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The Collective Model

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... have either an Oblate (like the earth) or a Prolate (like a rugby ball) shape. ... For high angular momentum, deformations have a prolate shape. ... – PowerPoint PPT presentation

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Title: The Collective Model


1
The Collective Model
  • Aard Keimpema

2
Contents
  • Vibrational modes of nuclei
  • Deformed nuclei
  • Rotational modes of nuclei
  • Coupling between rotational and vibrational states

3
Nuclear vibrations
  • The absorbtion spectrum of nuclei can be
    understood in terms of vibrations and rotations
    of the nucleus.
  • Distortion of surface
  • is spherical harmonic, ? is the
    multipolarity, a?(µ) a constant
  • (?0) monopole, (?1) dipole, etc
  • Oscilatations are quantized vibrational quantum
    of frequency ?? is called a phonon
  • Phonons of frequency ?? has - energy

  • - momentum

  • - parity

4
Isospin
  • Nucleons can vibrate in two ways
  • Protons and neutrons move in same direction,
    ?I0 (isoscalar)
  • Protons and neutrons move in opposing direction,
    ?I1 (isovector)

5
Vibrational modes
  • ?0 (monopole), radial vibrations
  • ?1 (dipole), no isoscalar modes (no dipole
    moment in center of mass shift)
  • ?2 (quadrupole), shape oscillations.

6
Microscopic interpretation of vibrational modes
  • Vibrations are identified with transitions
    between shell model states.
  • E.g. transition 2p3/2(N3) ?2d5/2(N4)
  • Transitions group around certain energies, Giant
    resonances

7
Photodisintegration spectrum of197Au
  • Gold atoms are bombarded with high energy gamma
    rays. Prompting the gold to emit neutrons.
  • This is the first observed giant dipole resonance

S.C. Fulz, Phys. Rev. Lett. 127, 1273 (1963)
8
Deformed nuclei I
  • Nuclei around magic numbers are spherically
    symmetric.
  • Adding neutrons to a closed shell nucleus leads
    to suppression of vibrational states.
  • Nucleus becomes less compact, leads stable
    deformations.
  • In deformed nuclei, also rotational states are
    possible.
  • Not possible in spherical symmetric nuclei,
    because of indistinguishability of the angular
    parameters.

9
Deformed nuclei II
  • For low angular momentum nuclei can have either
    an Oblate (like the earth) or a Prolate (like a
    rugby ball) shape.
  • Rotations associated with valance nucleons.
  • For high angular momentum, deformations have a
    prolate shape.
  • Rotations associated with rotation of the core
  • Angular momenta can get very high.

10
Gamma induced emission of neutrons in neodymium
  • Cross-section for gamma induced emission of
    neutrons.
  • The neodymium progresses from spherically
    symmetric to deformed.
  • First peak in 150Nd, vibrations along symmetry
    axis.
  • Second peak in 150Nd, vibrations orthongonal to
    symmetry axis.

11
How to make a rotating nucleus
  • A beam of ions is shot at a target
  • Peripheral collisions, may lead to fusion of two
    nuclei.
  • Initially the compound nucleus will emit light
    particles.
  • Finally, only gamma-ray emission is possible

12
Coupling vibrational and rotational angular
momentum
  • Coupling vibrational angular momentum K to the
    rotation R, giving total angular momentum J.
  • The z projection of J, , is a constant of
    motion.
  • Giving rotational angular momentum,
  • And rotational energy,
  • Where, I is the moment of inertia.

13
Rotational band structure
  • For given J, the K for which J(J1)-K2 is a
    minimum defines the lowest energy.
  • Lowest energy states are called the yrast states
  • For a nucleus in the groundstate, the states are
    filled in opposing Ks, k and -k ( giving total
    K0)
  • Angular momentum states Jp0,2,4,...

14
Moment of inertia
  • When viewing the moment of inertia as function of
    energy, we find 3 zones.
  • Zone 1 As ? increases, the nucleus stretches and
    I increases
  • Zone 2 Coriolis force, work opposite on K and
    K. Thus a preffered K direction is introduced.
    This will break the pairing. (backbending).
  • Zone 3 The moment of inertia assumes the rigid
    body value

E. Grosse et al.,Phys rev. Lett. 31, 840 (1973)
15
Superdeformed bands
  • Super deformed rotational band of
  • Spins of up to are observed

P.J. Twin et al.,Phys rev. Lett. 57, 811 (1986)
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