Nuclear Astrophysics Research with the MUSIC Detector at ATLAS and FRIB

Jun 9, 2025, 4:14 PM
22m
Old Madison

Old Madison

Parallel session presentation Particle and Nuclear Astrophysics Particle and Nuclear Astrophysics

Speaker

Eilens Lopez Saavedra (Argonne National laboratory)

Description

Reliable (α,n), (α,p), and (p,α) cross sections and reaction rates are critical to modeling nucleosynthesis in novae, X-ray bursts, and neutrino-driven winds, yet direct measurements at astrophysically relevant energies remain limited. \par
The Multi-Sampling Ionization Chamber (MUSIC) active-target detector is designed for precise measurements of ionization energy loss in nuclear reactions. In this talk the working principle of MUSIC will be discussed , its role in studying α-induced reactions, and recent experimental highlights including recent MUSIC campaigns at Argonne’s ATLAS and FRIB such as the first excitation function for the reaction (^{59}\mathrm{Cu}(p,\alpha)^{56}\mathrm{Ni}) importatnt to understand the Ni-Cu cycle and the key hot-CNO reaction (^{14}\mathrm{O}(\alpha,p)^{17}\mathrm{F}).

This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under contract number DE-AC02-06CH11357.

Primary author

Eilens Lopez Saavedra (Argonne National laboratory)

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