10,777 research outputs found
Why Select and Remain in my University: Re-examining Higher Education in South Africa
Tertiary institutions have a major role in providing relevant education that best meets the needs of the various constituencies served. To meet these needs an assessment of factors that influence their choices becomes imperative. As a result of the governments' policy to transform higher education in South Africa and the challenges brought about by globalisation and internationalisation, tertiary institutions are facing new challenges. Attracting quality students in a highly competitive education environment is crucial as the numbers of students' dropping out especially call attention to wastage in government funding. This paper examines some of the criteria used by South-African students, when choosing or evaluating a tertiary institution. The main findings include a significant positive link among trust in management, satisfaction with transport, perception of readiness for change and overall satisfaction with the university. These variables have indirect relationship with satisfaction with transport and living arrangement of students. Practical implications, limitations and suggestions for future studies were articulated
Measuring Service Quality in South Africa Higher Education: Developing a Multidimensional Scale
Increased competition in the educational environment has contributed to the growing importance of service quality measurement at higher education institutions. This paper investigates aspects of service quality in higher education as a step towards developing a standardised scale for its measurement. Using structured questionnaires, survey data was collected from students (n = 391) from two South African universities. Findings indicate that the service quality in higher education scale is a multidimensional construct loading on 13 factors with reasonable reliability coefficient and some construct validity. Significant relationships were found among a number of study variables. Some further research directions were suggested and policy implications discussed
HESS J1825-137: A pulsar wind nebula associated with PSR B1823-13?
HESS J1825-137 was detected with a significance of 8.1 in the
Galactic Plane survey conducted with the H.E.S.S. instrument in 2004. Both HESS
J1825-137 and the X-ray pulsar wind nebula G18.0--0.7 (associated with the
Vela-like pulsar PSR B1823-13) are offset south of the pulsar, which may be the
result of the SNR expanding into an inhomogeneous medium. The TeV size ( pc, for a distance of 4 kpc) is times larger than the X-ray size,
which may be the result of propagation effects as a result of the longer
lifetime of TeV emitting electrons, compared to the relatively short lifetime
of keV synchrotron emitting electrons. The TeV photon spectral index of can also be related to the extended PWN X-ray synchrotron photon index of
, if this spectrum is dominated by synchrotron cooling. The
anomalously large size of the pulsar wind nebula can be explained if the pulsar
was born with a relatively large initial spindown power and braking index
, provided that the SNR expanded into the hot ISM with relatively low
density ( cm).Comment: 4 pages, 4 figures, to appear in the Proc. of the 29th International
Cosmic Ray Conference, OG Sessio
K^+ -> pi^+ nu nu-bar and K_L -> pi^0 nu nu-bar Decays in the General MSSM
We reanalyze the rare decays K^+ -> pi^+ nu nu-bar and K_L -> pi^0 nu nu-bar
in a general MSSM with conserved R-parity. Working in the mass eigenstate basis
and performing adaptive scanning of a large space of supersymmetric parameters,
16 parameters in the constrained scan and 63 in the extended scan, we find that
large departures from the Standard Model expectations are possible while
satisfying all existing constraints. Both branching ratios can be as large as a
few times 10^{-10} with Br(K_L -> pi^0 nu nu-bar) often larger than Br(K^+ ->
pi^+ nu nu-bar) and close to its model independent upper bound. We give
examples of supersymmetric parameters for which large departures from the SM
expectations can be found and emphasize that the present 90% C.L. experimental
upper bound on Br(K^+ -> pi^+ nu nu-bar) gives a non trivial constraint on the
MSSM parameter space. Unlike previous analyses, we find that chargino box
diagrams can give, already for moderately light charged sleptons, a significant
contribution. As a byproduct we find that the ranges for the angles beta and
gamma in the unitarity triangle are relaxed due to the presence of new
CP-violating phases in K^0 - K^0-bar and B^0_d - B^0_d-bar mixing to 12 degrees
<= beta <= 27 degrees and 20 degrees <= gamma <= 110 degrees.Comment: 36 pages, 27 figures, latex, uses axodraw.st
Weak Quasi-elastic Production of Hyperons
The quasielastic weak production of and hyperons from
