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What is a Neutrino?
       Bradley J. Wogsland
      University of Tennessee




                                    What am I?

                                ν
Quantum Weirdness

                        λ = h/p
●   Quanta are not particles
    –   But can be approximated as such in limit of large momenta
●   Quanta are not waves
    –   But can be approximated as such in limit of low momenta
Examples
●   Monsieur de Broglie
    –   riding his bicycle at about 25 mph would have a
        wavelength λ ≈ 10-37m (and about 1030 eV/c momentum)
●   Photons
    –   visible light at λ ≈ 500nm has about 2.5 eV/c per photon
●   Neutrinos...
Wolfgang Pauli

                                     ●   Made up neutrino to
                                         conserve lepton
                                         number
                                     ●   n → p+ + e- + νe
                                     ●   Had already worked
                                         for Dirac vis a vis the
                                         positron
Pauli & Bohr at the top of physics
The Standard Model
●   Tabulation of the
    results of “particle”
    physics
●   Like the periodic table
    in Chemistry
●   A good guide, but
    starting to get a little
    too stretched at the
    seams...
The Weak Interaction
●   Allows quarks & leptons to change flavor
●   For example, neutron decay can be written
                                  -
              d(ud) → u(ud) + e + νe
●   (quarks not involved in the decay but still bound
    in the baryon are in parentheses)
●   Similar c to s and t to b reactions also occur
Massive Particles
●   Must travel at subluminal velocities
●   How fast they travel through the vacuum at a
    given energy depends on the mass

                             -iEt
               |ψ(t)> = e |ψ(0)>
                           E= p m
                               2      2
                    with
Bruno Pontecorvo
      ●   Born in 1913 (Pisa, Italy)
      ●   Worked under Fermi
      ●   Fled Italian fascism to North
          America in the mid-1930's
      ●   Proposed inverse β-decay detection
          of neutrinos in 1946 via
          37
      ●        Cl + νe → 37Ar + e-
      ●   Fled to the USSR after arrest of
          Klaus Fuchs in 1950
      ●   Predicted neutrino oscillations in
          1957
      ●   Dies in 1993 (Dubna, Russia)
Pontecorvo's Idea
●   The mass eigenstates of neutrinos don't
    correspond to the flavor eigenstates.
●   This is expressed by the PMNS matrix:

          [v1] [3/4 -1/8 1/8 ] [v e]
          [v2] ≈ [1/4 3/8 -3/8 ] [v μ]
          [v3] [ 0 1/2 1/2 ] [v τ]
               (All terms are squareroots)
Geometrically




θ12 ≈ π/6   θ23 ≈ π/4   θ13 ≈ 0 (< .2)
Quarks do it,too
●   This is expressed by the CKM matrix:

          [d] [.97 .22 .0037] [d m]
          [s] ≈ [.22 .97 .04 ] [s m]
          [b] [ 0 .04 .99 ] [b m]
        (Here the weak eigenstates are on the left)

●   Note that there is almost no mixing in this case
Mass Differences
●   So far, only the differences between the mass
    eigenstates can be measured
●   |∆m12| ≈ 9 meV
●   |∆m32| ≈ 50 meV
●   Overall upper bound ~200meV
Neutrino Mass Hierarchies


        2
       m3                                              2
                                                     m2
                                                     m12    m21
                                                              2


m32
  2

                                                           m32
                                                             2


        2
       m2
m2
  21                     (0.00 eV )22
                         (0.20
                         (0.10
                         (0.23                        2
       m12                                           m3

              “Verted”                  “Inverted”
So what is a neutrino?

A massive neutral lepton that interacts weakly. To
 calculate its propagation, use the mass basis. To
calculate its probability of interacting weakly, use
                  the flavor basis.

                         What am I?
                          Really?

                    ν
An Analogy
●   An electron is a spin-½ particle
●   We can measure this spin either up or down
●   Nevertheless, an electron can be in a state where
    it has a certain probability to be up and a certain
    probability to be down
●   Generally, we don't think of spin up and spin
    down electrons as two different particles, but as
    electrons with different spin orientations
Don't be surprised when neutrino oscillations
        become a textbook example of a macroscopic
                        quantum effect.




