neutrino lines from majoron dark matter
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Neutrino Lines from Majoron Dark Matter Julian Heeck based on: JH, Camilo Garcia-Cely, JHEP 1705 (2017) 102 [1701.07209]. NUFACT2017 28.9.2017 Is it possible to detect dark matter via neutrinos and not gamma-rays or anti-matter? Neutrinos


  1. Neutrino Lines from Majoron Dark Matter Julian Heeck based on: JH, Camilo Garcia-Cely, JHEP 1705 (2017) 102 [1701.07209]. NUFACT2017 28.9.2017

  2. Is it possible to detect dark matter via neutrinos and not gamma-rays or anti-matter?

  3. Neutrinos have masses and mix ● Mass splittings ✔ ● Angles ✔ ● Phase(s) ✘ ● Ordering ✘ ● Mass scale ✘ ● Dirac vs. Majorana ✘ ● Mass origin ✘ Julian Heeck (ULB) - Majorons 3

  4. Majoronic seesaw ● 3 singlets N R + new scalar B-L breaking scale Heavy scalar Majoron (inflaton?) [Chikashige, Mohapatra, Peccei, ‘81; Schechter, Valle, ‘82] ● Break U(1) B-L spontaneously: ● For Julian Heeck (ULB) - Majorons 4

  5. Parametrization of our ignorance “Known”: PMNS mixing matrix ● Leaves 9 unknown parameters. ● Here: hermitian [Davidson, Ibarra, hep-ph/0104076] ● One-to-one: ● Useful: majoron loop couplings depend on Julian Heeck (ULB) - Majorons 5

  6. Tree-level couplings ● Tiny coupling: neutrino mass over B-L breaking scale! ● Long lifetime → majoron dark matter! [Berezinsky, Valle ‘93; Lattanzi, Valle ‘07; Queiroz, Sinha, ‘14] ● DM abundance e.g. via freeze-in. [ McDonald, ‘02; Hall, Jedamzik, March-Russell, West ‘10; Frigerio, Hambye, Masso, ‘11 ] Julian Heeck (ULB) - Majorons 6

  7. Flavor of J → ν k ν k Mass eigenstates → no oscillations! Flavor ratios: [JH, Camilo Garcia-Cely, 1701.07209] Julian Heeck (ULB) - Majorons 7

  8. Indirect detection ● General limit from DM → invisible: [Audren, Lesgourgues, Mangano, Serpico, Tram, ‘14] ● Can we observe the neutrino lines ? – m J > 10 TeV: No. Dominant decay is J →ννh(h). ► no line! [Dudas, Mambrini, Olive, ‘15] – Also want to avoid electroweak Bremsstrahlung. [Kachelriess, Serpico, ‘07; Bell, Dent, Jacques, Weiler, ‘08; Queiroz, Yaguna, Weniger, ‘16] – For MeV < m J < 100 GeV: Yes! Julian Heeck (ULB) - Majorons 8

  9. Lower limit on breaking scale f (GeV) m J (GeV) = 2 E ν Julian Heeck (ULB) - Majorons 9 [JH, Camilo Garcia-Cely, 1701.07209]

  10. [JH, Camilo Garcia-Cely, 1701.07209] Lower limit on breaking scale f (GeV) Threshold for ν e p → n e + . m J (GeV) = 2 E ν Julian Heeck (ULB) - Majorons 10

  11. [JH, Camilo Garcia-Cely, 1701.07209] Lower limit on breaking scale f (GeV) Reinterpreted Super-K data. [Palomares-Ruiz, 0712.1937] Threshold for ν e p → n e + . m J (GeV) = 2 E ν Julian Heeck (ULB) - Majorons 11

  12. Lower limit on breaking scale f (GeV) m J (GeV) = 2 E ν Julian Heeck (ULB) - Majorons 12 [JH, Camilo Garcia-Cely, 1701.07209]

