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The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo
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The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Jan 17, 2018

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Lester Evans

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Page 1: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

The 3 MeV pygmy resonance in 163,164Dy

Hilde-Therese Nyhus

Department of Physics University of Oslo

Page 2: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Introduction Motivation for analyzing these nuclei Experimental method Level density Gamma-ray strength function

Page 3: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Motivation

Page 4: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

MotivationVarious other rare earth nucleihave been studied using theOslo method, one has then measured a width of the pygmyresonance between 1.2-1.5 MeV. This contradicts what has been measured in Prague for other rare earth nuclei, where abouthalf the width has been found.

Page 5: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

The reactions used to produce the nuclei

Page 6: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

The reactions used to produce the nuclei

At Oslo Cyclotron Laboratory:

164Dy(3He, 3He*)164Dy164Dy(3He, )163Dy

Page 7: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

The reactions used to produce the nuclei

At Oslo Cyclotron Laboratory:

164Dy(3He, 3He*)164Dy164Dy(3He, )163Dy

In Prague:162Dy(n, )163Dy

Page 8: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Experimental method-Gate on the various particles to construct coincidence matrix.

Page 9: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Coincidence matrixes

163Dy 164Dy

Page 10: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Experimental method-Gate on the various particles to construct coincidence matrix.

-Unfold the gamma spectrum and generate first generation matrix.

Page 11: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

First generation matrixes

163Dy 164Dy

Page 12: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Experimental method-Gate on the various particles to construct coincidence matrix.-Unfold the gamma spectrum and generate first generation matrix.

-The experimentally obtained first generation matrix is according to the Brink-Axel hypothesis proportional to the level density and gamma ray strength function.

P(E x,Eγ )∝T(Eγ )ρ(E x,Eγ )

Page 13: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Level density in 163,164Dy

Preliminary

163Dy 164Dy

Page 14: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Gamma-ray strength function with pygmy resonance

Gamma-ray strength function in 164Dy, with a pygmy resonance.

Gamma-ray strength function in 163Dy, with a pygmy resonance.

The width of the pygmy resconance masured in Prague is 0.6 MeV

163Dy 164Dy

Preliminary

Page 15: The 3 MeV pygmy resonance in 163,164 Dy Hilde-Therese Nyhus Department of Physics University of Oslo.

Gamma-ray strength function with pygmy resonance

Gamma-ray strength function in 163Dy, with a pygmy resonance.

The width of the pygmy resconance masured in Prague is 0.6 MeV

163Dy

Preliminary