Recommended reading: Neutrino Oscillations for Dummies
A Few BIG Questions Remain
●   What are the actual neutrino mass eigenstates?
    –  Currently we can only measure the
       differences.
●   Is the neutrino its own antiparticle?
    –  Majorana or Dirac question
●   Is there a deeper reason for so much mixing,
    unlike the quark case?
●   How did this craft of junk cross the Atlantic?

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Neutrinos

  • 1. What is a Neutrino? Bradley J. Wogsland University of Tennessee What am I? ν
  • 2. Quantum Weirdness λ = h/p ● Quanta are not particles – But can be approximated as such in limit of large momenta ● Quanta are not waves – But can be approximated as such in limit of low momenta
  • 3. Examples ● Monsieur de Broglie – riding his bicycle at about 25 mph would have a wavelength λ ≈ 10-37m (and about 1030 eV/c momentum) ● Photons – visible light at λ ≈ 500nm has about 2.5 eV/c per photon ● Neutrinos...
  • 4. Wolfgang Pauli ● Made up neutrino to conserve lepton number ● n → p+ + e- + νe ● Had already worked for Dirac vis a vis the positron Pauli & Bohr at the top of physics
  • 5. The Standard Model ● Tabulation of the results of “particle” physics ● Like the periodic table in Chemistry ● A good guide, but starting to get a little too stretched at the seams...
  • 6. The Weak Interaction ● Allows quarks & leptons to change flavor ● For example, neutron decay can be written - d(ud) → u(ud) + e + νe ● (quarks not involved in the decay but still bound in the baryon are in parentheses) ● Similar c to s and t to b reactions also occur
  • 7. Massive Particles ● Must travel at subluminal velocities ● How fast they travel through the vacuum at a given energy depends on the mass -iEt |ψ(t)> = e |ψ(0)> E= p m 2 2 with
  • 8. Bruno Pontecorvo ● Born in 1913 (Pisa, Italy) ● Worked under Fermi ● Fled Italian fascism to North America in the mid-1930's ● Proposed inverse β-decay detection of neutrinos in 1946 via 37 ● Cl + νe → 37Ar + e- ● Fled to the USSR after arrest of Klaus Fuchs in 1950 ● Predicted neutrino oscillations in 1957 ● Dies in 1993 (Dubna, Russia)
  • 9. Pontecorvo's Idea ● The mass eigenstates of neutrinos don't correspond to the flavor eigenstates. ● This is expressed by the PMNS matrix: [v1] [3/4 -1/8 1/8 ] [v e] [v2] ≈ [1/4 3/8 -3/8 ] [v μ] [v3] [ 0 1/2 1/2 ] [v τ] (All terms are squareroots)
  • 10. Geometrically θ12 ≈ π/6 θ23 ≈ π/4 θ13 ≈ 0 (< .2)
  • 11. Quarks do it,too ● This is expressed by the CKM matrix: [d] [.97 .22 .0037] [d m] [s] ≈ [.22 .97 .04 ] [s m] [b] [ 0 .04 .99 ] [b m] (Here the weak eigenstates are on the left) ● Note that there is almost no mixing in this case
  • 12. Mass Differences ● So far, only the differences between the mass eigenstates can be measured ● |∆m12| ≈ 9 meV ● |∆m32| ≈ 50 meV ● Overall upper bound ~200meV
  • 13. Neutrino Mass Hierarchies 2 m3 2 m2 m12 m21 2 m32 2 m32 2 2 m2 m2 21 (0.00 eV )22 (0.20 (0.10 (0.23 2 m12 m3 “Verted” “Inverted”
  • 14. So what is a neutrino? A massive neutral lepton that interacts weakly. To calculate its propagation, use the mass basis. To calculate its probability of interacting weakly, use the flavor basis. What am I? Really? ν
  • 15. An Analogy ● An electron is a spin-½ particle ● We can measure this spin either up or down ● Nevertheless, an electron can be in a state where it has a certain probability to be up and a certain probability to be down ● Generally, we don't think of spin up and spin down electrons as two different particles, but as electrons with different spin orientations
  • 16. Don't be surprised when neutrino oscillations become a textbook example of a macroscopic quantum effect. Recommended reading: Neutrino Oscillations for Dummies
  • 17. A Few BIG Questions Remain ● What are the actual neutrino mass eigenstates? – Currently we can only measure the differences. ● Is the neutrino its own antiparticle? – Majorana or Dirac question ● Is there a deeper reason for so much mixing, unlike the quark case? ● How did this craft of junk cross the Atlantic?