1,000,477 research outputs found
Il-qima ta' Ġunone u l-Knisja ta' Santa Maria della Porta
Ġunone kienet meqjuma f’dawn il-gżejjer sa minn żmien il-Feniċi. Il-kittieba jgħidu li kienu waqqfulha maqdes fuq il-għolja fejn illum jinsab Sant’Anġlu. L-awtur jgħid li meta saru t-tiswijiet fil-bini tal-Imdina, kellha tinħatt ukoll fuq il-Knisja ta’ Santa Maria della Porta. Fejn kienet din il-knisja saret biċċa mill-bitħa tal-Palazz Maisterjali li llum hu magħruf bħala Connaught Hospital. Din l-informazzjoni joħodha minn dak li sab fl-arkivji G. Darmanin-Demajo.N/
Three-body Faddeev Calculation for 11Li with Separable Potentials
The halo nucleus Li is treated as a three-body system consisting of an
inert core of Li plus two valence neutrons. The Faddeev equations are
solved using separable potentials to describe the two-body interactions,
corresponding in the n-Li subsystem to a p resonance plus a
virtual s-wave state. The experimental Li energy is taken as input and
the Li transverse momentum distribution in Li is studied.Comment: 6 pages, RevTeX, 1 figur
Il-fjuretti ta' S. Franġisk
Il-Fjuretti ta’ San Franġisk jittrattaw dwar il-ħajja ta’ San Franġisk u tal-ewwel dixxiplu tiegħu. Dawn il-fjuretti huma traduzzjoni bit-Taljan u li l-oriġinal tagħhom inkitbu bil-Latin ftit wara l-1322.N/
-NMR of Isolated Li Implanted into a Thin Copper Film
Depth-controlled -NMR was used to study highly spin-polarized Li
in a Cu film of thickness 100 nm deposited onto a MgO substrate. The positive
Knight Shifts and spin relaxation data show that Li occupies two sites at
low temperatures, assigned to be the substitutional () and octahedral ()
interstitial sites. Between 50 to 100 K, there is a site change from to
. The temperature dependence of the Knight shifts and spin-lattice
relaxation rates at high temperatures, i.e. when all the Li are in the
site, is consistent with the Korringa Law for a simple metal.Comment: Accepted for publication in Phys. Rev.
Unbound exotic nuclei studied by transfer to the continuum reactions
In this paper we show that the theory of transfer reactions from bound to
continuum states is well suited to extract structure information from data
obtained by performing "spectroscopy in the continuum". The low energy unbound
states of nuclei such as Li and He can be analyzed and the
neutron-core interaction, necessary to describe the corresponding borromean
nuclei Li and He can be determined in a semi-phenomenological way.
An application to the study of Li is then discussed and it is shown that
the scattering length for s-states at threshold can be obtained from the ratio
of experimental and theoretical cross sections. The scattering single particle
states of the system n+Li are obtained in a potential model. The
corresponding S-matrix is used to calculate the transfer cross section as a
function of the neutron continuum energy with respect to Li. Three
different reactions are calculated ,
, , to check the
sensitivity of the results to the target used and in particular to the transfer
matching conditions. Thus the sensitivity of the structure information
extracted from experimental data on the reaction mechanism is assessed.Comment: 21 pages, 5 ps figures, accepted for publication on Nucl. Phys.
Non-Clinical Benefits of Evidence - Based Veterinary Medicine
<div><strong>Clinical bottom line</strong></div><ul><li>There are few studies addressing business benefits of EBVM.</li><li>While the need for a wider adoption of EBVM has been highlighted and linked to commercial benefits, further empirical studies are needed to identify and quantify such linkages.</li></ul><p><br /> <img src="https://www.veterinaryevidence.org/rcvskmod/icons/oa-icon.jpg" alt="Open Access" /> <img src="https://www.veterinaryevidence.org/rcvskmod/icons/pr-icon.jpg" alt="Peer Reviewed" /></p
Three Li-rich K giants: IRAS 12327-6523, IRAS 13539-4153, and IRAS 17596-3952
We report on spectroscopic analyses of three K giants previously suggested to
be Li-rich: IRAS 12327-6523, IRAS 13539-4153, and IRAS 17596-3952.
High-resolution optical spectra and the LTE model atmospheres are used to
derive the stellar parameters: (, log , [Fe/H]), elemental
abundances, and the isotopic ratio C/C. IRAS 13539-4153 shows an
extremely high Li abundance of (Li) 4.2, a value ten
times more than the present Li abundance in the local interstellar medium. This
is the third highest Li abundance yet reported for a K giant. IRAS 12327-6523
shows a Li abundances of (Li) 1.4. IRAS 17596-3952 is a
rapidly rotating ( 35 km s) K giant with
(Li) 2.2. Infrared photometry which shows the presence
of an IR excess suggesting mass-loss. A comparison is made between these three
stars and previously recognized Li-rich giants.Comment: 17 pages, 6 figures, accepted for A
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