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system took a photograph of analog oscilloscope traces! ... analog oscilloscope. displays.... 8. Raw data: oscilloscope photographs! ... – PowerPoint PPT presentation

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Title: isospin


1
16.451 Lecture 14 Neutron beta decay 26 Oct.
2004
1
isospin
?
2
Neutron beta decay
2
Reaction
light particles or leptons, produced in
association.
  • Neutrino or little neutral one postulated
    in 1931 by Pauli (q 0, m? 0, s ½ )
  • Only associated with the weak interaction
    very difficult to detect
  • First detected by Reines Cowan, 1959 ?
    Nobel prize 1995

3
Related processes
3
? decay in a nucleus, where energetically
favourable, eg 25Al?25Mg decay
Notice the electron and anti-neutrino appear
together the positron and neutrino appear
together.... This suggests a new conserved
quantity called lepton number, Le
4
Detection of anti-neutrinos
4
5
5
Reines Cowan Experiment (1953)
  • Very low rate experiment gt 1013 incident
    antineutrinos/sec but only 3 events/hr!
  • ? 5 months of data taking!
  • No computer data acquisition! For each event,
    an automatically-triggered camera
  • system took a photograph of analog oscilloscope
    traces!
  • Delayed coincidence detection of both neutron
    and positron suppressed background
  • Auxiliary measurements to determine detection
    efficiencies, etc.
  • Absolute cross section measured was 1 x 10-43
    cm2 (10-19 b), in agreement with theory!!

6
Schematic of the experiment
6
delayed neutrons have to slow down...
positron annihilation (instantaneous)
7
2 water tanks, sandwiched between 3 scintillation
counters to detect ?s
7
vertical height 2 m surrounded in Pb
shielding to reduce ? background...
8
No computers! electronic coincidence pulses
for e and n-capture ?s....
8
9
Raw data oscilloscope photographs!
9
scintillation light from e annihilation first,
neutron capture later ( 3 10 ?s)
10
Data coincidence event rate as a function of
time delay
10
distribution indicates slowing-down time
of neutrons in water 1/v Cd capture cross
section is large at low energy!
Bottom line first direct demonstration of the
existence of antineutrinos!
11
More on lepton number
11
There are actually three generations of leptons
that we know about (in order of increasing mass
e, ?, ? ) and each one has its own distinct
associated neutrino type with a separately
conserved lepton number....
12
12
Case study state of the art neutron lifetime
measurement
13
13
Outline of the method
decay rate
measure rate by counting decay protons in a given
time interval (dN/dt) and normalizing to the
neutron beam flux (N)
Ideally done with cold neutrons, e.g. from a
reactor, moderated in liquid hydrogen...
Issues 1. precise decay volume ? 2. proton
detection ? 3. beam normalization ? ...
14
14
Neutron beam distribution definitely not
monoenergetic
  • MeV neutrons from a reactor are moderated
    by scattering in a large tank of
  • water (thermal) or liquid hydrogen
    (cold)
  • after many scatterings, they come to thermal
    equilibrium with the moderator and
  • are extracted down a beamline to the
    experiment
  • velocity distribution is Maxwellian
    energies in the meV range (kT 26 meV _at_ 293K)

Krane, Fig 12.4
15
Neutron detection at low energy
15
  • several light nuclei have enormous neutron
    capture cross sections at low energy
  • (recall, cross sectional area of a
    nucleus, e.g. 10B is about 0.2 barns, lecture 4)
  • key feature cross sections scale as
    1/velocity at low energy

16
Put this together for detector counting rates as
shown
16
neutrons must be captured to be detected!
17
Experimental details (all in vacuum, at ILL
reactor, France)
17
  • use Penning trap to confine decay protons
  • let them out of the trap after accumulation
    interval T
  • measure the ratio Ndet/Ndecay as a function of
    trap length L ? slope gives ?

18
Amazing results
18
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