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Liu, W. ; Wang, Y. ; Guo, B. ; Tang, X. ; Zeng, S. (Ed.)Sensitivity studies have shown that the 15 O(α, γ) 19 Ne reaction is the most important reaction rate uncertainty affecting the shape of light curves from Type I X-ray bursts. This reaction is dominated by the 4.03 MeV resonance in 19 Ne. Previous measurements by our group have shown that this state is populated in the decay sequence of 20 Mg. A single 20 Mg(βp α) 15 O event through the key 15 O(α, γ) 19 Ne resonance yields a characteristic signature: the emission of a proton and alpha particle. To achieve the granularity necessary for the identification of thismore »Free, publicly-accessible full text available January 1, 2023
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Liu, W. ; Wang, Y. ; Guo, B. ; Tang, X. ; Zeng, S. (Ed.)15 O( α , γ ) 19 Ne is regarded as one of the most important thermonuclear reactions in type I X-ray bursts. For studying the properties of the key resonance in this reaction using β decay, the existing Proton Detector component of the Gaseous Detector with Germanium Tagging (GADGET) assembly is being upgraded to operate as a time projection chamber (TPC) at FRIB. This upgrade includes the associated hardware as well as software and this paper mainly focusses on the software upgrade. The full detector set up is simulated using the ATTPCROOTv 2 data analysis framework for 20 Mgmore »Free, publicly-accessible full text available January 1, 2023
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This interdisciplinary, inter-institutional research initiation project is motivated by the need to develop practical strategies for broadening the participation of African American students in engineering. The central objective of the project is to conduct a comparative study of the factors affecting the success and pathways to engineering careers of African American students at a Predominantly White Institution (PWI), the University of Toledo, and a Historically Black University (Alabama Agricultural and Mechanical University). Through this research we hope to gain insight into the factors affecting the social and academic well-being of students at PWIs and HBCUs from a psychological and anthropologicalmore »
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Low enrollment, retention, and graduation rates of African American engineering students in the United States are a cause for concern [1]. Consequently, over the last decade there has been an upsurge of research identifying factors that have contributed to the problems encountered by African American students in higher education institutions in general, and in STEM fields in particular [2, 3]. The key factors identified as contributing to the attrition of minority African American students include perceptions of racism on campus, internalization of stereotypes, feelings of alienation and rejection, and inadequate support systems [4, 5]. In this context, considerations of institutionalmore »
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Abstract We search for signatures of gravitational lensing in the gravitational-wave signals from compact binary coalescences detected by Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) and Advanced Virgo during O3a, the first half of their third observing run. We study: (1) the expected rate of lensing at current detector sensitivity and the implications of a non-observation of strong lensing or a stochastic gravitational-wave background on the merger-rate density at high redshift; (2) how the interpretation of individual high-mass events would change if they were found to be lensed; (3) the possibility of multiple images due to strong lensing by galaxies ormore »Free, publicly-accessible full text available December 1, 2022
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Abstract We present a search for continuous gravitational-wave emission due to r-modes in the pulsar PSR J0537–6910 using data from the LIGO–Virgo Collaboration observing run O3. PSR J0537–6910 is a young energetic X-ray pulsar and is the most frequent glitcher known. The inter-glitch braking index of the pulsar suggests that gravitational-wave emission due to r-mode oscillations may play an important role in the spin evolution of this pulsar. Theoretical models confirm this possibility and predict emission at a level that can be probed by ground-based detectors. In order to explore this scenario, we search for r-mode emission in the epochsmore »Free, publicly-accessible full text available November 1, 2022
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Free, publicly-accessible full text available November 1, 2022