  13. Look for neutrinos from light DM! ● ν lines detectable down to MeV. ● For free in searches for diffuse supernova neutrino background. ● Borexino = indirect DM detector. ● Future direct DM detectors (LZ, ν XENONnT) = indirect DM detectors. ● Also Hyper-K, JUNO,... ● DM → ν easily dominant channel, no SU(2) argument as for multi-TeV DM. [El Aisati, Garcia-Cely, Hambye, Vanderheyden, 1706.06600] Julian Heeck (ULB) - Majorons 13

  14. One-loop couplings ● Diagonal: ● Off-diagonal: ● K = rest of seesaw! ● ● New parameter: ● One generation: [Chikashige, Mohapatra, Peccei, ‘81; Pilaftsis ‘94] Julian Heeck (ULB) - Majorons 14

  15. Indirect detection II ● DM → ττ, bb, tt, … give – continuous γ spectrum: Integral, Fermi-LAT. – anti-protons and positrons: e,p,γ PAMELA, AMS-02. ● DM decay around z ~ 1000: – modification of CMB. [Slatyer, Wu, 1610.06933] – independent of DM profile. Julian Heeck (ULB) - Majorons 15

  16. Indirect detection II [Slatyer, Wu, 1610.06933] ● DM → ττ, bb, tt, … give – continuous γ spectrum: Integral, Fermi-LAT. – anti-protons and positrons: e,p,γ PAMELA, AMS-02. ● DM decay around z ~ 1000: – modification of CMB. [Slatyer, Wu, 1610.06933] – independent of DM profile. Julian Heeck (ULB) - Majorons 16

  17. [JH, Camilo Garcia-Cely, 1701.07209] m J (GeV) Julian Heeck (ULB) - Majorons 17

  18. [JH, Camilo Garcia-Cely, 1701.07209] Strong CMB limits. [Slatyer, Wu, 1610.06933] m J (GeV) Julian Heeck (ULB) - Majorons 18

  19. [JH, Camilo Garcia-Cely, 1701.07209] Strong CMB limits. [Slatyer, Wu, 1610.06933] m J (GeV) Requires J→ hadrons. Julian Heeck (ULB) - Majorons 19

  20. Two-loop couplings [JH, Camilo Garcia-Cely, 1701.07209] ● Full calculation highly non-trivial. [ JH, Hiren Patel, in progress ] ● J-Z mixing formally similar to triplet majoron: [Bazzocchi, Lattanzi, Riemer-Sørensen, Valle, 0805.2372] (two loop) (one loop) ● Gives the only DM signature for m J < MeV. [Lattanzi, Riemer-Sørensen, Tórtola, Valle, ‘13; Queiroz, Sinha, ‘14] Julian Heeck (ULB) - Majorons 20

  21. Gamma line plot m J (GeV) m J (GeV) Julian Heeck (ULB) - Majorons 21

  22. Gamma line plot “MeV gap”, γ limits will improve a lot with e-ASTROGAM, AdEPT. m J (GeV) m J (GeV) Julian Heeck (ULB) - Majorons 22

  23. Is it possible to detect dark matter via neutrinos and not gamma-rays or anti-matter? Yes! depends on depends on Independent / Complementary! Julian Heeck (ULB) - Majorons 23

  24. Summary ● Majoron couplings suppressed by U(1) L scale. ● Automatically long-lived DM candidate. ● Seesaw and leptogenesis for free. ● For MeV < m J : J→νν in Borexino, Super-K,… ● Complementary to J→γγ, ℓℓ’, qq. Always look out for lines! Julian Heeck (ULB) - Majorons 24

  25. Backup

  26. Majoron = DM ● Naturally light, long-lived DM candidate. ● Indirect detection possible: – MeV < m J : J → νν, γγ, ff. – keV < m J < MeV: J →γγ. Maybe warm DM. [JH, Daniele Teresi, 1706.09909, 1709.07283] Majoron ≠ DM ● Increase couplings to produce J in lab. ● Measure seesaw parameters. [JH, work in progress] Julian Heeck (ULB) - Majorons 26

