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CPNR Workshop 2025

Neutrino with wave dark matter

From type oscillation to second leptogenesis

Yechan Kim

KAIST

PRD 108, 095028 (2023); JHEP 03 (2024) 003;

PRD 111, 055026 (2025); JHEP 07 (2025) 269

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Neutrino with wave dark matter

- Neutrino absolute mass

- Sterile neutrino

- Neutrino oscillation parameters

- Neutrino is Dirac type or Majorana type?

Many unknowns in Neutrino physics

- CP violation in PMNS

- Cosmic neutrino background (CnuB)

- Leptogenesis for BAU

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- Neutrino absolute mass

- Sterile neutrino

- Neutrino oscillation parameters

- Neutrino is Dirac type or Majorana type?

Many unknowns in Neutrino physics

- CP violation in PMNS

Wave dark matter

with ultra-light mass scale

Neutrino with wave dark matter

- Cosmic neutrino background (CnuB)

- Leptogenesis for BAU

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Neutrino mass variation

A Berlin (2016);

G Krnjaic, PAN Machado, L Necib (2017) …

Dirac-Majorana neutrino

type oscillation

YL ChoeJo, Y Kim, HS Lee (2023)

Potential oscillation

Y Kim, HS Lee (2025)

Second leptogenesis

YL ChoeJo, K Enomoto, Y Kim, HS Lee (2023);

YL ChoeJo, K Enomoto, Y Kim, HS Lee (2024)

Neutrino with wave dark matter

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Quasi-Dirac type

Seesaw is broken

Dirac-Majorana neutrino type oscillation

Seesaw

mechanism

Neutrinoless double

beta decay

Majorana type

LNV is suppressed

vs

Dirac

Majorana

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Dirac-Majorana neutrino type oscillation

Majorana

Quasi-Dirac

instantly

Pure-Dirac

Dirac-Majorana

neutrino type oscillation”

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Neutrino with wave dark matter (Yechan Kim)

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Majorana

type

Quasi-Dirac

type

LNV

LNV

Dirac-Majorana neutrino type oscillation

Turn-on/off behavior of 0νββ decay

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Potential oscillation

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Potential oscillation

Symmetry-restored

Symmetry-broken

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CPNR Workshop 2025

Potential oscillation

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Neutrino with wave dark matter (Yechan Kim)

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CPNR Workshop 2025

Potential oscillation

Implications for neutrino sector

 

Symmetry-restored

Symmetry-broken

Edoardo Vitagliano et al (2019)

Andrew J. Long et al (2014)

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Second leptogenesis

Temperature-dependent mass of N

1st

Production

1st

Decay

2nd

Production

2nd

Decay

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Neutrino with wave dark matter (Yechan Kim)

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Second leptogenesis

,

Lepton Asymmetry

Sphaleron

Baryon Asymmetry

CP-violating out-of-equilibrium decay of

Heavy Majorana neutrino

Leptogenesis

Sphaleron decoupling

EWSB

Second leptogenesis

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Second leptogenesis

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Second leptogenesis

Sphaleron decoupling

LAU

BAU

1st LG

2nd LG

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Summary

Thank You!

  • The interaction between neutrino and wave DM induce time-varying mass of the neutrino and also for the evolution over cosmic history.
  • The neutrino type may oscillate if the ratio of the Dirac and Majorana mass term varies.
  • The wave DM can generate the periodic symmetry breaking and restoration of the potential, and this leads to the modulation behavior of CnuB.
  • The temperature-dependent mass of the heavy neutrino provides the second leptogenesis, which can explain the large discrepancy between baryon and lepton asymmetries.

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Quasi-Dirac & Majorana limits

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Constraints on type oscillation

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Neutrino with wave dark matter (Yechan Kim)

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r: inter-nucleon distance (fm)

Neutrinoless double beta (0νββ) decay

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Conditions and constraints on potential oscillation

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Neutrino with wave dark matter (Yechan Kim)

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Singlet scalar dynamics in potential oscillation

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Remarks on potential oscillation

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Remarks on potential oscillation

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Parameter space for second LG

To avoid thermalization of wave DM by scattering

To avoid dominant quartic coupling

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Decay, scattering, and CP asymmetry in second LG