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Field dependent surface resistance of niobium on copper cavities

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Field dependent surface resistance of niobium on copper cavities. / Junginger, T.
In: Physical Review Special Topics - Accelerators and Beams, Vol. 18, No. 7, 072001, 20.07.2015.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Junginger, T 2015, 'Field dependent surface resistance of niobium on copper cavities', Physical Review Special Topics - Accelerators and Beams, vol. 18, no. 7, 072001. https://doi.org/10.1103/PhysRevSTAB.18.072001

APA

Junginger, T. (2015). Field dependent surface resistance of niobium on copper cavities. Physical Review Special Topics - Accelerators and Beams, 18(7), Article 072001. https://doi.org/10.1103/PhysRevSTAB.18.072001

Vancouver

Junginger T. Field dependent surface resistance of niobium on copper cavities. Physical Review Special Topics - Accelerators and Beams. 2015 Jul 20;18(7):072001. doi: 10.1103/PhysRevSTAB.18.072001

Author

Junginger, T. / Field dependent surface resistance of niobium on copper cavities. In: Physical Review Special Topics - Accelerators and Beams. 2015 ; Vol. 18, No. 7.

Bibtex

@article{82b45676b98a4297ae8c5a82db508f5c,
title = "Field dependent surface resistance of niobium on copper cavities",
abstract = "The surface resistance RS of superconducting cavities prepared by sputter coating a niobium film on a copper substrate increases significantly stronger with the applied rf field compared to cavities of bulk material. A possible cause is that the thermal boundary resistance between the copper substrate and the niobium film induces heating of the inner cavity wall, resulting in a higher RS. Introducing helium gas in the cavity, and measuring its pressure as a function of applied field allowed to conclude that the inner surface of the cavity is heated up by less than 120 mK when RS increases with Eacc by 100nΩ. This is more than one order of magnitude less than what one would expect from global heating. Additionally, the effects of cooldown speed and low temperature baking have been investigated in the framework of these experiments. It is shown that for the current state of the art niobium on copper cavities there is only a detrimental effect of low temperature baking. A fast cooldown results in a lowered RS.",
author = "T. Junginger",
year = "2015",
month = jul,
day = "20",
doi = "10.1103/PhysRevSTAB.18.072001",
language = "English",
volume = "18",
journal = "Physical Review Special Topics - Accelerators and Beams",
issn = "1098-4402",
publisher = "AMER PHYSICAL SOC",
number = "7",

}

RIS

TY - JOUR

T1 - Field dependent surface resistance of niobium on copper cavities

AU - Junginger, T.

PY - 2015/7/20

Y1 - 2015/7/20

N2 - The surface resistance RS of superconducting cavities prepared by sputter coating a niobium film on a copper substrate increases significantly stronger with the applied rf field compared to cavities of bulk material. A possible cause is that the thermal boundary resistance between the copper substrate and the niobium film induces heating of the inner cavity wall, resulting in a higher RS. Introducing helium gas in the cavity, and measuring its pressure as a function of applied field allowed to conclude that the inner surface of the cavity is heated up by less than 120 mK when RS increases with Eacc by 100nΩ. This is more than one order of magnitude less than what one would expect from global heating. Additionally, the effects of cooldown speed and low temperature baking have been investigated in the framework of these experiments. It is shown that for the current state of the art niobium on copper cavities there is only a detrimental effect of low temperature baking. A fast cooldown results in a lowered RS.

AB - The surface resistance RS of superconducting cavities prepared by sputter coating a niobium film on a copper substrate increases significantly stronger with the applied rf field compared to cavities of bulk material. A possible cause is that the thermal boundary resistance between the copper substrate and the niobium film induces heating of the inner cavity wall, resulting in a higher RS. Introducing helium gas in the cavity, and measuring its pressure as a function of applied field allowed to conclude that the inner surface of the cavity is heated up by less than 120 mK when RS increases with Eacc by 100nΩ. This is more than one order of magnitude less than what one would expect from global heating. Additionally, the effects of cooldown speed and low temperature baking have been investigated in the framework of these experiments. It is shown that for the current state of the art niobium on copper cavities there is only a detrimental effect of low temperature baking. A fast cooldown results in a lowered RS.

U2 - 10.1103/PhysRevSTAB.18.072001

DO - 10.1103/PhysRevSTAB.18.072001

M3 - Journal article

AN - SCOPUS:84940399159

VL - 18

JO - Physical Review Special Topics - Accelerators and Beams

JF - Physical Review Special Topics - Accelerators and Beams

SN - 1098-4402

IS - 7

M1 - 072001

ER -