Wednesday, June 20, 2012

Tin-100, a doubly magic nucleus

Tin-100, a doubly magic nucleus [ Back to EurekAlert! ] Public release date: 20-Jun-2012
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Contact: Dr. Andreas Battenberg
battenberg@zv.tum.de
49-892-891-0510
Technische Universitaet Muenchen

Key experiment in nuclear physics

Stable tin, as we know it, comprises 112 nuclear particles 50 protons and 632 neutrons. The neutrons act as a kind of buffer between the electrically repelling protons and prevent normal tin from decaying. According to the shell model of nuclear physics, 50 is a "magic number" that gives rise to special properties. Tin-100, with 50 protons and 50 neutrons, is "doubly magic," making it particularly interesting for nuclear physicists.

Shooting xenon-124 ions at a sheet of beryllium, the international team headed by physicists from the TU Muenchen, the Cluster of Excellence Origin and Structure of the Universe and the GSI in Darmstadt succeeded in creating tin-100 and analyzing its subsequent decay. Using specially developed particle detectors, they were able to measure the half-life and decay energy of tin-100 and its decay products. Their experiments confirmed that tin-100 has the fastest beta decay of all atomic nuclei, as previously predicted by theoretical physicists.

A repeat of the experiment is slated for the near future at the RIKEN research center in Japan. The beam intensity at RIKEN is higher in the mean time, allowing even more precise measurements. The aim of the research work is to improve the understanding of processes in the formation of heavy elements during explosions on the surface of compact stars. In addition, the researchers hope to draw conclusions on the neutrino mass from the measurements.

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This work was supported by the BMBF, by the GSI, by the DFG-Cluster of Excellence Origin and Structure of the Universe, by the EC within the FP6 through I3-EURONS and by the Swedish Research Council.

Original publication:

Superallowed Gamow-Teller Decay of the Doubly Magic Nucleus Sn-100, Hinke et al., Nature, 21. Juni 2012 DOI: 10.1038/nature11116



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Tin-100, a doubly magic nucleus [ Back to EurekAlert! ] Public release date: 20-Jun-2012
[ | E-mail | Share Share ]

Contact: Dr. Andreas Battenberg
battenberg@zv.tum.de
49-892-891-0510
Technische Universitaet Muenchen

Key experiment in nuclear physics

Stable tin, as we know it, comprises 112 nuclear particles 50 protons and 632 neutrons. The neutrons act as a kind of buffer between the electrically repelling protons and prevent normal tin from decaying. According to the shell model of nuclear physics, 50 is a "magic number" that gives rise to special properties. Tin-100, with 50 protons and 50 neutrons, is "doubly magic," making it particularly interesting for nuclear physicists.

Shooting xenon-124 ions at a sheet of beryllium, the international team headed by physicists from the TU Muenchen, the Cluster of Excellence Origin and Structure of the Universe and the GSI in Darmstadt succeeded in creating tin-100 and analyzing its subsequent decay. Using specially developed particle detectors, they were able to measure the half-life and decay energy of tin-100 and its decay products. Their experiments confirmed that tin-100 has the fastest beta decay of all atomic nuclei, as previously predicted by theoretical physicists.

A repeat of the experiment is slated for the near future at the RIKEN research center in Japan. The beam intensity at RIKEN is higher in the mean time, allowing even more precise measurements. The aim of the research work is to improve the understanding of processes in the formation of heavy elements during explosions on the surface of compact stars. In addition, the researchers hope to draw conclusions on the neutrino mass from the measurements.

###

This work was supported by the BMBF, by the GSI, by the DFG-Cluster of Excellence Origin and Structure of the Universe, by the EC within the FP6 through I3-EURONS and by the Swedish Research Council.

Original publication:

Superallowed Gamow-Teller Decay of the Doubly Magic Nucleus Sn-100, Hinke et al., Nature, 21. Juni 2012 DOI: 10.1038/nature11116



[ Back to EurekAlert! ] [ | E-mail | Share Share ]

?


AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert! system.


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