Quick search Find article
Quick search
Find article

On some spectral properties of billiards and nuclei—similarities and differences

A Richter

Show affiliations


Generic and non-generic features of billiards and nuclei which show up in certain spectral properties are discussed by way of selected examples. Firstly, the short- and long-range correlations of levels belonging to the magnetic dipole Scissors Mode in heavy deformed nuclei at an excitation energy of about 3 MeV prove that this mode is indeed caused by an ordered or regular collective motion. Secondly, the fine structure distribution of the so-called electric Pygmy Dipole Resonance around 6–7 MeV excitation energy seems to indicate a situation where the spectral properties are governed by mixed dynamics, i.e. by regular and chaotic features. However, in nuclei quantitative conclusions are always severely hampered by missing levels due to limited experimental resolution and detector efficiency. Thirdly, it is shown that this situation can be largely overcome by studying spectral properties in superconducting microwave billiards considered as nuclear analogues. As an example resonance strength distributions in billiards of mixed and fully chaotic dynamics are considered. Finally, it is demonstrated how symmetry breaking effects in nuclei—e.g. isospin symmetry breaking—can be studied through those resonance strength distributions by modelling the nuclear problem with coupled billiards.


PACS

05.45.Mt Quantum chaos; semiclassical methods

21.10.Ky Electromagnetic moments

24.60.Lz Chaos in nuclear systems

21.10.Pc Single-particle levels and strength functions

21.10.Hw Spin, parity, and isobaric spin

21.10.Jx Spectroscopic factors

Subjects

Nuclear physics

Statistical physics and nonlinear systems

Dates

Issue T125 (July 2006)

Received 5 August 2005, accepted for publication 1 September 2005

Published 28 June 2006



  1. On some spectral properties of billiards and nuclei—similarities and differences

    A Richter 2006 Phys. Scr. 2006 167

  2. Magnetic dipole and Gamow–Teller modes: quenching, fine structure and astrophysical implications

    A Richter 2005 J. Phys.: Conf. Ser. 20 13

  3. Superconductivity at 53.5 K in GdFeAsO1−δ

    Jie Yang et al 2008 Supercond. Sci. Technol. 21 082001

  4. Visualization of avalanches in magnetic thin films: temporal processing

    Alessandro Magni et al J. Stat. Mech. (2009) P01020

  5. DNA uptake into nuclei: numerical and analytical results

    Zénó Farkas et al 2003 J. Phys.: Condens. Matter 15 S1767

  6. The Hopf algebra approach to Feynman diagram calculations

    Kurusch Ebrahimi-Fard and Dirk Kreimer 2005 J. Phys. A: Math. Gen. 38 R385

  7. Dynamical versus statistical mesoscopic models for DNA denaturation

    Marc Joyeux and Ana-Maria Florescu 2009 J. Phys.: Condens. Matter 21 034101

  8. Classical dynamics of a non-integrable Hamiltonian near coupling-induced resonance islands

    Marc Joyeux 1996 J. Phys. A: Math. Gen. 29 5963

  9. Gravitational wave tails and binary star systems

    L Blanchet and G Schafer 1993 Class. Quantum Grav. 10 2699

  10. Examples of Newtonian limits of relativistic spacetimes

    Jürgen Ehlers 1997 Class. Quantum Grav. 14 A119

View by subject




Export








Please login to access our web services, or create an account if you don't yet have one.

You must have cookies enabled in your web browser to be able to login.

Username
Password

Forgotten your password? Get a new one here.