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EMMI Workshop: Light-ion collisions 2026

21.–25. Sept. 2026
Kirchhoff-Institut für Physik (KIP)
Europe/Berlin Zeitzone

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Sitzung

Neutron Skin, EOS

24.09.2026, 09:00
HS2 (Kirchhoff-Institut für Physik (KIP))

HS2

Kirchhoff-Institut für Physik (KIP)

Im Neuenheimer Feld 227 69120 Heidelberg

Präsentationsmaterialien

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  1. 5. QCD phase diagram with heavy and light ion collisions and connection to neutron stars
    Prof. Jacquelyn Noronha-Hostler (University of Illinois Urbana-Champaign)
    24.09.26, 09:00
    Theoretical

    What are the properties and phases of many-body QCD matter as we vary the temperature and densities of the system?
    Due to the Fermion sign problem, we cannot directly map out the QCD phase diagram from first principles. Instead, we require interdisciplinary constraints and phenomenological studies to reverse engineer information from A-A collisions, low-energy nuclear experiments,...

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  2. 84. From neutron skins to neutron stars
    Charles Horowitz (Indiana University)
    24.09.26, 09:25
    Theoretical
  3. 85. PUMA - status and prospects
    Alexandre Obertelli (TU Darmstadt)
    24.09.26, 09:50
    Experimental
  4. 49. Probing 48Ca neutron skin measurement capabilities at the LHC
    Maxim Virta (Niels Bohr Institute)
    24.09.26, 10:05
    Theoretical

    In neutron-heavy ions, the neutrons are anticipated to accumulate closer to the surface of the nucleus, known as the neutron skin effect. Measurements conducted by PREX and CREX collaborations have found the neutron skin effect in $^{208}$Pb and $^{48}$Ca ions, using parity-violating electron scattering. However, some discrepancies remain in comparison with ab initio calculations. These...

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