Model for hot spots and Q-slope behavior in granular niobium thin film superconducting rf cavities

We propose a model to explain power dissipation leading to the formation of hot spots in the inner walls of niobium thin film superconducting rf cavities. The physical mechanism that we explore is due to the constriction of surface electrical current flow at grain interface boundaries. This constric...

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Main Authors: Aymeric Ramiere, Claire Z. Antoine, Jay Amrit
Format: Article
Language:English
Published: American Physical Society 2022-02-01
Series:Physical Review Accelerators and Beams
Online Access:http://doi.org/10.1103/PhysRevAccelBeams.25.022001
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author Aymeric Ramiere
Claire Z. Antoine
Jay Amrit
author_facet Aymeric Ramiere
Claire Z. Antoine
Jay Amrit
author_sort Aymeric Ramiere
collection DOAJ
description We propose a model to explain power dissipation leading to the formation of hot spots in the inner walls of niobium thin film superconducting rf cavities. The physical mechanism that we explore is due to the constriction of surface electrical current flow at grain interface boundaries. This constriction creates an additional electrical contact resistance which induces localized punctual heat dissipation. The temperature at these spots is derived; and the electrical contact resistance is shown to depend on the magnetic field, on the grain contact size over which dissipation occurs, and on other key parameters, including the effective London penetration depth and the frequency. The surface resistance and the quality factors are determined using our model and are shown to be in excellent agreement with experimental data.
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spelling doaj.art-9762cf8861ba4204952f16458dd2ce1f2022-12-21T16:54:09ZengAmerican Physical SocietyPhysical Review Accelerators and Beams2469-98882022-02-0125202200110.1103/PhysRevAccelBeams.25.022001Model for hot spots and Q-slope behavior in granular niobium thin film superconducting rf cavitiesAymeric RamiereClaire Z. AntoineJay AmritWe propose a model to explain power dissipation leading to the formation of hot spots in the inner walls of niobium thin film superconducting rf cavities. The physical mechanism that we explore is due to the constriction of surface electrical current flow at grain interface boundaries. This constriction creates an additional electrical contact resistance which induces localized punctual heat dissipation. The temperature at these spots is derived; and the electrical contact resistance is shown to depend on the magnetic field, on the grain contact size over which dissipation occurs, and on other key parameters, including the effective London penetration depth and the frequency. The surface resistance and the quality factors are determined using our model and are shown to be in excellent agreement with experimental data.http://doi.org/10.1103/PhysRevAccelBeams.25.022001
spellingShingle Aymeric Ramiere
Claire Z. Antoine
Jay Amrit
Model for hot spots and Q-slope behavior in granular niobium thin film superconducting rf cavities
Physical Review Accelerators and Beams
title Model for hot spots and Q-slope behavior in granular niobium thin film superconducting rf cavities
title_full Model for hot spots and Q-slope behavior in granular niobium thin film superconducting rf cavities
title_fullStr Model for hot spots and Q-slope behavior in granular niobium thin film superconducting rf cavities
title_full_unstemmed Model for hot spots and Q-slope behavior in granular niobium thin film superconducting rf cavities
title_short Model for hot spots and Q-slope behavior in granular niobium thin film superconducting rf cavities
title_sort model for hot spots and q slope behavior in granular niobium thin film superconducting rf cavities
url http://doi.org/10.1103/PhysRevAccelBeams.25.022001
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