An analysis of the nuclear physics
Theoretical nuclear physics
The needs of the field far exceed the capabilities of the present state of the art in computers and computational methods. Some of the computational challenges facing nuclear physicists are described below. Since millions of collisions must be recorded from the finely divided, highly granular detectors, the total accumulated data volume will be close to one million gigabytes per year. The goal of this research internship is the testing of different detectors and the installing of improvements. The PHENIX detector focuses on the detection of leptons, photons, and hadrons in selected solid angles, with a high-rate capability, to emphasize the electromagnetic signatures of QGP formation. A prototype detector, an order of magnitude smaller, has recently succeeded in the development of the necessary new, high-purity, low-background materials and techniques. Proton decay was not observed, but this detector became the first to be able to count individual neutrino events from the Sun. Quantum Monte Carlo techniques, developed in the past few years, can predict the structures and simple reaction rates of light nuclei having up to 8 nucleons, using present supercomputers operating at about 10 gigaflops, i. Development of new schemes and novel concepts is continuously occurring. Due to these developments, unprecedented experiments can be performed in the near future to investigate problems in nuclear structure or nuclear astrophysics. Hall A houses two high-resolution magnetic spectrometers based on superconducting magnetic dipoles to bend the reaction products into their focal-plane detector systems.
Especially we are interested in the: - Deformation of stretched foils introduced by the beam pressure - Deformation of the foil caused by beam heating - Determination of absolute separations of two stretched foils using the capacity method The Measurements will be done at an ion source test bench.
We offer a research internship which is closely related to the above described facilities.
Although SNO will have a broad range of physics and astrophysics capabilities, its primary activity will be the detection of neutrinos from 8B decays in the Sun.
The detection of neutral mesons with high resolution and efficiency has been a long-standing technological challenge.
In the former case, experimental work needs to be done in the accelerator area of the institute. Thereby you will contribute to the analysis of a experiment. Silicon detectors close to the beam pipe provide nearly full solid-angle coverage for particle detection.
Their aim is to optimise the lay-out of the instrument or the beam intensity and purity of a rare isotope beam, i.
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