ADOPTED LEVELS for 93Ag

Author: Balraj Singh |  Citation: ENSDF |  Cutoff date: 31-JUL-2016 

Author: Coral M. Baglin |  Citation: Nucl. Data Sheets 112, 1163 (2011) |  Cutoff date: 15-Dec-2010 

 Full ENSDF file | Adopted Levels (PDF version) 


S(n)= 17120 keV CAS(p)= -1510 keV SYQ(α)= -2660 keV SY
Reference: 2012WA38,1997MO25

General Comments:

The 93Ag isotope is expected to be unbound towards proton emission.

1994He28: a few events (≈4 per 1014 106Cd ions) were tentatively assigned to 93Ag in Ni(106Cd,X),E=60 MeV/nucleon using projectile fragment separator at NSCL-MSU facility; however, the attribution of these events to contamination from neighboring peaks in the Z and Q spectra could not be ruled out. The flight time through the separator, was on the order of 150 ns.

1995Ry03: few events were very tentatively assigned to 93Ag in Ni(112Sn,X),E=58,62 MeV/nucleon using LISE3 separator at GANIL. Time of flight was ≈1.5 μs.

2008KrZW: 93Ag from fragmentation of 1 GeV/nucleon 124Xe beam; fragment recoil separator at GSI; ΔE, tof and magnetic rigidity measurements used for fragment identification; fragments stopped in Si implantation detector and β absorber (SIMBA).

2016Ce02: 93Ag nuclide produced and identified at RIBF-RIKEN facility in 9Be(124Xe,X) reaction at E=345 MeV/nucleon with an average beam intensity of 30 pnA. Identification of 93Ag was made by determining atomic Z and mass-to-charge ratio α/Q, where Q=charge state of the ions. The selectivity of ions was based on magnetic rigidity, time-of-flight and energy loss using BigRIPS separator and zero degree spectrometer ZDS. The separated nuclei were implanted in a wide range silicon-strip stopper array for ion and β particle detection WAS3ABi, consisting of three highly-segmented 1 mm thick double-sided silicon detectors, a stack of ten segmented 1 mm thick single-sided silicon strip detectors. The γ rays were detected by EURICA array of 84 HPGe detectors surrounding the WAS3ABi system. In addition an array of 18 LaBr3(Ce) detectors was used for γ detection in fast-timing measurements. α total of 31 events were assigned to 93Ag. 2015MoZZ is a conference report from the same group as 2016Ce02

Theoretical calculations of g.s. properties: 1997He24 (shell model), 2001Pa02 (relativistic mean field), 2001La01, 2002La37 (relativistic Hartree-Bogoliubov theory).

Q-value: Estimated uncertainties (2012Wa38): 710 for S(p), 620 for Q(α)

Q-value: S(p) and Q(α) from 2012Wa38, S(n) from 1997Mo25

Q-value: S(2p)=2050 640, Q(εp)=9440 500 (syst,2012Wa38). S(2n)=31850 (theory,1997Mo25)




E(level)
(keV)
T1/2(level)
  0 228 ns 16 
% ε = ?
% εp = ?
% p = ?

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Additional Level Data and Comments:

E(level)Jπ(level)T1/2(level)Comments
  0 228 ns 16 
% ε = ?
% εp = ?
% p = ?
α total of 31 events were assigned to 93Ag by 2016Ce02, which are assumed to correspond to the g.s. activity of 93Ag.
E(level): α total of 31 events were assigned to 93Ag by 2016Ce02, which are assumed to correspond to the g.s. activity of 93Ag.

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