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Related papers: Recoiling Ion-Channeling in Direct Dark Matter Det…

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The channeling of the recoiling nucleus in crystalline detectors after a WIMP collision would produce a larger scintillation or ionization signal in direct detection experiments than otherwise expected. I present estimates of the importance…

High Energy Physics - Phenomenology · Physics 2010-12-20 Graciela B. Gelmini

The channeling of the recoiling nucleus in crystalline detectors after a WIMP collision would produce a larger scintillation or ionization signal in direct detection experiments than otherwise expected. I present estimates of the importance…

High Energy Physics - Phenomenology · Physics 2010-02-11 Graciela B. Gelmini

The channeling of the ion recoiling after a collision with a WIMP changes the ionization signal in direct detection experiments, producing a larger signal scintillation or ionization than otherwise expected. We give estimates of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Nassim Bozorgnia , Graciela B. Gelmini , Paolo Gondolo

The channeling of the ion recoiling after a collision with a WIMP changes the ionization signal in direct detection experiments, producing a larger signal than otherwise expected. We give estimates of the fraction of channeled recoiling…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Nassim Bozorgnia

The channeling of the ion recoiling after a collision with a WIMP changes the ionization signal in direct detection experiments, producing a larger signal than otherwise expected. We give estimates of the fraction of channeled recoiling…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-09 Nassim Bozorgnia , Graciela B. Gelmini , Paolo Gondolo

The channeling of the ion recoiling after a collision with a WIMP changes the ionization signal in direct detection experiments, producing a larger scintillation or ionization signal than otherwise expected. We give estimates of the…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Nassim Bozorgnia , Graciela B. Gelmini , Paolo Gondolo

The channeling of the ion recoiling after a collision with a WIMP changes the ionization signal in direct detection experiments, producing a larger signal than otherwise expected. We give estimates of the fraction of channeled recoiling…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-01 Nassim Bozorgnia , Graciela B. Gelmini , Paolo Gondolo

The channeling effect in crystals refers to the orientation dependence of charged ion penetration in crystals. In direct dark matter crystalline detectors, a channeled ion recoiling after a collision with a WIMP gives all its energy to…

Instrumentation and Methods for Astrophysics · Physics 2011-09-06 Nassim Bozorgnia

The channeling of the ion recoiling after a collision with a WIMP in direct dark matter crystalline detectors produces a larger scintillation or ionization signal than otherwise expected. Channeling is a directional effect which depends on…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Nassim Bozorgnia , Graciela B. Gelmini , Paolo Gondolo

In this paper we study the effect of the channeling of ions recoiling from collisions with weakly interacting massive particles (WIMPs) in single crystal detectors. In particular we investigate the possibility that channeling may give rise…

Instrumentation and Methods for Astrophysics · Physics 2015-05-19 Richard J. Creswick , Shmuel Nussinov , Frank T. Avignone

Channeling of recoil ions in various crystals strongly depends on their direction. This, along with the WIMP wind due to the rotation of the galactic disc generates {\it daily} modulations of the channeling. Since channeling affect the…

High Energy Physics - Phenomenology · Physics 2008-07-25 Frank T. Avignone , Richard J Creswick , Shmuel Nussinov

Direct detection of dark matter with directional sensitivity is a promising concept for improving the search for weakly interacting massive particles. With information on the direction of WIMP induced nuclear recoils one has access to the…

High Energy Physics - Phenomenology · Physics 2015-10-15 Ciaran A. J. O'Hare

Cosmological observations indicate that most of the matter in the Universe is Dark Matter. Dark Matter in the form of Weakly Interacting Massive Particles (WIMPs) can be detected directly, via its elastic scattering off target nuclei. Most…

Directional detection can provide unambiguous observation of Dark Matter interactions even in presence of insidious backgrounds. The DM-TPC collaboration is developing a detector with the goal of measuring the direction and sense of nuclear…

Directional detection can provide unambiguous observation of Dark Matter interactions even in presence of insidious backgrounds. The DM-TPC collaboration is developing a detector with the goal of measuring the direction and sense of nuclear…

We propose a method to identify the direction of an incident Weakly Interacting Massive Particle (WIMP) via induced nuclear recoil. Our method is based on spectroscopic interrogation of quantum defects in macroscopic solid-state crystals .…

High Energy Physics - Phenomenology · Physics 2017-08-23 Surjeet Rajendran , Nicholas Zobrist , Alexander O. Sushkov , Ronald Walsworth , Mikhail Lukin

Measurement of the direction of the elastic nuclear recoil track and ionization charge distribution along it, gives unique possibility for unambiguous detection of the dark matter WIMP particle. Within current radiation detection…

Instrumentation and Detectors · Physics 2017-08-23 N. J. C. Spooner , P. Majewski

The direct search for dark matter in the form of weakly interacting massive particles (WIMP) is performed by detecting nuclear recoils (NR) produced in a target material from the WIMP elastic scattering. A promising experimental strategy…

