DOE-NP Accelerator R&D PI Meeting 2016 Presentations

Monday, 11/14/2016
DOE Headquarters, Germantown, MD, Room A-410
Meeting Agenda

Time	Dur. (min)	Presentation Title	Speaker	Institution	Topic
8:30 AM	5	Welcome and Introductory Remarks	Gillo, Jehanne	NP	-
8:35 AM	30	NP Accelerator R&D Program Overview	Farkhondeh, Manouchehr	NP	NP Accelerator R&D
9:05 AM	0	Novel Plasmonic Photocathodes for electron-ion colliders	Lukaszew, Rosa	W&M	Photocathode
9:05 AM	45	High Intensity Polarized Electron Gun	Redwine, Robert / Tsentalovich, Evgeni	MIT	High current Pol source /eRHIC
9:50 AM	35	Physics and technology of high-brightness high-power photoinjectors for beam coolers and electron ion colliders	Bazarov, Ivan/ Cultrera, Luca	Cornell	High current Photoinjector
10:25 AM	15	Coffee Break
10:40 AM	45	Coherent Electron Cooling Demonstration Experiment at RHIC	Litvinenko, Vladimir	BNL	CeC - cooling /eRHIC
11:25 AM	40	Development of a Polarized 3He Ion Source for RHIC	Milner, Richard	MIT	Pol ion source /eRHIC
12:05 PM	60	Lunch Break
1:05 PM	45	Critical Accelerator R&D for Achieving High Performance of a Polarized Medium Energy Electron Ion Collider (MEIC/JLEIC Collaboration)	Pilat, Fulvia	TJNAF	MEIC design
1:50 PM	30	Critical Accelerator R&D for Achieving High Performance of a Polarized Medium Energy Electron Ion Collider (MEIC/JLEIC Collaboration)	Sullivan, Michael	SLAC	MEIC design
2:20 PM	35	Critical Accelerator R&D for Achieving High Performance of a Polarized Medium Energy Electron Ion Collider (MEIC/JLEIC Collaboration)	Mustapha, Brahim/ Ostroumov, Peter	ANL	MEIC Design /ion injector
2:55 PM	15	Coffee Break
3:10 PM	35	Design Studies and Prototyping of Superferric Magnets for MEIC ((MEIC Collaboration))	McIntyre, Peter	TAMU	MEIC design
3:45 PM	30	Studies of Conventional and ERL-Based Recirculator Electron Cooling for an Electron Ion Collider	Erdelyi, Bela	NIU	e cooling software /MEIC
4:15 PM	30	500kV DC High Voltage Inverted Gun with Load-Locked CsK2Sb Deposition Chamber	Poelker, Matthew	TJNAF	High current Pol source
4:45 PM		Adjourn

Highlights

View all Highlights

Graph comparing a neutron star with a quark-matter core vs. a nuclear matter core in mass vs. radius. The quark matter core star would have less mass and radius than the nuclear matter core, as stars with smaller radii and more mass are too unstable.

New Clues on Twin Neutron Stars and the Extreme Physics Inside

Scientists have new insights into factors that determine how twin neutron stars—stars with the same mass but different sizes and compositions—can coexist.

Illustration of alpha fusion processes in stars and reactions used on Earth floating above an image of the Earth

Predictive Theory Revises Understanding of Alpha Processes During the Big Bang and in Massive Stars

Theoretical calculations enable more accurate determination of reaction rates for modelling primordial lithium-6 abundance and massive stars’ lifecycle.

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