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Nuclear Physics Advisory Panel (NPAP) report (PDF-3.8 MB) - STFC

Nuclear Physics Advisory Panel (NPAP) report (PDF-3.8 MB) - STFC

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Report of <strong>Nuclear</strong> <strong>Physics</strong> <strong>Advisory</strong> <strong>Panel</strong><br />

The physics of Nuclei, <strong>Nuclear</strong> Matter and Nucleosynthesis<br />

A2.3 Nuclei at extreme spins; breaking through the spin barrier<br />

One of the important tests of our<br />

understanding of nuclear matter is to test<br />

it at the extremes. One possible extreme<br />

is the highest angular momentum or spin.<br />

Nuclei can generate angular momentum<br />

in a number of ways, but one possibility is<br />

that the nucleons move collectively<br />

aligning their individual orbital motion with<br />

a collective axis. Eventually all of the<br />

valence particles have aligned their<br />

angular momentum, the question is can<br />

the nucleus then be made to spin any<br />

faster, if so how? In measurements led by<br />

UK researchers the nucleus 158 Er was<br />

spun not only up to the hypothetical<br />

maximum of 45 hbar, but was found to<br />

spin up to an incredible 65 hbar. The<br />

nucleus achieves this by breaking open<br />

the core to create more valence particles<br />

to align.<br />

E. Paul et al. Physical Review Letters 98, 012501 (2007)<br />

The evolution of the structure of the nucleus<br />

158 Er with increasing spin<br />

A2.4 Quark-Gluon Plasma<br />

(QGP)<br />

One of the greatest frontiers<br />

is the understanding the nature of<br />

matter at an instant after the big<br />

bang. This is the point in time in<br />

which the Universe consisted<br />

mainly of quarks of gluons, these<br />

then condensed/froze out into<br />

hadrons. The experiments at RHIC<br />

which collide Gold nuclei at<br />

relativistic energies permit the<br />

conditions of the early Universe to<br />

be recreated and this new phase of<br />

matter to be probed. The UK is a<br />

member of the STAR collaboration<br />

and hold important positions. The<br />

novelty of the science has meant<br />

the output has been prolific. Key<br />

Evidence for jet quenching found at RHIC<br />

PRL 90 083202<br />

discoveries made with STAR are the superfluid character of the QGP and the<br />

observation of jet suppression when jets pass through the QGP region. It is believed<br />

that one of the keys to understanding the nature of the QGP is characterising the<br />

attenuation of the jets. This will form a key part of the ALICE programme. There have<br />

been 15 Physical Review Letters published from STAR analysis over the last 3 years.<br />

= 29 =

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