Journal article 490 views 140 downloads
Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source
New Journal of Physics, Volume: 14, Issue: 10
Swansea University Authors: Helmut Telle, Timothy James
-
PDF | Version of Record
Distributed under the terms of a Creative Commons Attribution Non-Commercial (CC-BY-3.0)
Download (2.38MB)
DOI (Published version): 10.1088/1367-2630/14/10/103046
Abstract
The KArlsruhe TRItium Neutrino (KATRIN) experiment will measure the absolute mass scale of neutrinos with a sensitivity of m<sub>nu</sub> = 200 meV/c<super>2</super> by high-precision spectroscopy close to the tritium beta-decay endpoint at 18.6 keV. Its Windowless Gaseous Tr...
Published in: | New Journal of Physics |
---|---|
ISSN: | 1367-2630 |
Published: |
2012
|
Online Access: |
Check full text
|
URI: | https://cronfa.swan.ac.uk/Record/cronfa14498 |
first_indexed |
2013-07-23T12:12:20Z |
---|---|
last_indexed |
2019-06-13T19:20:39Z |
id |
cronfa14498 |
recordtype |
SURis |
fullrecord |
<?xml version="1.0"?><rfc1807><datestamp>2019-06-13T18:11:33.4651785</datestamp><bib-version>v2</bib-version><id>14498</id><entry>2013-03-27</entry><title>Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source</title><swanseaauthors><author><sid>7f645d598f0afb573309bc5f86ea46fa</sid><firstname>Helmut</firstname><surname>Telle</surname><name>Helmut Telle</name><active>true</active><ethesisStudent>false</ethesisStudent></author><author><sid>8a92e003a0ce92f67bba506d7f03344f</sid><firstname>Timothy</firstname><surname>James</surname><name>Timothy James</name><active>true</active><ethesisStudent>false</ethesisStudent></author></swanseaauthors><date>2013-03-27</date><abstract>The KArlsruhe TRItium Neutrino (KATRIN) experiment will measure the absolute mass scale of neutrinos with a sensitivity of m<sub>nu</sub> = 200 meV/c<super>2</super> by high-precision spectroscopy close to the tritium beta-decay endpoint at 18.6 keV. Its Windowless Gaseous Tritium Source (WGTS) is a beta-decay source of high intensity (10<super>11</super> s−1) and stability, where high-purity molecular tritium at 30 K is circulated in a closed loop with a yearly throughput of 10 kg. To limit systematic effects the column density of the source has to be stabilized at the 10<super>−3</super> level. This requires extensive sensor instrumentation and dedicated control and monitoring systems for parameters such as the beam tube temperature, injection pressure, gas composition and so on. In this paper, we give an overview of these systems including a dedicated laser-Raman system as well as several beta-decay activity monitors. We also report on the results of the WGTS demonstrator and other large-scale test experiments giving proof-of-principle that all parameters relevant to the systematics can be controlled and monitored on the 10<super>−3</super> level or better. As a result of these works, the WGTS systematics can be controlled within stringent margins, enabling the KATRIN experiment to explore the neutrino mass scale with the design sensitivity.</abstract><type>Journal Article</type><journal>New Journal of Physics</journal><volume>14</volume><journalNumber>10</journalNumber><publisher/><issnPrint>1367-2630</issnPrint><keywords/><publishedDay>29</publishedDay><publishedMonth>10</publishedMonth><publishedYear>2012</publishedYear><publishedDate>2012-10-29</publishedDate><doi>10.1088/1367-2630/14/10/103046</doi><url/><notes/><college>COLLEGE NANME</college><CollegeCode>COLLEGE CODE</CollegeCode><institution>Swansea University</institution><apcterm/><lastEdited>2019-06-13T18:11:33.4651785</lastEdited><Created>2013-03-27T12:57:57.0813970</Created><path><level id="1">Faculty of Science and Engineering</level><level id="2">School of Biosciences, Geography and Physics - Physics</level></path><authors><author><firstname>M</firstname><surname>Babutzka</surname><order>1</order></author><author><firstname>M</firstname><surname>Bahr</surname><order>2</order></author><author><firstname>J</firstname><surname>Bonn</surname><order>3</order></author><author><firstname>B</firstname><surname>Bornschein</surname><order>4</order></author><author><firstname>A</firstname><surname>Dieter</surname><order>5</order></author><author><firstname>G</firstname><surname>Drexlin</surname><order>6</order></author><author><firstname>K</firstname><surname>Eitel</surname><order>7</order></author><author><firstname>S</firstname><surname>Fischer</surname><order>8</order></author><author><firstname>F</firstname><surname>Glück</surname><order>9</order></author><author><firstname>S</firstname><surname>Grohmann</surname><order>10</order></author><author><firstname>M</firstname><surname>Hötzel</surname><order>11</order></author><author><firstname>T