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  1. Since 2015, Cyclotron Road fellows have advanced 74 companies, raised over $1.85 billion in follow-on funding, hired over 1400 employees, and introduced new products across industries, including energy, agriculture, and manufacturing. Learn more about today’s innovators tackling the challenges of tomorrow.

  2. Cyclotron Road provides unencumbered access and connections to collaborations with more than 4,000 scientists and faculty — including many Nobel Prize winners and more than 100 members of the National Academies — across Berkeley Lab and UC Berkeley.

  3. Cyclotron Road is a fellowship program for technology innovators at Lawrence Berkeley National Laboratory, or Berkeley Lab. Cyclotron Road supports entrepreneurial scientists as they advance their own technology projects that have the promise of significant global impact.

  4. 29 de mar. de 2024 · 1 Cyclotron Road, Berkeley, CA 94720, United States. Search for other works by this author on: Oxford Academic. Google Scholar. Joshua N Adkins, ... The Ohio State University, 1958 Neil Ave, Columbus, OH, 43210, United States. Search for other works by this author on: Oxford Academic.

  5. Hace 2 días · CMB lensing and Ly. 𝛼. \alpha. italic_α. forest cross bispectrum from DESI’s first-year quasar sample. Naim Göksel Karaçaylı\orcidlink0000-0001-7336-8912 karacayli.1@osu.edu Center for Cosmology and AstroParticle Physics, The Ohio State University, 191 West Woodruff Avenue, Columbus, OH 43210, USA Department of Astronomy, The Ohio ...

  6. These results suggest that although environmental conditions shape metabolism in common ways regardless of infection, virocell-specific strategies exist to support viral replication during nutrient limitation, and a framework now exists for identifying metabolic strategies of nutrient-limited virocells in nature.

  7. The high signal-to-noise of the CMB lensing cross-correlations enables several powerful consistency tests of these results, including com-parisons with constraints derived from cross-correlations only, and comparisons designed to test the robustness of the galaxy lensing and clustering measurements from DES.