nucleons and nuclei induced by antineutrinos is studied in the energy region of
some ongoing neutrino oscillation experiments in the intermediate energy
region. The hyperon nucleon transition form factors determined from neutrino
nucleon scattering and an analysis of high precision data on semileptonic
decays of neutron and hyperons using SU(3) symmetry have been used. The nuclear
effects due to Fermi motion and final state interaction effects due to hyperon
nucleon scattering have also been studied. The numerical results for
differential and total cross sections have been presented.Comment: 26 pages, 10 figure
Eerste kwartaal 2011 melkvee: melkprijs en saldo boven langjarig gemiddelde
De gestegen melkprijs in het eerste kwartaal 2011 kan de hogere voerkosten ruim compenseren. Hierdoor ligt het saldo van de melkveebedrijven in het eerste kwartaal hoger dan in dezelfde periode van 2010
Development of Drum-Buffer-Rope scheduling software to support a âwhat ifâ approach to scheduling job shops
Thesis (MScEng (Industrial Engineering))--University of Stellenbosch, 2006.The Theory of Constraints is a management philosophy based on the underlying assumption that
only a few constraining factors limit the throughput of the entire system. Drum-Buffer-Rope is
the production logistical solution of the Theory of Constraints. It is the implementation of
Constraints Management on the manufacturing shop floor, to manage physical resource
constraints. Drum-Buffer-Rope was designed with the purpose of increasing Throughput, while
simultaneously decreasing Inventory, and minimising Operating Expense. It aims to accomplish
these goals by focusing on simplifying and therefore reducing variability in the production
process, and ultimately protecting order due dates against disruptions.
The dynamic conditions under which typical job shops operate can make Constraints
Management of the resource constraints a cumbersome task. By following a âWhat Ifâ approach
to the scheduling process, the scheduler can play an interactive role in developing practical shop
floor schedules. In this way the scheduler can see the results of his/her ideas on the shop floor
situation quickly as immediate feedback is provided. The Drum-Buffer-Rope methodology only
finite schedules certain points in the manufacturing process therefore scheduling calculations can
be performed quickly if done in software. This makes it possible for the scheduler to analyse
various scenarios in a short period of time and allowing the development of near optimal shop
floor schedules by following a âWhat Ifâ approach to scheduling.
In this project, new developments in the field of Drum-Buffer-Rope were investigated, and the
newly developed Simplified Drum-Buffer-Rope methodology was researched. The
methodologies were incorporated in a fully developed software package that uses Drum-Buffer-
Rope or Simplified Drum-Buffer-Rope to marry the intrinsic knowledge of the shop-floor worker
with modern day computer technology to create production schedules that can be released to the
shop floor. Schedules are created rapidly enough by the software to enable the scheduler to
follow a âWhat Ifâ approach to create near optimal shop floor schedules. The developed software
was used with live data from a South African job shop to illustrate the âWhat Ifâ approach to
Simplified Drum-Buffer-Rope scheduling. The results show that throughput can be increased and
operating expense decreased, therefore increasing bottom line results, by analysing various
scenarios
A Model of the Spectral Evolution of Pulsar Wind Nebulae
Recent observations suggest that many old pulsar wind nebulae (PWNe) are
bright TeV gamma-ray sources without a strong X-ray counterpart. In this paper,
we study the spectral evolution of PWNe taking into account the energy which
was injected when they were young for old PWNe. We model the evolution of the
magnetic field and solve for the particle distribution inside a uniformly
expanding PWN. The model is calibrated by fitting the calculated spectrum to
the observations of the Crab Nebula at an age of a thousand years. We find that
only a small fraction of the injected energy from the Crab Pulsar goes to the
magnetic field, consistent with previous studies. The spectral evolution model
of the Crab Nebula shows that the flux ratio of TeV gamma-rays to X-rays
increases with time, which implies that old PWNe are faint at X-rays, but not
at TeV gamma-rays. The increase of this ratio is primarily because the magnetic
field decreases with time and is not because the X-ray emitting particles are
cooled more rapidly than the TeV gamma-ray emitting particles. Our spectral
evolution model matches the observed rate of the radio flux decrease of the
Crab Nebula.Comment: 5 pages, 3 figures. Proc. of the 2009 Fermi Symposium, Washington,
DC, Nov 2-5; eConf Proceedings C09112
- âŠ