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- From: Somogyi Gábor <somogyi.gabor AT wigner.hu>
- To: rmkiusers AT lists.kfki.hu, fizinfo AT lists.kfki.hu
- Subject: [Fizinfo] [Rmkiusers] Wigner FK RMI Elméleti Osztály Szemináriuma
- Date: Mon, 31 Mar 2025 16:31:44 +0200
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Wigner FK RMI Elméleti Osztály Szemináriuma
Tisztelettel meghívjuk
Prof. Azwinndini Muronga
(Summerstrand Campus South, South Africa)
“The Need for Beyond Second-Order Dissipative Fluid Dynamics for Heavy Ion
Collisions and Astrophysics”
címmel tartandó szemináriumára.
Kivonat:
Accurate modelling of relativistic fluids under extreme conditions—such as
those encountered in heavy ion collisions and astrophysical phenomena like
neutron star mergers—requires a theoretical framework that extends beyond the
limitations of first- and second-order dissipative fluid dynamics. While
second-order theories, particularly the Israel-Stewart formalism, represent a
critical improvement over first-order approaches by restoring causality and
stability, they may fall short in far-from-equilibrium regimes where rapid
expansion, large gradients, and strong coupling effects dominate.
This talk motivates the necessity of pursuing fluid dynamic theories beyond
second order. We highlight three key reasons: (i) second-order approaches
serve as the minimal bridge between classical and relativistic regimes, (ii)
higher-order corrections depend on lower-order terms and may impose
additional constraints on equilibrium behaviour, and (iii) essential
couplings between dissipative processes—such as heat flow, shear, and bulk
viscosities—are only fully realized at third order and beyond.
We will explore recent theoretical advancements, including third-order
frameworks derived from kinetic theory and the entropy principle, and discuss
their applications in modelling quark-gluon plasma evolution, early-time
dynamics in heavy ion collisions, and relativistic transport in astrophysical
systems. By addressing these needs, beyond-second-order fluid dynamics offers
a more complete and predictive framework for studying complex relativistic
systems across energy scales and environments.
Helye: Wigner FK RMI III. ép. Tanácsterem
Ideje: 2025 április 4. péntek d.u. 14 óra
Szívesen látunk minden érdeklődőt.
Somogyi Gábor
- [Fizinfo] [Rmkiusers] Wigner FK RMI Elméleti Osztály Szemináriuma, Somogyi Gábor, 03/31/2025
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