 102 protons and 152 neutrons--the heaviest nucleus studied in this manner to date. We find three excited structures, two of which are isomeric (metastable). One of these structures is firmly assigned to a two-proton excitation. These states are highly significant as their location is sensitive to single-particle levels above the gap in shell energies predicted at Z = 114, and thus provide a microscopic benchmark for nuclear models of the superheavy elements.
authors.affiliation: Department of Physics, University of Liverpool, Liverpool L69 7ZE, UK. rdh@ns.ph.liv.ac.uk
authors.forename: R-D
authors.initials: RD
authors.lastname: Herzberg
authors.forename: P T
authors.initials: PT
authors.lastname: Greenlees
authors.forename: P A
authors.initials: PA
authors.lastname: Butler
authors.forename: G D
authors.initials: GD
authors.lastname: Jones
authors.forename: M
authors.initials: M
authors.lastname: Venhart
authors.forename: I G
authors.initials: IG
authors.lastname: Darby
authors.forename: S
authors.initials: S
authors.lastname: Eeckhaudt
authors.forename: K
authors.initials: K
authors.lastname: Eskola
authors.forename: T
authors.initials: T
authors.lastname: Grahn
authors.forename: C
authors.initials: C
authors.lastname: Gray-Jones
authors.forename: F P
authors.initials: FP
authors.lastname: Hessberger
authors.forename: P
authors.initials: P
authors.lastname: Jones
authors.forename: R
authors.initials: R
authors.lastname: Julin
authors.forename: S
authors.initials: S
authors.lastname: Juutinen
authors.forename: S
authors.initials: S
authors.lastname: Ketelhut
authors.forename: W
authors.initials: W
authors.lastname: Korten
authors.forename: M
authors.initials: M
authors.lastname: Leino
authors.forename: A-P
authors.initials: AP
authors.lastname: Leppänen
authors.forename: S
authors.initials: S
authors.lastname: Moon
authors.forename: M
authors.initials: M
authors.lastname: Nyman
authors.forename: R D
authors.initials: RD
authors.lastname: Page
authors.forename: J
authors.initials: J
authors.lastname: Pakarinen
authors.forename: A
authors.initials: A
authors.lastname: Pritchard
authors.forename: P
authors.initials: P
authors.lastname: Rahkila
authors.forename: J
authors.initials: J
authors.lastname: Sarén
authors.forename: C
authors.initials: C
authors.lastname: Scholey
authors.forename: A
authors.initials: A
authors.lastname: Steer
authors.forename: Y
authors.initials: Y
authors.lastname: Sun
authors.forename: Ch
authors.initials: Ch
authors.lastname: Theisen
authors.forename: J
authors.initials: J
authors.lastname: Uusitalo