2-5 October 2017
Hotel Intourist Kolomenskoye 4*
Europe/Moscow timezone

Search for $2p$ decay of the first excited state of $^{17}$Ne

4 Oct 2017, 09:30
15m
Moskvorechye-2 hall (Hotel Intourist Kolomenskoye 4*)

Moskvorechye-2 hall

Hotel Intourist Kolomenskoye 4*

Kashyrskoye shosse, 39B, Moscow, Russia, 115409
Plenary/section talk Nuclear physics Nuclear physics - 1

Speaker

Mr. Pavel Sharov (Joint Institute for Nuclear Research)

Description

Structure of nuclei located near and beyond the drip-lines plays important role in the explosive astrophysical processes. The problem of two-proton decay of the $^{17}$Ne first excited state is a good example of such situation. The two-proton radiative capture is a possible bypass of the $^{15}$O waiting point in the rp-process. The rate of this process drastically depends on the $2p/\gamma$ branching ratio of the $^{17}$Ne first excited state. The first excited state of $^{17}$Ne (with $J^\pi = 3/2^{-}$) is located only 344 keV above the 2p decay threshold, and its $2p$ decay partial width is much less then the gamma-decay partial width. The existing experimental threshold for the $2p/\gamma$ ratio (0.77 %) [1] is a few orders of magnitude greater than theoretical predictions made for this value (2.5e-6)[2]. Experiments aimed at the measuring such low branching ratio require development of special methods. In the recent experiment at the ACCULINNA [3] fragment-separator (Flerov Lab. JINR) the two-proton decay of the low-lying states of $^{17}$Ne populated in the $p(^{18}$Ne$,d)^{17}$Ne transfer reaction were studied. Original combined-mass method was used in the experiment. This method allows to get relatively good energy resolution ($\sigma\sim 130$ keV) without serious restriction on luminosity. As result, new $2p/\gamma$ ratio threshold for the $^{17}$Ne $3/2^{-}$ state equal 0.016(3)% was achieved, that is about fifty times less than existing value. The proposed method is promising for the study of the searched $2p$ decay partial width at level of $\Gamma_{2p}/\Gamma_\gamma \approx 10^{-6}$ [1] [M. J. Chromik, et. al., Phys.Rev. C55 (2002) 024313] [2] [L. V. Grigorenko, M. V. Zhukov, Phys.Rev. C76 (2007) 014008] [3] http://aculina.jinr.ru/

Primary authors

Dr. Andrey Fomichev (Joint Institute for Nuclear Research) Prof. Gurgen Ter-Akopian (Joint Institute for Nuclear Research) Prof. Leonid Grigorenko (Joint Institute for Nuclear Research) Prof. Mikhail Golovkov (Joint Institute for Nuclear Research) Mr. Pavel Sharov (Joint Institute for Nuclear Research)

Presentation Materials

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