91̽»¨

Skip to main content
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding 91̽»¨
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
  • Support
91̽»¨
Bullet cluster image
Credit: Credit: X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.; Lensing Map: NASA/STScI

Professor Jocelyn Monroe

Professor of Particle Physics

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Particle Physics
jocelyn.monroe@physics.ox.ac.uk
Telephone: 273317
  • About
  • Publications

Search for low mass dark matter in DarkSide-50: the bayesian network approach

The European Physical Journal C SpringerOpen 83:4 (2023)

Authors:

P Agnes, IFM Albuquerque, T Alexander, AK Alton, M Ave, HO Back, G Batignani, K Biery, V Bocci, WM Bonivento, B Bottino, S Bussino, M Cadeddu, M Cadoni, F Calaprice, A Caminata, MD Campos, N Canci, M Caravati, N Cargioli, M Cariello, M Carlini, V Cataudella, P Cavalcante, S Cavuoti, S Chashin, A Chepurnov, C Cicalò, G Covone, D D’Angelo, S Davini, A De Candia, S De Cecco, G De Filippis, G De Rosa, AV Derbin, A Devoto, M D’Incecco, C Dionisi, F Dordei, M Downing, D D’Urso, M Fairbairn, G Fiorillo, D Franco, F Gabriele, C Galbiati, C Ghiano, C Giganti, GK Giovanetti

Abstract:

This study explores a minimal renormalizable dark matter (DM) model, incorporating a sub-GeV Majorana DM and a singlet scalar particle $\phi$. Using scalar and pseudo-scalar interactions (couplings $c_s$ and $c_p$), we investigate implications for DM detection, considering $s$-wave, $p$-wave, and combined ($s$+$p$ wave) contributions in DM annihilation cross-section, as well as loop-correction contributions to DM-nucleon elastic scattering. Identifying a broad parameter space ($10 \,\rm{MeV} < m_\chi \lesssim m_\phi$) within the $2\sigma$ allowed region, we explore scenarios ($\left|c_s\right|\gg \left|c_p\right|$, $\left|c_s\right|\ll \left|c_p\right|$, and $\left|c_s\right|\approx \left|c_p\right|$). We find that (i) a non-zero pseudo-scalar coupling alleviates direct detection constraints as a comparison with the previous pure scalar coupling case; (ii) CMB observations set stringent limits on pseudo-scalar interaction dominant cases, making $s$-wave annihilation viable only for $m_\chi>1\,\rm{GeV}$; (iii) the preferred $\phi$-resonance region can be tested in the future indirect detection experiments, such as e-ASTROGAM.Comment: 35 pages, 4 figure

Search for low-mass dark matter WIMPs with 12 ton-day exposure of DarkSide-50

Physical Review D 107:6 (2023)

Authors:

P Agnes, Ifm Albuquerque, T Alexander, Ak Alton, M Ave, Ho Back, G Batignani, K Biery, V Bocci, Wm Bonivento, B Bottino, S Bussino, M Cadeddu, M Cadoni, F Calaprice, A Caminata, N Canci, M Caravati, N Cargioli, M Cariello, M Carlini, V Cataudella, P Cavalcante, S Cavuoti, S Chashin, A Chepurnov, C Cicalò, G Covone, D D'Angelo, S Davini, A De Candia, S De Cecco, G De Filippis, G De Rosa, Av Derbin, A Devoto, M D'Incecco, C Dionisi, F Dordei, M Downing, D D'Urso, G Fiorillo, D Franco, F Gabriele, C Galbiati, C Ghiano, C Giganti, Gk Giovanetti, Am Goretti, G Grilli Di Cortona

Abstract:

We report on the search for dark matter weakly interacting massive particles (WIMPs) in the mass range below 10 GeV/c2, from the analysis of the entire dataset acquired with a low-radioactivity argon target by the DarkSide-50 experiment at Laboratori Nazionali del Gran Sasso. The new analysis benefits from more accurate calibration of the detector response, improved background model, and better determination of systematic uncertainties, allowing us to accurately model the background rate and spectra down to 0.06 keVer. A 90% C.L. exclusion limit for the spin-independent cross section of 3 GeV/c2 mass WIMP on nucleons is set at 6×10-43 cm2, about a factor 10 better than the previous DarkSide-50 limit. This analysis extends the exclusion region for spin-independent dark matter interactions below the current experimental constraints in the [1.2, 3.6] GeV/c2 WIMP mass range.

Search for Dark Matter Particle Interactions with Electron Final States with DarkSide-50.

