13-19 May 2018
Venice, Italy
Europe/Zurich timezone
The organisers warmly thank all participants for such a lively QM2018! See you in China in 2019!

The Power Spectrum of Heavy Ion Collisions

15 May 2018, 17:00
2h 40m
First floor and third floor (Palazzo del Casinò)

First floor and third floor

Palazzo del Casinò

Poster New theoretical developments Poster Session


Ms Meera Vieira Machado (Niels Bohr Institute)


Using features from Cosmic Microwave Background (CMB) analysis, we calculate the angular power spectrum of central heavy ion collisions at $ \sqrt{s_{NN}} = 5.02 \mathrm{TeV} $. The idea is to treat the particles' angular distribution like the background radiation originated from the recombination epoch of the early Universe. In practice, detector deficiencies and lack of full pseudorapidity ($\eta$) coverage introduce artificial structures to the power spectrum, which are related only to the geometric cuts, i.e. to the $ \eta $ range. We clarify this issue in order to determine what is the true power spectrum of an ideal detector. One can thus finally discover which properties of the Quark Gluon Plasma (QGP) can be seen through this type of analysis.

Content type Theory
Centralised submission by Collaboration Presenter name already specified

Primary author

Ms Meera Vieira Machado (Niels Bohr Institute)

Presentation Materials

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