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Stars as Laboratories for Fundamental Physics - MPP Theory Group

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308 Chapter 8<br />

system (ν L e , ν L µ , ν R e , ν R µ ) and (ν L e , ν L µ, ν R e , ν R µ ). Moreover, one may have<br />

both diagonal and transition magnetic moments so that <strong>for</strong> neutrinos<br />

the r.h.s. of the equation of motion is<br />

⎛<br />

⎞ ⎛<br />

∆ m c 2θ + V νe ∆ m s 2θ µ ee B T µ µe B T ν L ⎞<br />

e<br />

∆ m s 2θ −∆ m c 2θ + V νµ µ eµ B T µ µµ B T<br />

ν L µ<br />

⎜<br />

⎟ ⎜<br />

⎝ µ ee B T µ µe B T ∆ m c 2θ ∆ m s 2θ ⎠ ⎝ ν R ⎟<br />

e ⎠ , (8.59)<br />

µ eµ B T µ µµ B T ∆ m s 2θ −∆ m c 2θ νµ<br />

R<br />

where the right-handed neutrinos do not experience a medium-induced<br />

energy shift.<br />

For certain values of the parameters the oscillations between two<br />

states may dominate which are then described by a certain 2 × 2 submatrix.<br />

Then the general treatment is much like the flavor mixing<br />

problems studied earlier. In general, a much richer collection of solutions<br />

obtains—<strong>for</strong> a review see Pulido (1992).<br />

Electric transition moments can also play a role, and precessions<br />

in electric fields may be important. Majorana neutrinos have either<br />

electric or magnetic transition moments, but not both <strong>as</strong> long <strong>as</strong> CP<br />

remains conserved. Still, even electric transition moments would lead<br />

to spin-flavor oscillations in macroscopic magnetic fields.<br />

8.4.4 Twisting Magnetic Fields<br />

The problem of spin oscillations is further complicated by the possibility<br />

that the magnetic field changes its direction along the neutrino trajectory,<br />

i.e. that it may be “twisting” (Aneziris and Schechter 1991). In<br />

this c<strong>as</strong>e the equation of motion of a two-level spin-precession problem<br />

is b<strong>as</strong>ed on the Hamiltonian<br />

( BL B<br />

H = µ<br />

T e −iφ )<br />

B T e iφ , (8.60)<br />

−B L<br />

where the three parameters B L , B T , and φ vary along the neutrino<br />

trajectory. The transverse field strength B T is a physical magnetic<br />

field while the longitudinal one B L is an effective magnetic field which<br />

represents the neutrino m<strong>as</strong>s difference (spin-flavor oscillations!) and<br />

refractive medium effects. As long <strong>as</strong> B T maintains its direction along<br />

the trajectory, the ph<strong>as</strong>e φ can be globally chosen to be zero.<br />

If φ varies along the trajectory so that the neutrino experiences it to<br />

be a function of time, it is useful to trans<strong>for</strong>m the equation of motion to<br />

a coordinate system which corotates with B T so that in the new frame<br />

one is back to the old situation of a fixed direction <strong>for</strong> B T (Smirnov

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