505 research outputs found
Trapped-ion decay spectroscopy towards the determination of ground-state components of double-beta decay matrix elements
A new technique has been developed at TRIUMF's TITAN facility to perform
in-trap decay spectroscopy. The aim of this technique is to eventually measure
weak electron capture branching ratios (ECBRs) and by this to consequently
determine GT matrix elements of decaying nuclei. These branching
ratios provide important input to the theoretical description of these decays.
The feasibility and power of the technique is demonstrated by measuring the
ECBR of Cs.Comment: 9 pages, 9 figure
First direct mass-measurement of the two-neutron halo nucleus 6He and improved mass for the four-neutron halo 8He
The first direct mass-measurement of He has been performed with the
TITAN Penning trap mass spectrometer at the ISAC facility. In addition, the
mass of He was determined with improved precision over our previous
measurement. The obtained masses are (He) = 6.018 885 883(57) u and
(He) = 8.033 934 44(11) u. The He value shows a deviation from
the literature of 4. With these new mass values and the previously
measured atomic isotope shifts we obtain charge radii of 2.060(8) fm and
1.959(16) fm for He and He respectively. We present a detailed
comparison to nuclear theory for He, including new hyperspherical harmonics
results. A correlation plot of the point-proton radius with the two-neutron
separation energy demonstrates clearly the importance of three-nucleon forces.Comment: 4 pages, 2 figure
Elucidation of the anomalous A = 9 isospin quartet behaviour
Recent high-precision mass measurements of Li and Be, performed
with the TITAN Penning trap at the TRIUMF ISAC facility, are analyzed in light
of state-of-the-art shell model calculations. We find an explanation for the
anomalous Isobaric Mass Multiplet Equation (IMME) behaviour for the two = 9
quartets. The presence of a cubic = 6.3(17) keV term for the =
3/2 quartet and the vanishing cubic term for the excited =
1/2 multiplet depend upon the presence of a nearby = 1/2 state in
B and Be that induces isospin mixing. This is contrary to previous
hypotheses involving purely Coulomb and charge-dependent effects. = 1/2
states have been observed near the calculated energy, above the = 3/2
state. However an experimental confirmation of their is needed.Comment: 5 pages, 2 figure
First Penning-trap mass measurement in the millisecond half-life range: the exotic halo nucleus 11Li
In this letter, we report a new mass for Li using the trapping
experiment TITAN at TRIUMF's ISAC facility. This is by far the shortest-lived
nuclide, , for which a mass measurement has ever been
performed with a Penning trap. Combined with our mass measurements of
Li we derive a new two-neutron separation energy of 369.15(65) keV: a
factor of seven more precise than the best previous value. This new value is a
critical ingredient for the determination of the halo charge radius from
isotope-shift measurements. We also report results from state-of-the-art
atomic-physics calculations using the new mass and extract a new charge radius
for Li. This result is a remarkable confluence of nuclear and atomic
physics.Comment: Formatted for submission to PR
First direct Be electron capture -value measurement towards high-precision BSM neutrino physics searches
We report the first direct measurement of the nuclear electron capture (EC)
decay -value of Be Li via high-precision Penning
trap mass spectrometry (PTMS). This was performed using the LEBIT Penning trap
located at the National Superconducting Cyclotron Laboratory/Facility for Rare
Isotope Beams (NSCL/FRIB) using the newly commissioned Batch-Mode Ion-Source
(BMIS) to deliver the unstable Be samples. With a measured value of
= 861.963(23) keV this result is also three times more precise than
any previous determination of this quantity. This improved precision, and
accuracy of the Be EC decay -value is critical for ongoing experiments
that measure the recoiling nucleus in this system as a signature to search for
beyond Standard Model (BSM) neutrino physics using Be-doped superconducting
sensors
Mass Measurement of P for Improved Type-I X-ray Burst Modeling
Light curves are the primary observable of type-I x-ray bursts. Computational
x-ray burst models must match simulations to observed light curves. Most of the
error in simulated curves comes from uncertainties in process reaction
rates, which can be reduced via precision mass measurements of
neutron-deficient isotopes in the process path. We perform a precise
atomic mass measurement of P and use this new measurement to update
existing type-I x-ray burst models to produce an improved light curve.
High-precision Penning trap mass spectrometry was used to determine the
atomic mass of P. Modules for Experiments in Stellar Astrophysics (MESA)
was then used to simulate x-ray bursts using a 1D multi-zone model to produce
updated light curves. The mass excess of P was measured to be
-670.7 0.6 keV, a fourteen-fold precision increase over the mass reported
in AME2020. The Si()P and reverse photodisintegration
reaction rates have been determined to a higher precision based on the new,
high precision mass measurement of P, and MESA light curves generated
using these rates. Changes in the mass of P seem to have minimal effect
on XRB light curves, even in burster systems tailored to maximize impact.
The mass of P does not play a significant role in x-ray burst light
curves. It is important to understand that more advanced models don't just
provide more precise results, but often qualitatively different ones. This
result brings us a step closer to being able to extract stellar parameters from
individual x-ray burst observations. In addition, the Isobaric Multiplet Mass
Equation (IMME) has been validated for the quartet, but only
after including a small, theoretically predicted cubic term and utilizing an
updated excitation energy for the isobaric analogue state of Si.Comment: 8 pages, 7 figure
Penning-Trap Mass Measurements of the Neutron-Rich K and Ca Isotopes: Resurgence of the N = 28 Shell Strength
We present Penning-trap mass measurements of neutron-rich 44,47-50K and
49,50Ca isotopes carried out at the TITAN facility at TRIUMF-ISAC. The 44K mass
measurement was performed with a charge-bred 4+ ion utilizing the TITAN EBIT,
and agrees with the literature. The mass excesses obtained for 47K and 49,50Ca
are more precise and agree with the values published in the 2003 Atomic Mass
Evaluation (AME'03). The 48,49,50K mass excesses are more precise than the
AME'03 values by more than one order of magnitude. For 48,49K, we find
deviations by 7 sigma and 10 sigma, respectively. The new 49K mass excess
lowers significantly the two-neutron separation energy at the neutron number
N=30 compared with the separation energy calculated from the AME'03 mass-excess
values, and thus, increases the N=28 neutron-shell gap energy at Z=19 by
approximately 1 MeV.Comment: 6 pages, 5 figures, accepted for PR
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