17–22 May 2026
C.I.D
Europe/Zurich timezone

Solid State Amplifier Source Cooling Flow Configuration at LANSCE

TUP7375
19 May 2026, 16:00
2h
C.I.D

C.I.D

Deauville, France
Poster Presentation MC7.T38: Mechanical design Poster session

Speaker

Taylor Roybal (Los Alamos National Laboratory)

Description

The Los Alamos Neutron Science Center (LANSCE) uses 1.25 MW 805 MHz klystrons to power the coupled cavity linac (CCL) that accelerates H- beam from 100 to 800 MeV. Solid-state amplifiers can replace klystrons while providing the same energy input to the CCL. The solid-state amplifiers will require cooling to ensure the radio frequency (RF) components don’t overheat.
The existing water system used for the klystrons will be used to cool the solid-state amplifiers. There will be four “Colosseums”, that consist of a low-level RF blade, 40 high power RF blades, a 40-way splitter, and a 40-way combiner, that will replace one klystron. We must ensure there is sufficient water flow and pressure available to cool all these components. Interlocks are added to the system to ensure the protection of the RF components.

LA-UR-26-23644

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Authors

Bhavini Singh (Los Alamos National Laboratory) Taylor Roybal (Los Alamos National Laboratory)

Co-authors

Carlos Miera (Los Alamos National Laboratory) Eric Olivas (Los Alamos National Laboratory) Stephen Mano (Los Alamos National Laboratory)

Presentation materials

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