Instrumentation and Detectors · Physics 2024-01-12 20k Collaboration , P. Agnes , I. Ahmad , S. Albergo , I. F. M. Albuquerque , T. Alexander , A. K. Alton , P. Amaudruz , M. Atzori Corona , M. Ave , I. Ch. Avetisov , O. Azzolini , H. O. Back , Z. Balmforth , A. Barrado-Olmedo , P. Barrillon , A. Basco , G. Batignani , V. Bocci , W. M. Bonivento , B. Bottino , M. G. Boulay , J. Busto , M. Cadeddu , A. Caminata , N. Canci , G. Cappello , A. Capra , S. Caprioli , M. Caravati , N. Cargioli , M. Carlini , P. Castello , V. Cataudella , P. Cavalcante , S. Cavuoti , S. Cebrian , J. M. Cela Ruiz , S. Chashin , A. Chepurnov , E. Chyhyrynets , L. Cifarelli , D. Cintas , M. Citterio , B. Cleveland , V. Cocco , E. Conde Vilda , L. Consiglio , S. Copello , G. Covone , M. Czubak , M. D'Aniello , S. D'Auria , M. D. Da Rocha Rolo , S. Davini , A. de Candia , S. De Cecco , D. De Gruttola , G. De Filippis , D. Dell'Aquila , S. De Pasquale , G. De Rosa , G. Dellacasa , A. V. Derbin , A. Devoto , F. Di Capua , L. Di Noto , C. Dionisi , P. Di Stefano , G. Dolganov , F. Dordei , A. Elersich , E. Ellingwood , T. Erjavec , M. Fernandez Diaz , G. Fiorillo , P. Franchini , D. Franco , N. Funicello , F. Gabriele , D. Gahan , C. Galbiati , G. Gallina , G. Gallus , M. Garbini , P. Garcia Abia , A. Gendotti , C. Ghiano , C. Giganti , G. K. Giovanetti , V. Goicoechea Casanueva , A. Gola , G. Grauso , G. Grilli di Cortona , A. Grobov , M. Gromov , M. Guan , M. Guerzoni , M. Gulino , C. Guo , B. R. Hackett , A. L. Hallin , A. Hamer , M. Haranczyk , T. Hessel , S. Hill , S. Horikawa , F. Hubaut , J. Hucker , T. Hugues , An. Ianni , V. Ippolito , C. Jillings , S. Jois , P. Kachru , N. Kemmerich , A. A. Kemp , C. L. Kendziora , M. Kimura , I. Kochanek , K. Kondo , G. Korga , S. Koulosousas , A. Kubankin , M. Kuss , M. Kuzniak , M. La Commara , M. Lai , E. Le Guirriec , E. Leason , A. Leoni , X. Li , L. Lidey , M. Lissia , L. Luzzi , O. Lychagina , O. Macfadyen , I. N. Machulin , S. Manecki , I. Manthos , L. Mapelli , A. Margotti , S. M. Marik , C. Mariani , J. Maricic , A. Marini , M. Martínez , C. J. Martoff , G. Matteucci , K. Mavrokoridis , A. B. McDonald , A. Messina , R. Milincic , A. Mitra , A. Moharana , J. Monroe , E. Moretti , M. Morrocchi , T. Mróz , V. N. Muratova , C. Muscas , P. Musico , R. Nania , M. Nessi , G. Nieradka , K. Nikolopoulos , J. Nowak , K. Olchansky , A. Oleinik , V. Oleynikov , P. Organtini , A. Ortiz de Solórzano , L. Pagani , M. Pallavicini , L. Pandola , E. Pantic , E. Paoloni , G. Paternoster , P. A. Pegoraro , K. Pelczar , V. Pesudo , S. Piacentini , N. Pino , A. Pocar , D. M. Poehlmann , S. Pordes , P. Pralavorio , D. Price , F. Ragusa , Y. Ramachers , M. Razeti , A. L. Renshaw , M. Rescigno , F. Retiere , L. P. Rignanese , C. Ripoli , A. Rivetti , A. Roberts , C. Roberts , J. Rode , G. Rogers , L. Romero , M. Rossi , A. Rubbia , M. A. Sabia , P. Salomone , E. Sandford , S. Sanfilippo , D. Santone , R. Santorelli , C. Savarese , E. Scapparone , G. Schillaci , F. G. Schuckman , G. Scioli , M. Simeone , P. Skensved , M. D. Skorokhvatov , O. Smirnov , T. Smirnova , B. Smith , A. Sosa , F. Spadoni , M. Spangenberg , R. Stefanizzi , A. Steri , V. Stornelli , S. Stracka , M. Stringer , S. Sulis , A. Sung , Y. Suvorov , A. M. Szelc , R. Tartaglia , A. Taylor , J. Taylor , S. Tedesco , G. Testera , K. Thieme , T. N. Thorpe , A. Tonazzo , A. Tricomi , E. V. Unzhakov , T. Vallivilayil John , M. Van Uffelen , T. Viant , S. Viel , R. B. Vogelaar , J. Vossebeld , M. Wada , M. B. Walczak , H. Wang , Y. Wang , S. Westerdale , L. Williams , I. Wingerter-Seez , R. Wojaczynski , Ma. M. Wojcik , T. Wright , Y. Xie , C. Yang , A. Zabihi , P. Zakhary , A. Zani , A. Zichichi , G. Zuzel , M. P. Zykova

In direct dark matter detection experiments, conventional elastic scattering of WIMPs results in exponentially falling recoil spectra. In contrast, theories of WIMPs with excited states can lead to nuclear recoil spectra that peak at finite…

High Energy Physics - Phenomenology · Physics 2014-11-20 Rafael F. Lang , Neal Weiner
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