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相关论文: LEvEL: Low-Energy Neutrino Experiment at the LHC

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We discuss in detail the physics reach of an experimental set-up where electron neutrinos (anti-neutrinos) produced in a beta-beam facility at Fermi National Accelerator Laboratory (FNAL) are sent, over a distance of L~1300km, to the Deep…

高能物理 - 唯象学 · 物理学 2015-03-13 Sanjib Kumar Agarwalla , Patrick Huber

Neutrino trident production of di-lepton pairs is well recognized as a sensitive probe of both electroweak physics and physics beyond the Standard Model. Although a rare process, it could be significantly boosted by such new physics, and it…

高能物理 - 唯象学 · 物理学 2024-10-30 Wolfgang Altmannshofer , Toni Mäkelä , Subir Sarkar , Sebastian Trojanowski , Keping Xie , Bei Zhou

As long-baseline neutrino experiments enter the precision era, the difficulties associated with understanding neutrino interaction cross sections on atomic nuclei are expected to limit experimental sensitivities to oscillation parameters.…

SND@LHC is a compact and stand-alone experiment to perform measurements with neutrinos produced at the LHC in a hitherto unexplored pseudo-rapidity region of $7.2 < \eta < 8.4$, complementary to all the other experiments at the LHC. The…

高能物理 - 实验 · 物理学 2023-10-25 Ettore Zaffaroni

Heavy right-handed neutrinos (RHNs) provide the simplest explanation for the origin of light neutrino masses and mixings. If the RHN masses are at or below the weak scale, direct experimental discovery of these states is possible at…

高能物理 - 唯象学 · 物理学 2016-08-26 Brian Batell , Maxim Pospelov , Brian Shuve

We study the feasibility to observe sterile neutrinos with masses in the range 5 GeV $< m_N < 20$ GeV at the LHC, using exclusive semileptonic modes involving pions, $W\to \ell N \to \pi \ell\ell, 2\pi \ell\ell$ and $3\pi \ell\ell$. We thus…

高能物理 - 唯象学 · 物理学 2020-02-26 Claudio O. Dib , Choong Sun Kim , Sebastian Tapia Araya

We show that the Deep Underground Neutrino Experiment (DUNE), with significant but feasible new efforts, has the potential to deliver world-leading results in solar neutrinos. With a 100 kton-year exposure, DUNE could detect $\gtrsim 10^5$…

高能物理 - 唯象学 · 物理学 2020-07-27 Francesco Capozzi , Shirley Weishi Li , Guanying Zhu , John F. Beacom

The last energy-frontier lepton collider, LEP, established several limits that still hold today. A key one is the counting of three light neutrino species from the invisible decay width of the Z boson. From a collider calorimetry…

仪器与探测器 · 物理学 2025-05-19 Wonyong Chung

We present a new experimental method for measuring the process of Coherent Elastic Neutrino Nucleus Scattering (CENNS). This method uses a detector situated transverse to a high energy neutrino beam production target. This detector would be…

The neutrino trident scattering process in neutrino - tungsten interactions at the LHC energy regime is investigated, and the cross-sections for different leptonic final states in coherent and incoherent interactions are estimated.…

高能物理 - 唯象学 · 物理学 2024-06-21 Reinaldo Francener , Victor P. Goncalves , Diego R. Gratieri

Next generation neutrino oscillation experiments like DUNE and T2HK are multi-purpose observatories, with a rich physics program beyond oscillation measurements. A special role is played by their near detector facilities, which are…

高能物理 - 唯象学 · 物理学 2022-02-11 Moritz Breitbach , Luca Buonocore , Claudia Frugiuele , Joachim Kopp , Lukas Mittnacht

The Large Hadron Collider forward (LHCf) experiment has been designed to use the LHC to benchmark the hadronic interaction models used in cosmic-ray physics. The LHCf experiment measures neutral particles emitted in the very forward region…

Development of large mass detectors for low-energy neutrinos and dark matter may allow supernova detection via neutrino-nucleus elastic scattering. An elastic-scattering detector could observe a few, or more, events per ton for a galactic…

天体物理学 · 物理学 2009-11-07 C. J. Horowitz , K. J. Coakley , D. N. McKinsey

Neutrinos continue to provide a testing ground for the structure of the standard model of particle physics as well as hints towards the physics beyond the standard model. Neutrinos of energies spanning over several orders of magnitude,…

高能物理 - 唯象学 · 物理学 2023-12-19 V. Pandey

In the first 10 seconds of a core-collapse supernova, almost all of its progenitor's gravitational potential, O(10$^{53}$~ergs), is carried away in the form of neutrinos. These neutrinos, with O(10~MeV) kinetic energy, can interact via…

天体物理仪器与方法 · 物理学 2018-03-07 Dev Ashish Khaitan

We consider the production of a heavy neutrino and its possible signals at the Large Hadron-electron Collider (LHeC) in the context of an inverse-seesaw model for neutrino mass generation. The inverse seesaw model extends the Standard Model…

高能物理 - 唯象学 · 物理学 2016-08-31 Subhadeep Mondal , Santosh Kumar Rai

Soon, a new generation of neutrino telescopes, presently under planning, will target the discovery of ultra-high-energy (UHE) neutrinos of cosmic origin, with energies higher than 100 PeV, that promise unique insight into astrophysics and…

高能天体物理现象 · 物理学 2023-08-16 Victor B. Valera , Mauricio Bustamante , Olga Mena

Heavy neutral leptons are present in many well-motivated beyond the Standard Model theories, sometimes being accessible at present colliders. Depending on their masses and couplings they could be long-lived and lead to events with displaced…

