75 research outputs found

    FACTORS AFFECTING TRANSFER COMMUTER STUDENT SUCCESS: UNDERSTANDING STUDENT SENSE OF CONNECTEDNESS TO CAMPUS AND THE COLLEGIATE SUPPORT NETWORK

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    This paper presents two mixed-methods studies that explored sense of connectedness and the collegiate support network of transfer students at predominantly commuter institutions of higher education. Findings are relevant for student affairs practitioners and administrators at four-year, heavily commuter campuses and community colleges. The first study, a needs assessment, aimed to understand the experience of transfer students at a regional, four-year, commuter university. Interviews with campus administrators identified transfer student retention factors within the themes of student dependent, campus dependent, and jointly dependent. The student survey revealed no statistically significant differences between FTIAC and transfer students on connectedness or perceived support from parents/family, statistically significantly higher levels of perceived peer support among FTIAC students, and statistically significantly higher perceived faculty/staff support among transfer students. The findings, in part, did not align with the extant literature and warranted further inquiry. A follow-up study sought to understand if students’ perceptions of connectedness and support at predominantly commuter campuses might align more with community college students. The follow-up study was conducted at two four-year universities and a community college. Qualitative interviews and focus groups sought to understand how pre-transfer expectations of a four-year university experience compared to actual experiences of transfer students at a predominantly commuter institution. The study also sought to compare the experiences of community college to students at four-year, heavily commuter campuses. The study found no statistically significant differences on connectedness, parent/family support, faculty/staff support, or peer support when comparing community college students to the transfer students. Post hoc analyses evaluated differences based on student living arrangements and involvement yielding insights and implications for practitioners. Reassurance of worth, particularly from faculty/staff and parents/family had the greatest effect on students’ sense of connectedness

    The Long-Baseline Neutrino Experiment: Exploring Fundamental Symmetries of the Universe

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    The preponderance of matter over antimatter in the early Universe, the dynamics of the supernova bursts that produced the heavy elements necessary for life and whether protons eventually decay --- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our Universe, its current state and its eventual fate. The Long-Baseline Neutrino Experiment (LBNE) represents an extensively developed plan for a world-class experiment dedicated to addressing these questions. LBNE is conceived around three central components: (1) a new, high-intensity neutrino source generated from a megawatt-class proton accelerator at Fermi National Accelerator Laboratory, (2) a near neutrino detector just downstream of the source, and (3) a massive liquid argon time-projection chamber deployed as a far detector deep underground at the Sanford Underground Research Facility. This facility, located at the site of the former Homestake Mine in Lead, South Dakota, is approximately 1,300 km from the neutrino source at Fermilab -- a distance (baseline) that delivers optimal sensitivity to neutrino charge-parity symmetry violation and mass ordering effects. This ambitious yet cost-effective design incorporates scalability and flexibility and can accommodate a variety of upgrades and contributions. With its exceptional combination of experimental configuration, technical capabilities, and potential for transformative discoveries, LBNE promises to be a vital facility for the field of particle physics worldwide, providing physicists from around the globe with opportunities to collaborate in a twenty to thirty year program of exciting science. In this document we provide a comprehensive overview of LBNE's scientific objectives, its place in the landscape of neutrino physics worldwide, the technologies it will incorporate and the capabilities it will possess.Comment: Major update of previous version. This is the reference document for LBNE science program and current status. Chapters 1, 3, and 9 provide a comprehensive overview of LBNE's scientific objectives, its place in the landscape of neutrino physics worldwide, the technologies it will incorporate and the capabilities it will possess. 288 pages, 116 figure

    VERITAS: Status and Highlights

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    The VERITAS telescope array has been operating smoothly since 2007, and has detected gamma-ray emission above 100 GeV from 40 astrophysical sources. These include blazars, pulsar wind nebulae, supernova remnants, gamma-ray binary systems, a starburst galaxy, a radio galaxy, the Crab pulsar, and gamma-ray sources whose origin remains unidentified. In 2009, the array was reconfigured, greatly improving the sensitivity. We summarize the current status of the observatory, describe some of the scientific highlights since 2009, and outline plans for the future.Comment: Presented at the 32nd ICRC, Beijing, 201

    First measurement of quasi-elastic Λ\Lambda baryon production in muon anti-neutrino interactions in the MicroBooNE detector

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    We present the first measurement of the cross section of Cabibbo-suppressed Λ\Lambda baryon production, using data collected with the MicroBooNE detector when exposed to the neutrinos from the Main Injector beam at the Fermi National Accelerator Laboratory. The data analyzed correspond to 2.2×10202.2 \times 10^{20} protons on target of neutrino mode running and 4.9×10204.9 \times 10^{20} protons on target of anti-neutrino mode running. An automated selection is combined with hand scanning, with the former identifying five candidate Λ\Lambda production events when the signal was unblinded, consistent with the GENIE prediction of 5.3±1.15.3 \pm 1.1 events. Several scanners were employed, selecting between three and five events, compared with a prediction from a blinded Monte Carlo simulation study of 3.7±1.03.7 \pm 1.0 events. Restricting the phase space to only include Λ\Lambda baryons that decay above MicroBooNE's detection thresholds, we obtain a flux averaged cross section of 2.01.7+2.2×10402.0^{+2.2}_{-1.7} \times 10^{-40} cm2/^2/Ar, where statistical and systematic uncertainties are combined

