New Superheavy Element Isotopes:<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi>Pu</mml:mi><mml:mprescripts/><mml:none/><mml:mn>242</mml:mn></mml:mmultiscripts><mml:mo stretchy="false">(</mml:mo><mml:mmultiscripts><mml:mi>Ca</mml:mi><mml:mprescripts/><mml:none/><mml:mn>48</mml:mn></mml:mmultiscripts><mml:mo>,</mml:mo><mml:mn>5</mml:mn><mml:mi>n</mml:mi><mml:mo stretchy="false">)</mml:mo><mml:mmultiscripts><mml:mn>1</mml:mn><mml:mprescripts/><mml:none/><mml:mn>285</mml:mn></mml:mmultiscripts><mml:mn>14</mml:mn></mml:math>
Abstract
The new, neutron-deficient, superheavy element isotope $^{285}114$ was produced in $^{48}\mathrm{Ca}$ irradiations of $^{242}\mathrm{Pu}$ targets at a center-of-target beam energy of 256 MeV (${E}^{*}=50\text{ }\text{ }\mathrm{MeV}$). The $\ensuremath{\alpha}$ decay of $^{285}114$ was followed by the sequential $\ensuremath{\alpha}$ decay of four daughter nuclides, $^{281}\mathrm{Cn}$, $^{277}\mathrm{Ds}$, $^{273}\mathrm{Hs}$, and $^{269}\mathrm{Sg}$. $^{265}\mathrm{Rf}$ was observed to decay by spontaneous fission. The measured $\ensuremath{\alpha}$-decay $Q$ values were compared with those from a macroscopic-microscopic nuclear mass model to give insight into superheavy element shell effects. The $^{242}\mathrm{Pu}(^{48}\mathrm{Ca},5n)^{285}114$ cross section was ${0.6}_{\ensuremath{-}0.5}^{+0.9}\text{ }\text{ }\mathrm{pb}$.
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