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This paper examines the initial beliefs held by elementary educators (n=11) and their students about teaching and learning quantum concepts at the elementary level. All teachers were participants in a grant-funded project focused on developing teachers’ quantum content knowledge and creating curricular resources to use in elementary classrooms. Although elementary teachers had limited knowledge of quantum at the beginning of the project, they expressed excitement and a belief that learning quantum would create future possibilities for their students. 

Quantum science and computing represent a vital intersection between science and technology, gaining increasing importance in modern society. There is a pressing need to incorporate these concepts into the K-12 curriculum, equipping new generations with the tools to navigate and thrive in an evolving technological landscape. This study explores the professional learning of K-12 teachers (n = 49) related to quantum concepts and pedagogy. We used open-ended surveys, field notes, workshop artifacts, and interviews to examine teachers’ perceptions of quantum and how they made connections between quantum and their curriculum. Our data reveal that most teachers were excited and interested in teaching quantum but were aware of potential barriers and concerns that might get in the way of teaching quantum. We found that teachers readily identified connections to math and science in their curriculum, but only a few made connections to computing. Enthusiasm for teaching quantum concepts was found in both elementary and secondary educators, suggesting a widespread recognition of its importance in preparing students for a future where quantum technology is a fundamental aspect of their lives and careers. 

The percentage of women receiving bachelor’s degrees in physics (25%) in the U.S. lags well behind that of men, and women leave the major at higher rates. Achieving equity in physics will mean that women stay in physics at the same rates as men, but this will require changes in the culture and support structures. A strong sense of belonging can lead to higher retention rates so interventions meant to increase dimensions of physics identity (interest, recognition, performance, and competence) may increase persistence overall and increase women’s retention differentially. We describe our model in which mentorship, an understanding of career options (career conceptualization), and leadership are inputs into the development of these dimensions of physics identity. This paper includes preliminary results from a qualitative study that aims to better understand how career conceptualization, leadership, and mentorship contribute to the development of physics identity and belonging. We report results from a survey of 15 undergraduate physics students which was followed up by interviews with 5 of those students. The students were from 2 institutions: a small private liberal arts college in the midwest region of the U.S. and a large public university in the southeast region of the U.S. classified as a Hispanic-serving institution (HSI). With respect to mentorship, consistent with the existing literature, we found that it could provide critical support for students’ engagement in the physics community. Leadership experiences have not previously been positioned as an important input into identity, yet we found that they helped women in physics feel more confident, contributing to their recognition of themselves as physics people. While the data on how career conceptualization contributed to the building of identity is limited, there are some connections to recognition and competence, and it will be an interesting avenue of future exploration. Published by the American Physical Society2024 

Background:Programmes that provide scientists and engineers with support to engage in public policy have proliferated in the United States, with many opportunities available for training, networking and placements within government and government-facing organisations. This trend suggests that an evolution may be occurring at the science–policy interface. However, there is little extant data on the structure, aims and impacts of these programmes. Aims and objectives:This study maps the current landscape of US programmes seeking to train researchers at all career stages to engage in policy. We focus on Virginia, a state with a substantial number and diversity of programmes, to assess: (1) how they conceptualise their audiences, activities and impacts; and (2) which roles in policy and types of evidence use they address. Methods:We developed a database of US policy programmes (n=174) and conducted a case study of those in Virginia through surveys and interviews with their leaders (n=12). Findings:The majority (57%) of science policy programmes are state-based. These programmes include student organisations, government placements and fellowships, and academic certificates, degrees, and other trainings. While these reflect diverse models for how to engage researchers in policy, Virginia programme leaders across these categories similarly conceived long-term impacts, audiences and activities, researcher roles in policy, and types of decision-maker evidence use. And they perceived limited ability to implement evidence-based approaches within their programmes. Discussion and conclusion:Building additional programmatic capacity – through shared learning and partnerships – could lend support to this emerging trend in science policy with implications for US research and governance. 

Low-mass galaxies are thought to play a large role in reionizing the Universe at redshifts, z > 6. However, due to limited UV data on low-mass galaxies, the models used to estimate the escape of radiation are poorly constrained. Using theoretical models of radiation transport in dusty galaxies with clumpy gas media, we translate measurements of the UV slopes of a sample of low-mass low-z KISSR galaxies to their escape fraction values in Ly-alpha radiation, fesc (LyA), and in the Ly-continuum, fesc (LyC). These low-mass starforming systems have potentially steep UV slopes, and could provide a much-needed relation between easily measured spectral properties such as UV slope or LyA line properties, and the escape of LyA/LyC radiation. Such a relation could advance studies of primordial star clusters and the underlying physical conditions characterizing early galaxies, one of the target observation goals of the soon to-be-launched James Webb Space Telescope. This work was supported by the University of San Francisco Faculty Development Fund, and NSF grant AST-1637339. We thank the Aspen Center for Physics, where some of this work was conducted, and which is supported by National Science Foundation grant PHY-1607611.