    Search for heavy neutral leptons in electron-positron and neutral-pion final states with the MicroBooNE detector

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    We present the first search for heavy neutral leptons (HNL) decaying into νe+e\nu e^+e^- or νπ0\nu\pi^0 final states in a liquid-argon time projection chamber using data collected with the MicroBooNE detector. The data were recorded synchronously with the NuMI neutrino beam from Fermilab's Main Injector corresponding to a total exposure of 7.01×10207.01 \times 10^{20} protons on target. We set upper limits at the 90%90\% confidence level on the mixing parameter Uμ42\lvert U_{\mu 4}\rvert^2 in the mass ranges 10mHNL15010\le m_{\rm HNL}\le 150 MeV for the νe+e\nu e^+e^- channel and 150mHNL245150\le m_{\rm HNL}\le 245 MeV for the νπ0\nu\pi^0 channel, assuming Ue42=Uτ42=0\lvert U_{e 4}\rvert^2 = \lvert U_{\tau 4}\rvert^2 = 0. These limits represent the most stringent constraints in the mass range 35<mHNL<17535<m_{\rm HNL}<175 MeV and the first constraints from a direct search for νπ0\nu\pi^0 decays.Comment: Version as accepted by Physical Review Letters, some presentational changes and updated references, no changes to result

    First demonstration of O(1ns)\mathcal{O}(1\,\text{ns}) timing resolution in the MicroBooNE liquid argon time projection chamber

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    MicroBooNE is a neutrino experiment located in the Booster Neutrino Beamline (BNB) at Fermilab, which collected data from 2015 to 2021. MicroBooNE's liquid argon time projection chamber (LArTPC) is accompanied by a photon detection system consisting of 32 photomultiplier tubes used to measure the argon scintillation light and determine the timing of neutrino interactions. Analysis techniques combining light signals and reconstructed tracks are applied to achieve a neutrino interaction time resolution of O(1ns)\mathcal{O}(1\,\text{ns}). The result obtained allows MicroBooNE to access the ns neutrino pulse structure of the BNB for the first time. The timing resolution achieved will enable significant enhancement of cosmic background rejection for all neutrino analyses. Furthermore, the ns timing resolution opens new avenues to search for long-lived-particles such as heavy neutral leptons in MicroBooNE, as well as in future large LArTPC experiments, namely the SBN program and DUNE

    First Measurement of Differential Cross Sections for Muon Neutrino Charged Current Interactions on Argon with a Two-proton Final State in the MicroBooNE Detector

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    We present the first measurement of differential cross sections for charged-current muon neutrino interactions on argon with one muon, two protons, and no pions in the final state. Such interactions leave the target nucleus in a two-particle two-hole state; these states are of great interest, but currently there is limited information about their production in neutrino-nucleus interactions. Detailed investigations of the production of two-particle two-hole states are vital to support upcoming experiments exploring the nature of the neutrino, and the development of the liquid-argon time-projection-chamber has made possible the isolation of such final states. The opening angle between the two protons, the angle between the total proton momentum and the muon, and the total transverse momentum of the final state system are sensitive to the underlying physics processes as embodied in a variety of models. Realistic initial-state momentum distributions are shown to be important in reproducing the data.Comment: To be submitted to PR

    Measurement of triple-differential inclusive muon-neutrino charged-current cross section on argon with the MicroBooNE detector

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    We report the first measurement of the differential cross section d2σ(Eν)/dcos(θμ)dPμd^{2}\sigma (E_{\nu})/ d\cos(\theta_{\mu}) dP_{\mu} for inclusive muon-neutrino charged-current scattering on argon. This measurement utilizes data from 6.4×1020\times10^{20} protons on target of exposure collected using the MicroBooNE liquid argon time projection chamber located along the Fermilab Booster Neutrino Beam with a mean neutrino energy of approximately 0.8~GeV. The mapping from reconstructed kinematics to truth quantities, particularly from reconstructed to true neutrino energy, is validated by comparing the distribution of reconstructed hadronic energy in data to that of the model prediction in different muon scattering angle bins after conditional constraint from the muon momentum distribution in data. The success of this validation gives confidence that the missing energy in the MicroBooNE detector is well-modeled in simulation, enabling the unfolding to a triple-differential measurement over muon momentum, muon scattering angle, and neutrino energy. The unfolded measurement covers an extensive phase space, providing a wealth of information useful for future liquid argon time projection chamber experiments measuring neutrino oscillations. Comparisons against a number of commonly used model predictions are included and their performance in different parts of the available phase-space is discussed

    Differential cross section measurement of charged current νe\nu_{e} interactions without final-state pions in MicroBooNE

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    In this letter we present the first measurements of an exclusive electron neutrino cross section with the MicroBooNE experiment using data from the Booster Neutrino Beamline at Fermilab. These measurements are made for a selection of charged-current electron neutrinos without final-state pions. Differential cross sections are extracted in energy and angle with respect to the beam for the electron and the leading proton. The differential cross section as a function of proton energy is measured using events with protons both above and below the visibility threshold. This is done by including a separate selection of electron neutrino events without reconstructed proton candidates in addition to those with proton candidates. Results are compared to the predictions from several modern generators, and we find the data agrees well with these models. The data shows best agreement, as quantified by pp-value, with the generators that predict a lower overall cross section, such as GENIE v3 and NuWro
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