General Public - Atomic, Nuclear and Hadronic Physics

Atomic physics (or atom physics) is the field of physics that studies atoms as isolated systems composed of electrons and an atomic nucleus. It is primarily concerned with the arrangement of electrons around the nucleus and the processes by which these arrangements change.

Atomic Physics also deals with radiation. In this field, this Atomic Physics is very very related to medicin, since it provides important diagnose and therapy methods.

Part of the members of the ICC are specialized in the study of radiation transport in matter and its applications in dosimetry and medical physics

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Nuclear physics is the branch of physics devoted to the study of the atomic nucleus. It covers three different aspects: probing the fundamental particles (protons and neutrons) and their interactions, classifying and interpreting the properties of nuclei, and providing technological advances. One of the most recent interests in theoretical and experimental Nuclear Physics is the study of Nuclear Structure beyond the stability line.

Researchers at ICC study the structure and dynamics of nuclei beyond the stability line. The availability in the near future of intense and energetic beams of short lived nuclei will allow to confront those studies with the experiment.

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Another branch of Nuclear Physics is Hypernuclear Physics. A hypernucleus is a bound system of nucleons and one or more hyperons (baryons with strangeness content). Researchers at ICC study the structure, dynamics and the decays of hypenuclei.

Researchers at ICC study the structure, dynamics and the decays of hypenuclei and participate in some of the ongoing and future hypernuclear experimental programs (DAFNE, JLAB, MAMI-C, HypHI, PANDA), which will provide the decisive data for testing theoretical predictions.

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Nuclear Physics is also closely related to Astrophysics, in particular when studing the composition and structure of compact stars. A compact star is formed from the collapsed remnant of a massive star, a Type II, Type Ib, or Type Ic supernova and models predict that it consists mostly of neutrons. It is a very hot star supported by the Pauli exclusion principle repulsion between neutrons. A compact star is one of the few possible conclusions of stellar evolution. The crucial ingredient to undertant its properties is the Nuclear Matter Equation of State.

Researchers of the ICC are making an important effort in the construction of realistic Nuclear Matter Equations of State.

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A field originally developed from Nuclear Physics is hadron physics. Hadron physics concerns the study of particles which interact through the strong force (hadrons). Protons and neutrons, which build the atomic nucleus, are the most familiar examples of hadrons. Hadrons are composed of quarks and gluons.

Researchers of the ICC study the properties of hadrons in the nuclear medium (finite density and temperature), and use effective models and lattice QCD simulations to describe the interaction among hadrons at low energies.

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Under extreme conditions of temperature, hadrons may lose their identity and dissolve in a new state of matter, the so called quark-gluon plasma, similar to the primordial matter in the early Universe. These conditions can be reproduced in heavy ion collision experiments. The experimental results provide circunstancial evidence for a new phase of matter exixting above a temperature of about 170 MeV. In future experiments at CERN-LHC this research program will be continued towards higher temperatures and smaller net baryon densities. Another relativistic heavy ion experiment (FAIR at GSI) will study the hadron mater - quark gluon plasma phase transition in the region of smaller temperature, but high baryon density.

The ICC participates in the development of the LHC and FAIR facilities and some of the scheduled experiments.

 

Learn more about Nuclear Physics

http://www.lbl.gov/abc/index.html
  • The ABC of Nuclear Science - A brief introduction to Nuclear Science. It looks at Antimatter, Beta rays, Cosmic connection and much more. Visit here and learn about radioactivity - alpha, beta and gamma decay. Find out the difference between fission and fusion. Learn about the structure of the atomic nucleus. Learn how elements on the earth were produced. Do you know that you are being bombarded constantly by nuclear radiation from the Cosmos? Discover if there are radioactive products found in a grocery store. Do you know if you have ever eaten radioactive food? Find out what materials are needed to shield us from alpha, beta, gamma, radiation. Discover what have we gained by its study.

http://www.lbl.gov/abc/index.html
  • Neutron Stars and Pulsars - A web page about neutron stars. A neutron star is about 20 km in diameter and has the mass of about 1.4 times that of our Sun. This means that a neutron star is so dense that on Earth, one teaspoonful would weigh a billion tons! Because of its small size and high density, a neutron star possesses a surface gravitational field about 2 x 1011 times that of Earth. Neutron stars can also have magnetic fields a million times stronger than the strongest magnetic fields produced on Earth.