r. machleidtnuclear forces - lecture 1 history, facts, phen. (cnsss13) 1 nuclear forces - lecture 1...

R. Machleidt Nuclear Forces - Lecture 1 History, Facts, Phen. (CNSSS13)

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Nuclear Forces- Lecture 1 -

R. MachleidtUniversity of Idaho

History, Facts and Phenomenology

12th CNS International Summer School (CNSSS13)28 August to 03 September 2013 -- CNS Wako Campus

R. Machleidt Nuclear Forces - Lecture 1 History, Facts, Phen. (CNSSS13)

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Nuclear Forces- Overview of all lectures -

• Lecture 1: History, facts, and phenomenology

• Lecture 2: The meson theory of nuclear forces

• Lecture 3: QCD and nuclear forces; effective field theory (EFT) for low-energy QCD

• Lecture 4: Nuclear forces from chiral EFT

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Lecture 1: History, Facts, and Phenomenology

Historical review

Properties of the nuclear force

Phenomenological descriptions

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History of Nuclear Forces: Phase I

1930’sChadwick (1932): Neutron

Heisenberg (1932): First Phenomenology (Isospin)

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Heisenberg and his contribution of 1932

Heisenberg

Niels Bohr

Pauli

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Zeitschrift fuer Physik 77, 1

(1932)

On the Structure of Atomic Nuclei. I.

….

… Chadwick …

… suggests the assumption that atomic nuclei are built from protons and neutrons without electrons …

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Zeitschrift fuer Physik 77, 1 (1932), cont’d

Precursor of the idea of Boson Exchange!

… the force … between proton and neutron …

….. in analogy to the H2+-ion --- an exchange of negative charge will take place, …

This exchange can be visualized by electrons which do not have spin and follow the rules of bose statistics …

2H

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History, Phase I cont’d

1930’sChadwick (1932): Neutron

Heisenberg (1932): First Phenomenology (Isospin)

Yukawa (1935): Meson Hypothesis

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Yukawa and his idea

S. Tomonaga, H. Yukawa, and S. Sakata in the 1950s.

TomonagaYukawa

Sakata

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From:

H. Yukawa, Proc. Phys. Math. Soc. Japan 17, 48 (1935).

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History, Phase I cont’d

1930’sChadwick (1932): Neutron

Heisenberg (1932): First Phenomenology (Isospin)

Yukawa (1935): Meson Hypothesis

1950’sTaketani, Nakamura, Sasaki (1951): 3 ranges.

One-Pion-Exchange (OPE): o.k.

Multi-pion exchanges: Problems!

Taketani, Machida, Onuma (1952);

Brueckner, Watson (1953).

Quotes by Bethe (1953) and Goldberger (1960)

“Pion Theories”

Discovery of the pion in cosmic ray (1947) and in theBerkeley Cyclotron Lab (1948).Nobelprize awarded to Yukawa (1949). 1940’s

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Scientific American, September 1953

What Holds

the Nucleus Together?

by Hans A. Bethe

In the past quarter century physicists have devoted a huge amount of experimentation and mental labor to this problem – probably more man-hours than have been given to any other scientific question in the history of mankind.

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“There are few problems in nuclear theoretical physics which have attracted more attention than that of trying to determine the fundamental interaction between two nucleons. It is also true that scarcely ever has the world of physics owed so little to so many …… It is hard to believe that many of the authors are talking about the same problem or, in fact, that they know what the problem is.” M. L. Goldberger

Midwestern Conference on Theoretical Physics, Purdue University, 1960

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History, Phase I (The first pion period)

1930’sChadwick (1932): Neutron

Heisenberg (1932): First Phenomenology (Isospin)

Yukawa (1935): Meson Hypothesis

1950’sTaketani, Nakamura, Sasaki (1951): 3 ranges.

One-Pion-Exchange (OPE): o.k.

Multi-pion exchanges: Problems!

Taketani, Machida, Onuma (1952);

Brueckner, Watson (1953).

Quotes by Bethe (1953) and Goldberger (1960)

“Pion Theories”

Discovery of the pion in cosmic ray (1947) and in theBerkeley Cyclotron Lab (1948).Nobelprize awarded to Yukawa (1949). 1940’s

The first pion period:

results in a disaster

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Phase II: The meson period

1960’sMany pions = multi-pion resonances:

One-Boson-Exchange Model

...)782(),770(),600(

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Phase II: The meson period

1960’sMany pions = multi-pion resonances:

One-Boson-Exchange Model

...)782(),770(),600(

...

