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The Large Hadron Collider - the World`s Largest Microscope
The Large Hadron Collider - the World`s Largest Microscope

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Multi-modal fission in collinear ternary cluster decay of 252Cf(sf, fff)
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... lower for lighter central fragments: For the case of the nonsymmetric CCT-decay with three different final fragments (Ni, Ca, Sn), two barriers corresponding to the interaction of A 3 with fragment A 1 or/and with A 2 are obtained, they can be plotted in a twodimensional contour as shown in Fig. 5. W ...
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... several hundred MeV using the relativistic Love-Franey effective interaction based on relativistic impulse approximation [35]. They well explained experimental data especially polarization observables for 16 O, 40,48 Ca, 90 Zr, and, 208 Pb by treating the exchange term. Sakaguchi et al. calibrated t ...
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... is very similar to QED but with 3 conserved “colour” charges In QED: • the electron carries one unit of charge • the anti-electron carries one unit of anti-charge • the force is mediated by a massless “gauge boson” – the photon In QCD: • quarks carry colour charge: • anti-quarks carry anti-charge: • ...
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... With increasing demand for high density magnetic recording devices a paradigm shift is required to overcome the super-paramagnetic limit. By using a high anisotropy material, such as L10 FePt, and heat assisted magnetic recording the areal density can be taken well beyond 1 Tbit/in2 . For FePt the g ...
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... Also, which process(es) lead to the baryon asymmetry of the universe? Which process(es) can predict the small ratio η? What is the nature of the dark-matter of the universe? How can the CBR look the same in all directions [16] when it comes from causally disconnected regions of space? This is referr ...
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... just the problem of three gravitating bodies, for example the Sun, Saturn and Uranus. The full problem cannot be solved analytically, are there some options? Neglecting interactions between the last two, we have two independent one–particle problems, Sun–Uranus and Sun–Saturn which can easily be sol ...
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... thanks goes to my advisor Colin Morningstar who had the confidence to put me on such an important project, and who had the patience to let me learn from my mistakes. I am also grateful to Keisuke (Jimmy) Juge, Matthew Bellis, David Richards, Robert Edwards, and George Fleming who took the time to an ...
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Microscopy of 2D Fermi Gases - Institut für Laserphysik
Microscopy of 2D Fermi Gases - Institut für Laserphysik

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Nuclear structure

Understanding the structure of the atomic nucleus is one of the central challenges in nuclear physics.
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