51猎奇入口

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • 51猎奇入口
    • Undergraduates
    • Postgraduates
  • Engage
    • For young people
    • For teachers
    • For the public
    • For alumni
    • For business
  • Support
Menu
LSST/Rubin Dome Bridge Installation
Credit: Rubin Obs/NSF/AURA

Dr Farrukh Azfar

Lecturer

Research theme

  • Particle astrophysics & cosmology
  • Fundamental particles and interactions

Sub department

  • Particle Physics

Research groups

  • Accelerator Neutrinos
  • Rubin-LSST
Farrukh.Azfar@physics.ox.ac.uk
Telephone: 01865 (2)73327
Denys Wilkinson Building, room 669
  • About
  • Publications

Deep Underground Neutrino Experiment (DUNE) near detector conceptual design report

Instruments MDPI 5:4 (2021) 31

Authors:

A Abed Abud, Babak Abi, R Acciarri, Farrukh Azfar, G Barr, F Battisti, P Hamacher-Baumann, C Hasnip, M Kabirnezhad, XG Lu, A Reynolds, P Rodrigues, F Spagliardi, A Weber, Kang Yang

Abstract:

The Deep Underground Neutrino Experiment (DUNE) is an international, world-class experiment aimed at exploring fundamental questions about the universe that are at the forefront of astrophysics and particle physics research. DUNE will study questions pertaining to the preponderance of matter over antimatter in the early universe, the dynamics of supernovae, the subtleties of neutrino interaction physics, and a number of beyond the Standard Model topics accessible in a powerful neutrino beam. A critical component of the DUNE physics program involves the study of changes in a powerful beam of neutrinos, i.e., neutrino oscillations, as the neutrinos propagate a long distance. The experiment consists of a near detector, sited close to the source of the beam, and a far detector, sited along the beam at a large distance. This document, the DUNE Near Detector Conceptual Design Report (CDR), describes the design of the DUNE near detector and the science program that drives the design and technology choices. The goals and requirements underlying the design, along with projected performance are given. It serves as a starting point for a more detailed design that will be described in future documents.

Supernova neutrino burst detection with the Deep Underground Neutrino Experiment

The European Physical Journal C SpringerOpen 81:5 (2021) 423

Authors:

B Abi, R Acciarri, MA Acero, G Adamov, D Adams, M Adinolfi, Z Ahmad, J Ahmed, T Alion, S Alonso Monsalve, C Alt, J Anderson, C Andreopoulos, MP Andrews, F Andrianala, S Andringa, A Ankowski, M Antonova, S Antusch, A Aranda-Fernandez, A Ariga, LO Arnold, MA Arroyave, J Asaadi, A Aurisano, V Aushev, D Autiero, F Azfar, H Back, JJ Back, C Backhouse, P Baesso, L Bagby, R Bajou, S Balasubramanian, P Baldi, B Bambah, F Barao, G Barenboim, GJ Barker, W Barkhouse, C Barnes, G Barr, J Barranco Monarca, N Barros, JL Barrow, A Bashyal, V Basque, F Bay, JL Bazo Alba

Abstract:

We investigate the feasibility of using deep learning techniques, in the form of a one-dimensional convolutional neural network (1D-CNN), for the extraction of signals from the raw waveforms produced by the individual channels of liquid argon time projection chamber (LArTPC) detectors. A minimal generic LArTPC detector model is developed to generate realistic noise and signal waveforms used to train and test the 1D-CNN, and evaluate its performance on low-level signals. We demonstrate that our approach overcomes the inherent shortcomings of traditional cut-based methods by extending sensitivity to signals with ADC values below their imposed thresholds. This approach exhibits great promise in enhancing the capabilities of future generation neutrino experiments like DUNE to carry out their low-energy neutrino physics programs

Supernova neutrino burst detection with the deep underground neutrino experiment: DUNE Collaboration

European Physical Journal C 81:5 (2021)

Authors:

