96 research outputs found
Long-term accumulation of soil carbon and nitrogen in grazed bermudagrass pastures
Last updated: 10/22/201
Recommandations specifiques d'engrais: Calibration et validation du module phosphore du modele NuMaSS
Fertiliser recommendations in Mali as well as in many other countries of West Africa were made according to Chaminade's method. For socio-economic reasons, correcting deficiency rates of major nutrients were vulgarized. These blanket recommendation, when applied, lead to a continuous soil nutrient mining. The objective of this research was to calibrate and validate the P module of NuMass. Laboratory incubations were conducted to calibrate the P buffering coefficients used by the P module. Rates of N, P and lime predicted by NuMass model, considered as specific recommendations, were compared to the blanket recommendations in the field in order to validate them. The buffer coefficients were inversely proportional to the clay content. The buffering coefficient of sandy soils of Cinzana/Mali (0.73) and Kollo/Niger P3 (0.63) were higher compared to the clayey soils of Longorola-bf (0.22) and Kollo/Niger (0.21). Generally, buffering coefficients obtained by laboratory incubation (0.60) tended to be lower than the estimated coefficient by the P module NuMass (0.67). The range of the used soil texture (1.5-54.6 % clay) showed that the buffering coefficients estimated by the P module of NuMass were correct for flooded soils. Grain yield of different trials and tests do not indicate the expected higher performance of specific recommendations of fertilisers from NuMass model compared to the used blanket recommendation (1624 and 1582 kg ha-1 of maize; respectively
First atom lifetime and scattering length measurements
The results of a search for hydrogen-like atoms consisting of
mesons are presented. Evidence for atom production
by 24 GeV/c protons from CERN PS interacting with a nickel target has been seen
in terms of characteristic pairs from their breakup in the same target
() and from Coulomb final state interaction (). Using
these results the analysis yields a first value for the atom lifetime
of fs and a first model-independent measurement of
the S-wave isospin-odd scattering length
( for isospin ).Comment: 14 pages, 8 figure
Determination of scattering lengths from measurement of atom lifetime
The DIRAC experiment at CERN has achieved a sizeable production of
atoms and has significantly improved the precision on its lifetime
determination. From a sample of 21227 atomic pairs, a 4% measurement of the
S-wave scattering length difference
has been attained, providing an important test of Chiral Perturbation Theory.Comment: 6 pages, 6 figure
Measurement of the 10 keV resonance in the B()Be reaction via the Trojan Horse Method
The B(p,)Be bare nucleus astrophysical S(E)-factor has
been measured for the first time at energies from about 100 keV down to about 5
keV by means of the Trojan Horse Method (THM). In this energy region, the
S(E)-factor is strongly dominated by the 8.699 MeV C level
(J=), producing an s-wave resonance centered at about
10 keV in the entrance channel. Up to now, only the high energy tail of this
resonant has been measured, while the low-energy trend is extrapolated from the
available direct data. The THM has been applied to the quasi-free
H(B,Be)n reaction induced at a boron-beam energy of
24.5 MeV. An accurate analysis brings to the determination of the
B(p,)Be S(E)-factor and of the corresponding electron
screening potential , thus giving for the first time an independent
evaluation of it.Comment: Authors thank the (anonymous) referee for detailed comments and
suggestions. The paper is already submitted to Physical Review
Investigation of pairs in the effective mass region near
The DIRAC experiment at CERN investigated in the reaction
the particle pairs and with relative momentum in the pair system less than 100 MeV/c.
Because of background influence studies, DIRAC explored three subsamples of
pairs, obtained by subtracting -- using time-of-flight (TOF) technique
-- background from initial distributions with sample fractions
more than 70\%, 50\% and 30\%. The corresponding pair distributions in and
in its longitudinal projection were analyzed first in a Coulomb model,
which takes into account only Coulomb final state interaction (FSI) and
assuming point-like pair production. This Coulomb model analysis leads to a
yield increase of about four at MeV/c compared to 100 MeV/c.
In order to study contributions from strong interaction, a second more
sophisticated model was applied, considering besides Coulomb FSI also strong
FSI via the resonances and and a variable distance
between the produced mesons. This analysis was based on three different
parameter sets for the pair production. For the 70\% subsample and with best
parameters, pairs was found to be compared to extracted by means of the Coulomb model. Knowing the efficiency
of the TOF cut for background suppression, the total number of detected
pairs was evaluated to be around , which agrees with
the result from the 30\% subsample. The pair number in the 50\%
subsample differs from the two other values by about three standard deviations,
confirming -- as discussed in the paper -- that experimental data in this
subsample is less reliable
New astrophysical S factor for the (15)N(p,gamma)(16)O reaction via the asymptotic normalization coefficient (ANC) method
Journals published by the American Physical Society can be found at http://publish.aps.org/The (15)N(p,gamma)(16)O reaction provides a path from the CN cycle to the CNO bi-cycle and CNO tri-cycle. The measured astrophysical factor for this reaction is dominated by resonant capture through two strong J(pi) = 1(-) resonances at E(R) = 312 and 962 keV and direct capture to the ground state. Asymptotic normalization coefficients (ANCs) for the ground and seven excited states in (16)O were extracted from the comparison of experimental differential cross sections for the (15)N((3)He,d)(16)O reaction with distorted-wave Born approximation calculations. Using these ANCs and proton and alpha resonance widths determined from an R-matrix fit to the data from the (15)N(p,alpha)(12)C reaction, we carried out an R-matrix calculation to obtain the astrophysical factor for the (15)N(p,gamma)(16)O reaction. The results indicate that the direct capture contribution was previously overestimated. We find the astrophysical factor to be S(0) = 36.0 +/- 6.0 keV b, which is about a factor of 2 lower than the presently accepted value. We conclude that for every 2200 +/- 300 cycles of the main CN cycle one CN catalyst is lost due to this reaction
Evidence for -atoms with DIRAC
We present evidence for the first observation of electromagnetically bound
-pairs (-atoms) with the DIRAC experiment at the CERN-PS.
The -atoms are produced by the 24 GeV/c proton beam in a thin Pt-target
and the and -mesons from the atom dissociation are analyzed in
a two-arm magnetic spectrometer. The observed enhancement at low relative
momentum corresponds to the production of 173 54 -atoms. The mean
life of -atoms is related to the s-wave -scattering lengths, the
measurement of which is the goal of the experiment. From these first data we
derive a lower limit for the mean life of 0.8 fs at 90% confidence level.Comment: 15 pages, 9 figure
- …