The WIMP Argon Programme (WARP) is an experiment at Laboratori Nazionali del Gran Sasso, Italy, for the research of cold dark matter.[1] It aims to detect nuclear recoils in liquid argon induced by weakly interacting massive particles (WIMP) through scintillation light; the apparatus can also detect ionization so to exclude interactions of photons and electrons. The experiment is a recognized CERN experiment (RE15).[2][3]
Collaboration Members
- Università degli Studi di Pavia e INFN
P.Benetti, E.Calligarich, M.Cambiaghi, C.Montanari(+), A.Rappoldi, G.L.Raselli, M.Roncadelli, M.Rossella, C.Vignoli
- Laboratori Nazionali del Gran Sasso (INFN-LNGS)
M. Antonello, O.Palamara, L.Pandola, C.Rubbia(*), E.Segreto, A.Szelc
- Università degli Studi dell'Aquila e INFN
R.Acciarri, M. Antonello, N. Canci, F.Cavanna, F.Di Pompeo(++), L.Grandi(++)
(++ also at INFN-LNGS)
- Università degli Studi di Napoli e INFN
F.Carbonara, A.Cocco, G.Fiorillo, G.Mangano
- Princeton University Department of Physics
F.Calaprice, C.Galbiati, B.Loer, R.Saldanha
- Università degli Studi di Padova e INFN
B.Baibussinov, S.Centro, M.B.Ceolin, G.Meng, F.Pietropaolo,S.Ventura
References
- ↑ Acciarri, R; Antonello, M; Baibussinov, B; Benetti, P; Calaprice, F; Calligarich, E; Cambiaghi, M; Canci, N et al. (2010-01-01). "The WArP experiment". Journal of Physics: Conference Series (IOP Publishing) 203 (1): 012006. doi:10.1088/1742-6596/203/1/012006. ISSN 1742-6596. Bibcode: 2010JPhCS.203a2006A.
- ↑ "Recognized Experiments at CERN". CERN. http://committees.web.cern.ch/rec/welcome.html.
- ↑ "RE15/WARP: A double phase argon programme for dark matter detection". CERN. https://greybook.cern.ch/greybook/experiment/detail?id=RE15.
External links
- WARP: Wimp Argon Programme, on the LNGS website.
Dark matter |
|---|
| 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 |
- Axino
- Axion
- Dark photon
- Holeum
- LSP
- Minicharged particle
- Neutralino
- Sterile neutrino
- SIMP
- WIMP
|
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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 |
- Antimatter
- Dark energy
- Exotic matter
- Galaxy formation and evolution
- Illustris project
- Imaginary mass
- Negative mass
- UniverseMachine
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 | Original source: https://en.wikipedia.org/wiki/WIMP Argon Programme. Read more |