Physical review letters 130:10 (2023) 101002

Authors:

P Agnes, Ifm Albuquerque, T Alexander, Ak Alton, M Ave, Ho Back, G Batignani, K Biery, V Bocci, Wm Bonivento, B Bottino, S Bussino, M Cadeddu, M Cadoni, F Calaprice, A Caminata, Md Campos, N Canci, M Caravati, N Cargioli, M Cariello, M Carlini, V Cataudella, P Cavalcante, S Cavuoti, S Chashin, A Chepurnov, C Cicalò, G Covone, D D'Angelo, S Davini, A De Candia, S De Cecco, G De Filippis, G De Rosa, Av Derbin, A Devoto, M D'Incecco, C Dionisi, F Dordei, M Downing, D D'Urso, G Fiorillo, D Franco, F Gabriele, C Galbiati, C Ghiano, C Giganti, Gk Giovanetti, Am Goretti

Abstract:

We present a search for dark matter particles with sub-GeV/c^{2} masses whose interactions have final state electrons using the DarkSide-50 experiment's (12 306±184)  kg d low-radioactivity liquid argon exposure. By analyzing the ionization signals, we exclude new parameter space for the dark matter-electron cross section σ[over ¯]_{e}, the axioelectric coupling constant g_{Ae}, and the dark photon kinetic mixing parameter κ. We also set the first dark matter direct-detection constraints on the mixing angle |U_{e4}|^{2} for keV/c^{2} sterile neutrinos.

Search for Dark-Matter-Nucleon Interactions via Migdal Effect with DarkSide-50.

Physical review letters 130:10 (2023) 101001

Authors:

P Agnes, Ifm Albuquerque, T Alexander, Ak Alton, M Ave, Ho Back, G Batignani, K Biery, V Bocci, Wm Bonivento, B Bottino, S Bussino, M Cadeddu, M Cadoni, F Calaprice, A Caminata, Md Campos, N Canci, M Caravati, N Cargioli, M Cariello, M Carlini, V Cataudella, P Cavalcante, S Cavuoti, S Chashin, A Chepurnov, C Cicalò, G Covone, D D'Angelo, S Davini, A De Candia, S De Cecco, G De Filippis, G De Rosa, Av Derbin, A Devoto, M D'Incecco, C Dionisi, F Dordei, M Downing, D D'Urso, M Fairbairn, G Fiorillo, D Franco, F Gabriele, C Galbiati, C Ghiano, C Giganti, Gk Giovanetti

Abstract:

Dark matter elastic scattering off nuclei can result in the excitation and ionization of the recoiling atom through the so-called Migdal effect. The energy deposition from the ionization electron adds to the energy deposited by the recoiling nuclear system and allows for the detection of interactions of sub-GeV/c^{2} mass dark matter. We present new constraints for sub-GeV/c^{2} dark matter using the dual-phase liquid argon time projection chamber of the DarkSide-50 experiment with an exposure of (12 306±184)  kg d. The analysis is based on the ionization signal alone and significantly enhances the sensitivity of DarkSide-50, enabling sensitivity to dark matter with masses down to 40  MeV/c^{2}. Furthermore, it sets the most stringent upper limit on the spin independent dark matter nucleon cross section for masses below 3.6  GeV/c^{2}.

Volume reduction of water samples to increase sensitivity for radioassay of lead contamination

Applied Water Science Springer 12:7 (2022)

Authors:

A Aguilar-Arevalo, C Canet, MA Cruz-Pérez, A Deisting, A Dias, JC D’Olivo, F Favela-Pérez, EA Garcés, A González Muñoz, JO Guerra-Pulido, J Mancera-Alejandrez, DJ Marín-Lámbarri, M Martinez Montero, JR Monroe, S Paling, SJM Peeters, PR Scovell, C Türkoğlu, E Vázquez-Jáuregui, J Walding

Abstract:

The World Health Organisation (WHO) presents an upper limit for lead in drinking water of 10 parts per billion ppb. Typically, to reach this level of sensitivity, expensive metrology is required. To increase the sensitivity range of low-cost devices, this paper explores the prospects of using a volume reduction technique of a boiled water sample doped with Lead-210 (210 Pb), as a means to increase the solute’s concentration. 210Pb is a radioactive lead isotope and its concentration in a water sample can be measured with e.g. High Purity Germanium (HPGe) detectors at the Boulby Underground Germanium Suite. Concentrations close to the WHO limit have not been examined. This paper presents a measurement of the volume reduction technique retaining 99±(9)% of 210Pb starting from a concentration of 1.9×10−6 ppb before reduction and resulting in 2.63×10−4 ppb after reduction. This work also applies the volume reduction technique to London tap water and reports the radioassay results from gamma counting in HPGe detectors. Among other radio-isotopes, 40K, 210Pb, 131I and 177Lu were identified at measured concentrations of 2.83×103 ppb, 2.55×10−7 ppb, 5.06×10−10 ppb and 5.84×10−10 ppb in the London tap water sample. This technique retained 90±50% of 40K. Stable lead was inferred from the same water sample at a measured concentration of 0.012 ppb, prior to reduction

Pagination

  • First page First
  • Previous page Prev
  • Page 1
  • Page 2
  • Page 3
  • Page 4
  • Current page 5
  • Page 6
  • Page 7
  • Page 8
  • Page 9
  • …
  • Next page Next
  • Last page Last

Footer 91̽»¨

  • 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,

91̽»¨,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

Department Of Physics text logo

© 91̽»¨ - Department of Physics

Cookies | Privacy policy | Accessibility statement

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Giving to Physics