  27. Reconstruct seesaw? ● ● Jνν coupling to measure U(1) L scale f. ● Use Jff couplings to reconstruct ● Diagonal K entries from e.g. Jee, Jμμ, and Jγγ. ● Off-diagonal |K αβ | from LFV: α→ βJ. ● Phase of off-diagonal K αβ ? Take from axion/ALP searches. Julian Heeck (ULB) - Majorons 27

  28. Lepton flavor violation ● Standard LFV in seesaw: ● Great signature, but requires light N R. ● With majoron: look for mono-energetic lepton: [Pilaftsis, ‘94; Feng, Moroi, Murayama, Schnapka, ‘98; Hirsch, Vicente, Meyer, Porod, ‘09] Julian Heeck (ULB) - Majorons 28

  29. μ→e J with J→ invisible ● TWIST, ‘15: limits on different anisotropies. ● Chiral coupling μP L eJ suppresses sensitivity! [JH, Camilo Garcia-Cely, 1701.07209] ● Bremsstrahlung is competitive: μ→e J γ. [Goldman, Hallin, Hoffman, Piilonen, Preston, ‘87] ● Approximate limit Julian Heeck (ULB) - Majorons 29

  30. τ → ℓ J with J→ invisible ● ARGUS, ‘95; 5e5 taus. ● Belle, ‘16 prelim.; 1e9 taus. τ → μ J O(20) times better than ARGUS! τ → e J m J (GeV) ● Also interesting for LFV Z’. [JH, 1602.03810; Altmannshofer, Chen, Dev, Soni, 1607.06832] ● Improvement with Belle-II. ● No limits yet on J→ visible or τ → ℓ J γ. Julian Heeck (ULB) - Majorons 30

  31. Mass origin via seesaw mechanism ● Introduce 3 singlets N R : ● For ● Majorana neutrinos: hope for 0νββ! ● Bonus: leptogenesis (even with majoron). [Aristizabal Sierra, Tortola, Valle, Vicente, ‘14] Julian Heeck (ULB) - Majorons 31

  32. Parametrization of our ignorance “Known”: PMNS mixing matrix 9 parameters not known: or ● M R (3 parameters) and ● Just [Davidson, Ibarra, hep-ph/0104076] ● Hermitian, contains 9 with real parameters. [Casas, Ibarra, hep-ph/0103065] ● ● Julian Heeck (ULB) - Majorons 32

  33. Spontaneous B – L breaking ● Instead of explicitly, break U(1) B-L spontaneously: ● New scalar Breaking scale Heavy scalar Majoron (inflaton?) [Chikashige, Mohapatra, Peccei, ‘81; Schechter, Valle, ‘82] ● Scalar potential: Julian Heeck (ULB) - Majorons 33

  34. Pseudo -Goldstone ● Spontaneous global U(1) breaking gives m J = 0 . ● Non-zero mass from: – Breaking by gravity, e.g. wormholes, [Alonso, Urbano, 1706.07415] – Anomalies, e.g. if U(1) B-L = U(1) PQ. [Mohapatra, Senjanovic ‘83; Langacker, Peccei, Yanagida ‘86; SMASH ‘16] – Explicit breaking, e.g. Stay ignorant here, just put m J . Julian Heeck (ULB) - Majorons 34

  35. Dark matter abundance ● Freeze out via λJJHH: – m J ~ m h /2, – m J > 400 GeV. Julian Heeck (ULB) - Majorons 35

  36. Dark matter abundance ● Freeze out via λJJHH: – m J ~ m h /2, – m J > 400 GeV. ● Freeze in: Stephen West Lyman-α constraints < 12 keV! Use different mechanism: JH, Teresi, 1706.09909, 1709.07283 . [McDonald, ‘02; Hall, Jedamzik, March-Russell, West ‘10; Frigerio, Hambye, Masso, ‘11] Julian Heeck (ULB) - Majorons 36

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