高能物理 - 唯象学 · 物理学 2018-08-15 Xabier Marcano

Neutrinos provide a unique probe of both particle physics and the high-energy universe, traversing astronomical distances with minimal interaction. Their charged-current scattering cross section encodes fundamental information about weak…

高能物理 - 实验 · 物理学 2026-05-12 N. Bhuiyan , K. Abe , Y. Asaoka , M. Harada , Y. Hayato , K. Hiraide , T. H. Hung , K. Ieki , M. Ikeda , J. Kameda , Y. Kanemura , Y. Kataoka , S. Miki , S. Mine , M. Miura , S. Moriyama , K. Nakagiri , M. Nakahata , S. Nakayama , Y. Noguchi , G. Pronost , K. Sato , H. Sekiya , R. Shinoda , M. Shiozawa , Y. Suzuki , A. Takeda , Y. Takemoto , H. Tanaka , T. Yano , S. Chen , Y. Itow , T. Kajita , R. Nishijima , K. Okumura , T. Tashiro , T. Tomiya , X. Wang , P. Fernandez , F. J. de Garay Arcones , L. Labarga , D. Samudio , B. Zaldivar , C. Yanagisawa , B. Jargowsky , E. Kearns , J. Mirabito , L. Wan , T. Wester , B. W. Pointon , J. Bian , B. Cortez , N. J. Griskevich , Y. Jiang , M. B. Smy , H. W. Sobel , V. Takhistov , A. Yankelevich , J. Hill , D. H. Moon , R. G. Park , B. S. Yang , K. Scholberg , C. W. Walter , O. Drapier , A. Ershova , M. Ferey , E. Le Blévec , Th. A. Mueller , P. Paganini , C. Quach , R. Rogly , T. Nakamura , J. S. Jang , R. P. Litchfield , L. N. Machado , F. J. P. Soler , J. G. Learned , K. Choi , S. Cao , L. H. V. Anthony , N. W. Prouse , M. Scott , Y. Uchida , V. Berardi , N. F. Calabria , M. G. Catanesi , N. Ospina , E. Radicioni , A. Langella , G. De Rosa , G. Collazuol , M. Feltre , M. Mattiazzi , L. Ludovici , M. Gonin , L. Périssé , B. Quilain , M. Fukazawa , S. Horiuchi , A. Kawabata , M. Kobayashi , Y. M. Liu , Y. Maekawa , Y. Nishimura , A. Oka , R. Akutsu , M. Friend , T. Hasegawa , Y. Hino , T. Ishida , T. Kobayashi , T. Matsubara , T. Nakadaira , Y. Oyama , A. Portocarrero Yrey , K. Sakashita , T. Sekiguchi , G. T. Burton , F. Di Lodovico , T. Katori , R. Kralik , N. Latham , R. M. Ramsden , V. Siccardi , S. Aoyama , H. Banbara , Y. Inaba , H. Ito , M. Nishigami , T. Sone , A. T. Suzuki , Y. Takeuchi , S. Wada , H. Zhong , J. Feng , L. Feng , S. Han , J. Hikida , J. R. Hu , Z. Hu , M. Kawaue , T. Kikawa , T. Nakaya , T. V. Ngoc , R. A. Wendell , S. J. Jenkins , N. McCauley , A. Tarrant , M. Fanì , M. J. Wilking , Z. Xie , Y. Fukuda , H. Menjo , Y. Yoshioka , J. Lagoda , M. Mandal , J. Zalipska , M. Mori , J. Jiang , Y. Asano , K. Hamaguchi , H. Ishino , Y. Koshio , F. Nakanishi , S. Ohshita , T. Tada , T. Ishizuka , G. Barr , D. Barrow , L. Cook , S. Samani , D. Wark , A. Holin , F. Nova , M. Jo , S. Jung , J. Yoo , J. E. P. Fannon , L. Kneale , T. Peacock , P. Stowell , H. Okazawa , S. M. Lakshmi , S. Hong , E. Kwon , M. W. Lee , J. W. Seo , I. Yu , Y. Ashida , A. K. Ichikawa , K. D. Nakamura , S. Abe , S. Goto , S. Kodama , Y. Kong , H. Hayasaki , Y. Masaki , Y. Mizuno , T. Muro , K. Nakagiri , Y. Nakajima , M. Sekiyama , N. Taniuchi , T. Yamazumi , M. Yokoyama , P. de Perio , S. Fujita , C. Jesús-Valls , K. Martens , Ll. Marti , A. D. Santos , K. M. Tsui , M. R. Vagins , S. Izumiyama , M. Kuze , R. Matsumoto , R. Asaka , C. Ise , M. Ishitsuka , M. Sugo , M. Wako , K. Yamauchi , Y. Nakano , F. Cormier , R. Gaur , M. Hartz , A. Konaka , X. Li , B. R. Smithers , S. Chen , Y. Wu , B. D. Xu , A. Q. Zhang , B. Zhang , H. Adhikary , M. Girgus , P. Govindaraj , M. Posiadala-Zezula , Y. S. Prabhu , S. B. Boyd , R. Edwards , D. Hadley , M. O'Flaherty , B. Richards , A. Ali , B. Jamieson , C. Bronner , D. Horiguchi , A. Minamino , Y. Sasaki , R. Shibayama , R. Shimamura

Astrophysical and atmospheric neutrinos are important probes of the powerful accelerators that produce cosmic-rays with EeV energies. Understanding these accelerators is a key goal of neutrino observatories, along with searches for…

高能天体物理现象 · 物理学 2019-06-07 Spencer R. Klein