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Phase II: The meson period

1960’sMany pions = multi-pion resonances:

One-Boson-Exchange Model

1970’sRefined Meson Theories

Sophisticated models for two-pion exchange:

Paris Potential (Lacombe et al., PRC 21, 861 (1980))

Bonn potential (Machleidt et al., Phys. Rep. 149, 1 (1987))

...)782(),770(),600(

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The exponential tail of phase II(or the epigone period of meson theory)(or the epigone period of meson theory)

1980’s Nijmegen: We need more precision!!!“A χ²/dat of ≈ 2 is not good enough, it has to be 1.0”

1990’s1993: The high-precision Nijmegen phase shift analysis

1994-2001: High-precision NN potentials:

Nijmegen I, II, ’93, Reid93 (Stoks et al. 1994)

Argonne V18 (Wiringa et al, 1995)

CD-Bonn (Machleidt et al. 1996, 2001)

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Gell-MannZweig

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1960’sMany pions = multi-pion resonances:

One-Boson-Exchange Model

...)782(),770(),600( Gell-Mann and Zweig (1963):

3 quarks!

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1980’s Nuclear physicists discover QCD:

Quark cluster models.

1990 –

today

Nuclear physicists discover Effective Field Theory (EFT):

Weinberg (1990); Ordonez, Ray, van Kolck (1994/96).

Another “pion theory”; but now right: constrained by chiral symmetry

Phase III: The QCD/EFT period

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1980’s Nijmegen: We need more precision!!!

1990’s1993: The high-precision Nijmegen phase shift analysis

1994-2001: High-precision NN potentials:

Nijmegen I, II, ’93, Reid93;

Argonne V18;

CD-Bonn.

1980’s Nuclear physicists discover QCD:

Quark cluster models.

1990 -today

Nuclear physicists discover Effective Field Theory (EFT):

Weinberg (1990); Ordonez, Ray, van Kolck (1994/96).

Another “pion theory”; but now right: constrained by chiral symmetry

Phase III: The QCD/EFT period

The second pion period:

No disaster!

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Properties of the nuclear force

• Finite range• Intermediate-range attraction• Short-range repulsion (“hard core”)• Spin-dependent non-central forces:

- Tensor force

- Spin-orbit force• Charge independence

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Finite range

• Comparison of the binding energies of

show that the nuclear force is of finite range (1-2 fm) and very strong within that range (Wigner, 1933).

• “Saturation”. Nuclei with A>4 show saturation: Volume and binding energies of nuclei are proportional to the mass number A.

particle)-(alpha He(triton),H deuteron),(H 432

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Intermediate-range attraction

Nuclei are bound. The average distance between nucleons in nuclei is about 2 fm which must roughly correspond to the range of the attractive force.

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Short-range repulsion (“hard core”)

Analyze 1S0 phase shifts and compare to 1D2 phase shifts.

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Non-central forces

Tensor Force: First evidence from the deuteron

Deuteron

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Tensor force, cont’d

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Tensor force, cont’d

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Non-central forces

Spin-Orbit Force

Nucleus or proton

rightleft

Proton 1

Proton 2

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Summary:Most important parts of the nuclear force

ShortInter-mediate Long range

Tensor force

Spin-orbit force

Central force

Taketani, Nakamura, Sasaki (1951): 3 ranges

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Charge-independence

• After correcting for the electromagnetic interaction, the forces between nucleons (pp, nn, or np) in the same state are almost the same.

• “Almost the same”: Charge-independence is slightly broken.• Notation: Equality between the pp and nn forces: Charge symmetry. Equality between pp/nn force and np force: Charge independence.• Better notation: Isospin symmetry; invariance under rotations in isospin space.

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Since the scattering length is a magnifying glass on the interaction, charge-independence breaking (CIB) is seen most clearly in the different scattering lengths of pp, nn, and np low-energy scattering.

Charge-symmetry breaking (CSB) - after electromagnetic effects have been removed:

Charge-independence breaking: Evidence

fm 02.074.23 npa

Charge-independence breaking (CIB):

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Phenomenological descriptions

• Symmetries and the general expression for the NN potential

• Historically important examples of phenomenological NN potentials

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The symmetries

• Translation invariance• Galilean invariance• Rotation invariance• Space reflection invariance• Time reversal invariance• Invariance under the interchange of particle 1 and 2• Isospin symmetry• Hermiticity

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Most general two-body potential under those symmetries (Okubo and Marshak, Ann. Phys. 4, 166 (1958))

with

NNV central

tensorquadratic spin-orbit

spin-orbit

another tensor

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Potentials which are based upon the operator structure shown on the previous slide (but may not include all operators shown or may include

additional operators) are called “Phenomenological Potentials”.Some historically important examples are given below.

• Gammel-Thaler potential ( Phys. Rev. 107, 291, 1339 (1957)), hard-core.

• Hamada-Johnston potential (Nucl. Phys. 34, 382 (1962)), hard core.

• Reid potential (Ann. Phys. (N.Y.) 50, 411 (1968)), soft core.• Argonne V14 potential (Wiringa et al., Phys. Rev. C 29, 1207

(1984)), uses 14 operators.• Argonne V18 potential (Wiringa et al., Phys. Rev. C 51, 38

(1995)), uses 18 operators.

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End Lecture 1