WIMP Argon Programme

You can help expand this article with text translated from the corresponding article in українська.  (November 2018) Click [show] for important translation instructions.

*   * Machine translation, like DeepL or Google Translate, is a useful starting point for translations, but translators must revise errors as necessary and confirm that the translation is accurate, rather than simply copy-pasting machine-translated text into the English Wikipedia.
* Do not translate text that appears unreliable or low-quality. If possible, verify the text with references provided in the foreign-language article.
* You must provide copyright attribution in the edit summary accompanying your translation by providing an interlanguage link to the source of your translation. A model attribution edit summary is `Content in this edit is translated from the existing українська Wikipedia article at [[:uk:Exact name of the українська article]]; see its history for attribution.`
* You may also add the template `{{Translated page|uk|Exact name of українська article}}` to the talk page.
* For more guidance, see Wikipedia:Translation.

|

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

1. ↑ 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). doi:10.1088/1742-6596/203/1/012006. ISSN 1742-6596. Bibcode: 2010JPhCS.203a2006A.
2. ↑ "Recognized Experiments at CERN". CERN. http://committees.web.cern.ch/rec/welcome.html.
3. ↑ "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.

* v
* t
* e

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

Hypothetical particles|

* Axino
* Axion
* Dark photon
* Holeum
* LSP
* Minicharged particle
* Neutralino
* Sterile neutrino
* SIMP
* WIMP

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

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

|

Indirect detection|

* AMS-02
* ANTARES
* ATIC
* CALET
* CAST
* DAMPE
* Fermi
* HAWC
* HESS
* IceCube
* MAGIC
* MOA
* OGLE
* PAMELA
* VERITAS

Other projects|

* MultiDark
* PVLAS

Potential dark galaxies|

* HE0450-2958
* HVC 127-41-330
* Smith's Cloud
* VIRGOHI21

Related|

* Antimatter
* Dark energy
* Exotic matter
* Galaxy formation and evolution
* Illustris project
* Imaginary mass
* Negative mass
* UniverseMachine

0.00

(0 votes)

Original source: https://en.wikipedia.org/wiki/WIMP Argon Programme. Read more

|

Retrieved from "https://handwiki.org/wiki/index.php?title=Physics:WIMP_Argon_Programme&oldid=3843064"
*[v]: View this template
*[t]: Discuss this template
*[e]: Edit this template