Sterile neutrinos, also known as neutral heavy leptons, heavy neutrinos, or right-handed neutrinos, are theoretical particles that are extremely difficult to find. This is because they are not affected by all of fundamental forces that rule normal physics, only gravity. They are detected by a theory called the seesaw mechanism which says that when sterile neutrinos are near other neutrinos (tiny particles which are not affected by much), they increase their own mass by lowering the mass of the nearby neutrinos. Detection probably comes from the fact that they are affected by gravity.
Think of it as a particle that absorbs the energy of other particles of the same family type. Once one is near another of its family, it raises its mass by lowering (absorbing) another's overall mass.
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| Elementary | |
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| Composite | | Hadrons | | Baryons |
- Nucleon
- Delta baryon
- Lambda baryon
- Sigma baryon
- Xi baryon
- Omega baryon
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| Mesons |
- Pion
- Rho meson
- Eta and eta prime mesons
- Bottom eta meson
- Phi meson
- J/psi meson
- Omega meson
- Upsilon meson
- Kaon
- B meson
- D meson
- Quarkonium
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| Exotic hadrons |
- Tetraquark (Double-charm tetraquark)
- Pentaquark
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| Others | |
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| Hypothetical | | Baryons | |
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| Mesons |
- Glueball
- Theta meson
- T meson
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| | Others |
- Mesonic molecule
- Pomeron
- Diquark
- R-hadron
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| Quasiparticles | |
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| Lists |
- Baryons
- Mesons
- Particles
- Quasiparticles
- Timeline of particle discoveries
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| Related | |
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Forms of dark matter |
- Baryonic dark matter
- Cold dark matter
- Hot dark matter
- Light dark matter
- Mixed dark matter
- Warm dark matter
- Self-interacting dark matter
- Scalar field dark matter
- Primordial black holes
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| Hypothetical particles | |
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Theories and objects |
- Cuspy halo problem
- Dark fluid
- Dark galaxy
- Dark globular cluster
- Dark matter halo
- Dark radiation
- Dark star
- Dwarf galaxy problem
- Halo mass function
- Mass dimension one fermions
- Massive compact halo object
- Mirror matter
- Navarro–Frenk–White profile
- Scalar field dark matter
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Search experiments | Direct detection |
- ADMX
- ANAIS
- ArDM
- CDEX
- CDMS
- CLEAN
- CoGeNT
- COSINE
- COUPP
- CRESST
- CUORE
- D3
- DAMA/LIBRA
- DAMA/NaI
- DAMIC
- DarkSide
- DARWIN
- DEAP
- DM-Ice
- DMTPC
- DRIFT
- EDELWEISS
- EURECA
- KIMS
- LUX
- LZ
- MACRO
- MIMAC
- NAIAD
- NEWAGE
- NEWS-G
- PandaX
- PICASSO
- PICO
- ROSEBUD
- SABRE
- SIMPLE
- TREX-DM
- UKDMC
- WARP
- XENON
- XMASS
- ZEPLIN
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Indirect detection |
- AMS-02
- ANTARES
- ATIC
- CALET
- CAST
- DAMPE
- Fermi
- HAWC
- HESS
- IceCube
- MAGIC
- MOA
- OGLE
- PAMELA
- VERITAS
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| Other projects | |
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| Potential dark galaxies |
- HE0450-2958
- HVC 127-41-330
- Smith's Cloud
- VIRGOHI21
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| Related | |
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