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Fundamentals of Neutron Physics
M. Scott Dewey
National Institute of Standards and Technology
11/10/2011 Radiation Metrology Workshop, Buenos
Aires, Argentina
Acknowledgements for slides
Geoff Greene, Pieter Mumm, Dan Neuman,…
Short History Lesson
Ernest Rutherford
1920 Noting that atomic number (Z) does not correspond to
atomic weight, Rutherford suggests that, in addition to
“bare” protons, the nucleus contains some tightly bound
“proton- electron pairs” or neutrons.
1930 Bothe and Becker discovered a penetrating, neutral
radiation when alpha particles hit a Be target.
1931 Mme Curie shows that they are not gamma rays and they
have sufficient momentum to eject p’s from paraffin.
?
Irene Curie
Walter Bothe
nCBe 129
1932 Chadwick replaced the paraffin with a variety of other
targets and, by measuring the recoil energies of the
ejected particles, was able to determine the mass of the
neutral particle
M = 1.15 ± ~10%
Chadwick claimed this was Rutherford’s “Neutron”
J. Chadwick, Proc. Roy. Soc., A 136 692 (1932)
1933 Bainbridge makes precision measurements of the atomic masses
of the proton and the deuteron using the mass spectrograph
1934 Chadwick and Goldhaber make the first “precision”
measurement of the neutron mass by looking at the
photo-disassociation of the deuteron
Using 2.62MeV gammas from Thorium and determining the
recoil energy of the protons they were able to determine*:
1. The neutron cannot be a bound “proton-electron pair” 2. It is energetically possible for a neutron to decay to e-+ p+
*Chadwick and Goldhaber, Nature, 134 237 (1934)
h d p n
0005.00080.1nM
KEY OBSERVATION: Mn > Mp + Me
Sources of neutrons
• Neutron generators – D + D n + 3He yields 2.5 MeV neutrons
– D + T n + 4He yields 14.1 MeV neutrons
• Radioactive sources – 252Cf, half-life 2.6 years
– Am-Be, half-life 432.2 years
Spellation Neutron Source
NIST Center for Neutron Research
H and D scatter very differently
Neutrons are very sensitive to hydrogen!
H
D O
Si
C Appropriate wavelength and energy
=> geometry of key motions
Weak neutron – nucleus interaction
=> penetrating
=> easily modeled
Why Neutrons?
Magnetic moment
Source
Thermal neutron instrumentation
Liquid hydrogen cold neutron source
Cold neutron instrumentation
Neutron guides
NIST Develops Neutron Instrumentation & Makes it Available to the Scientific Community
www.ncnr.nist.gov
The NCNR Has 25 Operating Beam Instruments Tailored to Specific Needs …
www.ncnr.nist.gov
NG6 Neutron
Physics NG7 Prompt
NG7 Interferometer
BT2 Neutron
Imaging Facil.
Thermal
Column
Diffraction
Instruments
Spectrometers
Other Neutron Methods
NG3 30 m SANS
NG7 30 m SANS
NG1 Vert. Refl.
NG1 AND/R
NG7 Hor. Refl.
BT8 Resid.
Stress Diff.
BT1
Powd.
Diff. BT5 USANS
NG0 MACS
NG2 Backscattering Spec.
NG5 Spin-Echo Spec. NG-5 SPINS
NG4 Disk Chopper
TOF Spec.
BT7 3-Axis Spec.
BT9 3-Axis Spec.
BT4 FANS
NG2 Backscattering Spec.
NG5 Spin-Echo Spec. NG-5 SPINS
NG4 Disk Chopper
TOF Spec.
NG3 30 m SANS
BT5 USANS
NG1 Depth Pofiling
Emission rate of a neutron source
Concept of the Mn bath
Role of the manganese
Time (hours)
Where do the neutrons go?
NIST Manganese Baths
The neutron exhibits much of the richness of nuclear physics, but is vastly simpler, and thus more interpretable, than nuclei.
The neutron can be used to probe Strong, Weak, EM and Gravitational phenomena as well as serving as probe for new interactions.
Neutron decay is the archetype for all nuclear beta decay and is a key process in astrophysics.
The neutron is well suited as a laboratory for tests of physics beyond the Standard Model.
Why Study Neutrons?
The Neutron is complicated enough to be interesting…
But is simple enough to be understandable.
Some Neutron Properties Mechanical Properties
Mass
Gravitational Mass (equivalence principle test)
Spin
Electromagnetic Properties
Charge (or limit on neutrality)
Internal Charge Distribution
Magnetic Dipole Moment
Electric Dipole Moment
Neutron Decay
Neutron Mean Lifetime
Correlations in Neutron Decay
“Exotic” Decay modes
Miscellaneous Quantum Numbers:
Intrinsic Parity (P), Isospin (I), Baryon Number (B), Strangeness (S), …
Neutron Decay
1930 Pauli proposes the “neutrino” to explain apparent energy
and angular momentum non-conservation in beta decay
1934 Fermi takes the neutrino idea seriously and develops his
theory of beta decay
1935 The β decay of the neutron is predicted by Chadwick and
Goldhaber based on their observation that Mn>Mp+Me .
Based on their ΔM, the neutron lifetime is estimated at ~½
hr.
1948 Snell and Miller observe neutron decay at Oak Ridge
1951 Robson makes the first “measurement” of the neutron
lifetime
Wolfgang Pauli
Enrico Fermi
Modern View of Neutron Decay:
Fermi’s View of Neutron Decay:
Neutron Lifetime (The need for a new measurement)
900
890
880
870
Neu
tro
n L
ifet
ime
(s)
2005200019951990
Year
beam UCN bottle
PDG tau = (885.7 +/- 0.8) sNew result from Serebrov et al.
Neutron lifetime dominates the theoretical uncertainty of 4He abundance.
Thermal Equilibrium (T > 1 MeV)
After Freezeout n/p decreases due to neutron decay
Nucleosynthesis (T~0.1 MeV) Light elements are formed.
almost all neutrons
present are 4He
e-
e-
Big Bang Nucleosynthesis
Measuring the Neutron Lifetime
Step 1. Get One Neutron “Bottle”
Measuring the Neutron Lifetime
Step 1. Fill Neutron “Bottle”
neutrons
Measuring the Neutron Lifetime
Step 3. Let neutron decays for time t~τn
Time
Decay R
ate
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
n
p
e
ep
pp
pn
Measuring the Neutron Lifetime
Step 4. Pour neutrons out and count
0 n
t
N t N e
Mampe et al, PRL 63 (1989) Serebrov et al, Phys Lett B605 (2005)
Magnet form
Racetrack coil
Cupronickel tube
Acrylic lightguide
TPB-coated acrylic tube
Solenoid
Neutron shielding Collimator
Beam stop
Trapping region
Huffman, et al, Nature, 403 (2000)
Some Neutron Bottles
NIST Lifetime Apparatus