B Abi, R Acciarri, MA Acero, G Adamov, D Adams, M Adinolfi, Z Ahmad, J Ahmed, T Alion, S Alonso Monsalve, C Alt, J Anderson, C Andreopoulos, MP Andrews, F Andrianala, S Andringa, A Ankowski, M Antonova, S Antusch, A Aranda-Fernandez, A Ariga, LO Arnold, MA Arroyave, J Asaadi, A Aurisano, V Aushev, D Autiero, F Azfar, H Back, JJ Back, C Backhouse, P Baesso, L Bagby, R Bajou, S Balasubramanian, P Baldi, B Bambah, F Barao, G Barenboim, GJ Barker, W Barkhouse, C Barnes, G Barr, J Barranco Monarca, N Barros, JL Barrow, A Bashyal, V Basque, F Bay, JLB Alba, JF Beacom, E Bechetoille, B Behera, L Bellantoni, G Bellettini, V Bellini, O Beltramello, D Belver, N Benekos, F Bento Neves, J Berger, S Berkman, P Bernardini, RM Berner, H Berns, S Bertolucci, M Betancourt, Y Bezawada, M Bhattacharjee, B Bhuyan, S Biagi, J Bian, M Biassoni, K Biery, B Bilki, M Bishai, A Bitadze, A Blake, B Blanco Siffert, FDM Blaszczyk, GC Blazey, E Blucher, J Boissevain, S Bolognesi, T Bolton, M Bonesini, M Bongrand, F Bonini, A Booth, C Booth, S Bordoni, A Borkum, T Boschi, N Bostan, P Bour, SB Boyd, D Boyden, J Bracinik, D Braga, D Brailsford

Abstract:

The deep underground neutrino experiment (DUNE), a 40-kton underground liquid argon time projection chamber experiment, will be sensitive to the electron-neutrino flavor component of the burst of neutrinos expected from the next Galactic core-collapse supernova. Such an observation will bring unique insight into the astrophysics of core collapse as well as into the properties of neutrinos. The general capabilities of DUNE for neutrino detection in the relevant few- to few-tens-of-MeV neutrino energy range will be described. As an example, DUNE鈥檚 ability to constrain the 谓e spectral parameters of the neutrino burst will be considered.

Measurement of the Positive Muon Anomalous Magnetic Moment to 0.46 ppm

(2021)

Authors:

