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Collective oscillations of SN neutrinos :: A three-flavor course ::

Collective oscillations of SN neutrinos :: A three-flavor course ::. Amol Dighe Tata Institute of Fundamental Research, Mumbai. Melbourne Neutrino Theory Workshop, 2-4 June 2008. Collective effects in a nutshell.

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Collective oscillations of SN neutrinos :: A three-flavor course ::

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  1. Collective oscillations of SN neutrinos:: A three-flavor course :: Amol Dighe Tata Institute of Fundamental Research, Mumbai Melbourne Neutrino Theory Workshop, 2-4 June 2008

  2. Collective effects in a nutshell • Large neutrino density near the neutrinosphere gives rise to substantial neutrino-neutrino potential • Nonlinear equations of motion, give rise to qualitatively and quantitatively new neutrino flavor conversion phenomena • Effects observed numerically in SN numerical simulations since 2006 (Duan, Fuller, Carlson, Qian) • Analytical understanding in progress (Pastor, Raffelt, Semikoz, Hannestad, Sigl, Wong, Smirnov, Abazajian, Beacom, Bell, Esteban-Pretel, Tomas, Fogli, Lisi, Marrone, Mirizzi, Dasgupta, Dighe et al.) • Substantial impact on the prediction of SN neutrino flavor convensions

  3. Equations of motion including collective potential Density matrix : Eqn. of Motion : Hamiltonian : Useful convention: Antineutrinos : mass-matrix flips sign , as if p is negative (Sigl, Raffelt: NPB 406: 423, 1993; Raffelt, Smirnov: hep-ph/0705.1830) Useful approximation: Neglect three-angle effects: single-angle approximation (reasonably valid: Fogli et al.) Pantaleone’s - interaction MSW potential Mass matrix

  4. Collective neutrino oscillation: two flavors In dense neutrino gases… 1 1 Synchronized oscillation :Neutrinos with all energies oscillate at the same frequency Pee Pee 0 0 L L Bipolar oscillation : Neutrinos and antineutrinos with all energies convert pairwise; flipping periodically to the other flavor state Spectral split : Energy spectrum of two flavors gets exchanged above a critical energy f E E

  5. 2- flavors : Formalism Expand all matrices in terms of Pauli matricesas The following vectors result from the matrices EOM resembles spin precession

  6. The spinning top analogy • Motion of the average P defined by • Construct the “Pendulum’’ vector • EOMs are given by • Mapping to Top : • EOMs now become • Note that these areequations of a spinning top!!!(Hannestad, Raffelt, Sigl, Wong: astro-ph/0608695; Fogli, Lisi, Mirizzi, Marrone: hep-ph/0707.1998)

  7. B z  P x Synchronized oscillation • Spin is very large : Top precesses about direction of gravity • At large  » avg :Q precesses about B with frequencyavg • Therefore S precesses about B with frequency avg • Large : all P are bound together: same EOM • Survival probability : • (Pastor, Raffelt, Semikoz: hep-ph/0109035) Precession = Sinusoidal Oscillation

  8. B z  P x Bipolar oscillation • Spin is not very large : Top precesses and nutates • At large  ≥ avg :Q precesses + nutates about B • Therefore S does the same • All P are still bound together, same EOM: • Survival probability : • (Hannestad, Raffelt, Sigl, Wong: astro-ph/0608695; Duan, Fuller, Carlson, Qian: astro-ph/0703776) Nutation = Inverse elliptic functions

  9. z P x  B Adiabatic spectral split • Top falls down when it slows down (when mass increases) • If  decreases slowly P keeps up with H • As →0 from its large value :Paligns with hB • For inverted hierarchy P has to flip, BUT… • B.D is conserved so all Pcan’t flip • Low energy modes anti-align • All P with  < c flip over • Spectral Split • (Raffelt, Smirnov:hep-ph/0705.1830)

  10. 3- flavors : Formalism • Expand all matrices in terms of Gell-Mann matrices as • The following vectors result from the matrices • EOM formally resembles spin precession

  11. Motion of the polarization vector P • P moves in eight-dimensional space, inside the “Bloch sphere” (All the volume inside a 8-dim sphere is not accessible) • Flavor content is given by diagonal elements: e3 and e8 components (allowed projection: interior of a triangle)

  12. Some observations about 3- case • When ε = ∆m212 /∆m312 is taken to zero, the problem must reduce to a 2- flavor problem • That problem is solved easily by choosing a useful basis • When we have 3- flavors • Each term by itself reduces to a 2- flavor problem • Hierarchical ``precession frequencies’’, so factorization possible • Enough to look at the e3 and e8 components of P

  13. e8 nx ne e3 P ny The e3 - e8 triangle

  14. ne nx e3ey e8ey Vacuum/Matter/Synchronized Oscillations Bipolar Spectral Split P ny The 2-n flavorslimit Mass matrix gives only Evolution function looks like So that,

  15. nx ne • Each sub-system has widely • different frequency • Interpret motion as a product of successive precessions in different subspaces of SU(3) • To first order, P Atmospheric Solar ny (Opposite order for bipolar) 3-n flavors and factorization Neutrinos trace something like Lissajous figures in the e3-e8 triangle

  16. nx ne P ny Synchronized oscillations All energies have same trajectory, but different speeds

  17. nx ne P ny Bipolar oscillations Petal-shaped trajectories due to bipolar oscillations

  18. nx ne P ny Spectral splits Two lepton number conservation laws : B.Dconserved (Duan, Fuller, Qian: hep-ph/0801.1363; Dasgupta, Dighe, Mirizzi, Raffelt hep-ph/0801.1660)

  19. A typical SN scenario Order of events : (1) Synchronization (2) Bipolar (3) Split Collective effects (4) MSW resonances (5) Shock wave Traditional effects (6) Earth matter effects

  20. Before Split Swap After Spectral splits in SN spectra Neutrinos Antineutrinos

  21. Survival probabilities after collective+MSW • Spectral split in neutrinos for inverted hierarchy • All four scenarios are in principle distinguishable

  22. Presence / absence of shock effects Condition for shock effects: Neutrinos: p should be different for A and C Antineutrinos: pbar should be different for B and D

  23. Presence / absence of Earth matter effects Conditions for Earth matter effects: Neutrinos: p should be nonzero Antineutrinos: pbar should be nonzero

  24. State of the Collective For “standard” SN, flavor conversion can be predicted more-or-less robustly (Talks of Basudeb Dasgupta, Andreu Esteban-Pretel, Sergio Pastor) Some open issues still to be clarified are: • How multi-angle decoherence is prevented • Behaviour at extremely small 13values • Possible nonadiabaticity in spectral splits • Possible interference between MSW resonances and bipolar oscillations Collective efforts are in progress !

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