Mary Hall Reno

Dr. Mary Hall Reno


Research Focus & Metrics

Academic Career Length

44Years (1983-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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24 October 2016 in Reports on Progress in Physics
Verified
Journal Article
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SASergey Alekhin
Sergey Alekhin
WAWolfgang Altmannshofer
Wolfgang Altmannshofer
TATakehiko Asaka
Takehiko Asaka
BBBrian Batell
Brian Batell
FBFedor Bezrukov
Fedor Bezrukov
KZKathryn M Zurek
Kathryn M Zurek
This paper describes the physics case for a new fixed target facility at CERN SPS. The SHiP ( search for hidden particles ) experiment is intended to hunt for new physics in the largely unexplored domain of very weakly interacting particles with masses below the Fermi scale, inaccessible to the LHC experiments, and to study tau neutrino physics. The same proton beam setup can be used later to look for decays of tau-leptons with lepton flavour number non-conservation, τ → 3 μ and to search for weakly-interacting sub-GeV dark matter candidates. We discuss the evidence for physics beyond the standard model and describe interactions between new particles and four different portals —scalars, vectors, fermions or axion-like particles. We discuss motivations for different models, manifesting themselves via these interactions, and how they can be probed with the SHiP experiment and present several case studies. The prospects to search for relatively light SUSY and composite particles at SHiP are also discussed. We demonstrate that the SHiP experiment has a unique potential to discover new physics and can directly probe a number of solutions of beyond the standard model puzzles, such as neutrino masses, baryon asymmetry of the Universe, dark matter, and inflation.

30 September 1998 in Physical Review D
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RGRaj Gandhi
Raj Gandhi
CQChris Quigg
Chris Quigg
MRMary Hall Reno
Mary Hall Reno
ISIna Sarcevic
Ina Sarcevic
We report new calculations of the cross sections for deeply inelastic neutrino-nucleon scattering at neutrino energies between 109eV and 1021eV. We compare with results in the literature and assess the reliability of our predictions. For completeness, we briefly review the cross sections for neutrino interactions with atomic electrons, emphasizing the role of the W-boson resonance in ν¯ee interactions for neutrino energies in the neighborhood of 6.3 PeV. Adopting model predictions for extraterrestrial neutrino fluxes from active galactic nuclei, gamma-ray bursters, and the collapse of topological defects, we estimate event rates in large-volume water Čerenkov detectors and large-area ground arrays.

1 August 1996 in Astroparticle Physics
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Journal Article
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RGRaj Gandhi
Raj Gandhi
CQChris Quigg
Chris Quigg
MRMary Hall Reno
Mary Hall Reno
ISIna Sarcevic
Ina Sarcevic

20 January 2023 in Journal of Physics G: Nuclear and Particle Physics
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Journal Article
Open access
JFJonathan L Feng
Jonathan L Feng
FKFelix Kling
Felix Kling
MRMary Hall Reno
Mary Hall Reno
JRJuan Rojo
Juan Rojo
DSDennis Soldin
Dennis Soldin
RFRenata Zukanovich Funchal
Renata Zukanovich Funchal
High energy collisions at the High-Luminosity Large Hadron Collider (LHC) produce a large number of particles along the beam collision axis, outside of the acceptance of existing LHC experiments. The proposed Forward Physics Facility (FPF), to be located several hundred meters from the ATLAS interaction point and shielded by concrete and rock, will host a suite of experiments to probe standard model (SM) processes and search for physics beyond the standard model (BSM). In this report, we review the status of the civil engineering plans and the experiments to explore the diverse physics signals that can be uniquely probed in the forward region. FPF experiments will be sensitive to a broad range of BSM physics through searches for new particle scattering or decay signatures and deviations from SM expectations in high statistics analyses with TeV neutrinos in this low-background environment. High statistics neutrino detection will also provide valuable data for fundamental topics in perturbative and non-perturbative QCD and in weak interactions. Experiments at the FPF will enable synergies between forward particle production at the LHC and astroparticle physics to be exploited. We report here on these physics topics, on infrastructure, detector, and simulation studies, and on future directions to realize the FPF’s physics potential.

20 August 2008 in Physical Review D
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RERikard Enberg
Rikard Enberg
MRMary Hall Reno
Mary Hall Reno
ISIna Sarcevic
Ina Sarcevic
We calculate the prompt neutrino flux from atmospheric charm production by cosmic rays, using the dipole picture in a perturbative QCD framework, which incorporates the parton saturation effects present at high energies. We compare our results with the next-to-leading-order perturbative QCD result and find that saturation effects are large for neutrino energies above 106  GeV, leading to a substantial suppression of the prompt neutrino flux. We comment on the range of prompt neutrino fluxes due to theoretical uncertainties.

1 May 2014 in Journal of Cosmology and Astroparticle Physics
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Journal Article
Open access
TGTolga Güver
Tolga Güver
AEArif Emre Erkoca
Arif Emre Erkoca
MRMary Hall Reno
Mary Hall Reno
ISIna Sarcevic
Ina Sarcevic