B Abi, T Albahri, S Al-Kilani, D Allspach, LP Alonzi, A Anastasi, A Anisenkov, F Azfar, K Badgley, S Bae脽ler, I Bailey, VA Baranov, E Barlas-Yucel, T Barrett, E Barzi, A Basti, F Bedeschi, A Behnke, M Berz, M Bhattacharya, HP Binney, R Bjorkquist, P Bloom, J Bono, E Bottalico, T Bowcock, D Boyden, G Cantatore, RM Carey, J Carroll, BCK Casey, D Cauz, S Ceravolo, R Chakraborty, SP Chang, A Chapelain, S Chappa, S Charity, R Chislett, J Choi, Z Chu, TE Chupp, ME Convery, A Conway, G Corradi, S Corrodi, L Cotrozzi, JD Crnkovic, S Dabagov, PM De Lurgio, PT Debevec, S Di Falco, P Di Meo, G Di Sciascio, R Di Stefano, B Drendel, A Driutti, VN Duginov, M Eads, N Eggert, A Epps, J Esquivel, M Farooq, R Fatemi, C Ferrari, M Fertl, A Fiedler, AT Fienberg, A Fioretti, D Flay, SB Foster, H Friedsam, E Frle啪, NS Froemming, J Fry, C Fu, C Gabbanini, MD Galati, S Ganguly, A Garcia, DE Gastler, J George, LK Gibbons, A Gioiosa, KL Giovanetti, P Girotti, W Gohn, T Gorringe, J Grange, S Grant, F Gray, S Haciomeroglu, D Hahn, T Halewood-Leagas, D Hampai, F Han, E Hazen, J Hempstead, S Henry, AT Herrod, DW Hertzog, G Hesketh, A Hibbert, Z Hodge, JL Holzbauer, KW Hong, R Hong, M Iacovacci, M Incagli, C Johnstone, JA Johnstone, P Kammel, M Kargiantoulakis, M Karuza, J Kaspar, D Kawall, L Kelton, A Keshavarzi, D Kessler, KS Khaw, Z Khechadoorian, NV Khomutov, B Kiburg, M Kiburg, O Kim, SC Kim, YI Kim, B King, N Kinnaird, M Korostelev, I Kourbanis, E Kraegeloh, VA Krylov, A Kuchibhotla, NA Kuchinskiy, KR Labe, J LaBounty, M Lancaster, MJ Lee, S Lee, S Leo, B Li, D Li, L Li, I Logashenko, A Lorente Campos, A Luc脿, G Lukicov, G Luo, A Lusiani, AL Lyon, B MacCoy, R Madrak, K Makino, F Marignetti, S Mastroianni, S Maxfield, M McEvoy, W Merritt, AA Mikhailichenko, JP Miller, S Miozzi, JP Morgan, WM Morse, J Mott, E Motuk, A Nath, D Newton, H Nguyen, M Oberling, R Osofsky, J-F Ostiguy, S Park, G Pauletta, GM Piacentino, RN Pilato, KT Pitts, B Plaster, D Po膷ani膰, N Pohlman, CC Polly, M Popovic, J Price, B Quinn, N Raha, S Ramachandran, E Ramberg, NT Rider, JL Ritchie, BL Roberts, DL Rubin, L Santi, D Sathyan, H Schellman, C Schlesier, A Schreckenberger, YK Semertzidis, YM Shatunov, D Shemyakin, M Shenk, D Sim, MW Smith, A Smith, AK Soha, M Sorbara, D St枚ckinger, J Stapleton, D Still, C Stoughton, D Stratakis, C Strohman, T Stuttard, HE Swanson, G Sweetmore, DA Sweigart, MJ Syphers, DA Tarazona, T Teubner, AE Tewsley-Booth, K Thomson, V Tishchenko, NH Tran, W Turner, E Valetov, D Vasilkova, G Venanzoni, VP Volnykh, T Walton, M Warren, A Weisskopf, L Welty-Rieger, M Whitley, P Winter, A Wolski, M Wormald, W Wu, C Yoshikawa

Measurement of the positive muon anomalous magnetic moment to 0.46 ppm

Physical Review Letters American Physical Society 126 (2021) 141801

Authors:

B Abi, Farrukh Azfar, S Henry

Abstract:

We present the first results of the Fermilab National Accelerator Laboratory (FNAL) Muon g−2 Experiment for the positive muon magnetic anomaly aμ≡(gμ−2)/2. The anomaly is determined from the precision measurements of two angular frequencies. Intensity variation of high-energy positrons from muon decays directly encodes the difference frequency ωa between the spin-precession and cyclotron frequencies for polarized muons in a magnetic storage ring. The storage ring magnetic field is measured using nuclear magnetic resonance probes calibrated in terms of the equivalent proton spin precession frequency ˜ω′p in a spherical water sample at 34.7 °C. The ratio ωa/˜ω′p, together with known fundamental constants, determines aμ(FNAL)=116592040(54)×10−11 (0.46 ppm). The result is 3.3 standard deviations greater than the standard model prediction and is in excellent agreement with the previous Brookhaven National Laboratory (BNL) E821 measurement. After combination with previous measurements of both μ+ and μ−, the new experimental average of aμ(Exp)=116592061(41)×10−11 (0.35 ppm) increases the tension between experiment and theory to 4.2 standard deviations.

Pagination

  • First page First
  • Previous page Prev
  • …
  • Page 3
  • Page 4
  • Page 5
  • Page 6
  • Current page 7
  • Page 8
  • Page 9
  • Page 10
  • Page 11
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

漏 University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • 51猎奇入口
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • 51猎奇入口
  • Giving to Physics