M</firstname><surname>James</surname><order>12</order></author><author><firstname>W</firstname><surname>Käfer</surname><order>13</order></author><author><firstname>M</firstname><surname>Leber</surname><order>14</order></author><author><firstname>B</firstname><surname>Monreal</surname><order>15</order></author><author><firstname>F</firstname><surname>Priester</surname><order>16</order></author><author><firstname>M</firstname><surname>Röllig</surname><order>17</order></author><author><firstname>M</firstname><surname>Schlösser</surname><order>18</order></author><author><firstname>U</firstname><surname>Schmitt</surname><order>19</order></author><author><firstname>F</firstname><surname>Sharipov</surname><order>20</order></author><author><firstname>M</firstname><surname>Steidl</surname><order>21</order></author><author><firstname>M</firstname><surname>Sturm</surname><order>22</order></author><author><firstname>H H</firstname><surname>Telle</surname><order>23</order></author><author><firstname>N</firstname><surname>Titov</surname><order>24</order></author><author><firstname>Helmut</firstname><surname>Telle</surname><order>25</order></author><author><firstname>Timothy</firstname><surname>James</surname><order>26</order></author></authors><documents><document><filename>0014498-13062019181026.pdf</filename><originalFilename>Babutzka_2012_New_J._Phys._14_103046.pdf</originalFilename><uploaded>2019-06-13T18:10:26.0130000</uploaded><type>Output</type><contentLength>2519783</contentLength><contentType>application/pdf</contentType><version>Version of Record</version><cronfaStatus>true</cronfaStatus><embargoDate>2019-06-13T00:00:00.0000000</embargoDate><documentNotes>Distributed under the terms of a Creative Commons Attribution Non-Commercial (CC-BY-3.0)</documentNotes><copyrightCorrect>true</copyrightCorrect><language>eng</language></document></documents><OutputDurs/></rfc1807> |
spelling |
2019-06-13T18:11:33.4651785 v2 14498 2013-03-27 Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source 7f645d598f0afb573309bc5f86ea46fa Helmut Telle Helmut Telle true false 8a92e003a0ce92f67bba506d7f03344f Timothy James Timothy James true false 2013-03-27 The KArlsruhe TRItium Neutrino (KATRIN) experiment will measure the absolute mass scale of neutrinos with a sensitivity of m<sub>nu</sub> = 200 meV/c<super>2</super> by high-precision spectroscopy close to the tritium beta-decay endpoint at 18.6 keV. Its Windowless Gaseous Tritium Source (WGTS) is a beta-decay source of high intensity (10<super>11</super> s−1) and stability, where high-purity molecular tritium at 30 K is circulated in a closed loop with a yearly throughput of 10 kg. To limit systematic effects the column density of the source has to be stabilized at the 10<super>−3</super> level. This requires extensive sensor instrumentation and dedicated control and monitoring systems for parameters such as the beam tube temperature, injection pressure, gas composition and so on. In this paper, we give an overview of these systems including a dedicated laser-Raman system as well as several beta-decay activity monitors. We also report on the results of the WGTS demonstrator and other large-scale test experiments giving proof-of-principle that all parameters relevant to the systematics can be controlled and monitored on the 10<super>−3</super> level or better. As a result of these works, the WGTS systematics can be controlled within stringent margins, enabling the KATRIN experiment to explore the neutrino mass scale with the design sensitivity. Journal Article New Journal of Physics 14 10 1367-2630 29 10 2012 2012-10-29 10.1088/1367-2630/14/10/103046 COLLEGE NANME COLLEGE CODE Swansea University 2019-06-13T18:11:33.4651785 2013-03-27T12:57:57.0813970 Faculty of Science and Engineering School of Biosciences, Geography and Physics - Physics M Babutzka 1 M Bahr 2 J Bonn 3 B Bornschein 4 A Dieter 5 G Drexlin 6 K Eitel 7 S Fischer 8 F Glück 9 S Grohmann 10 M Hötzel 11 T M James 12 W Käfer 13 M Leber 14 B Monreal 15 F Priester 16 M Röllig 17 M Schlösser 18 U Schmitt 19 F Sharipov 20 M Steidl 21 M Sturm 22 H H Telle 23 N Titov 24 Helmut Telle 25 Timothy James 26 0014498-13062019181026.pdf Babutzka_2012_New_J._Phys._14_103046.pdf 2019-06-13T18:10:26.0130000 Output 2519783 application/pdf Version of Record true 2019-06-13T00:00:00.0000000 Distributed under the terms of a Creative Commons Attribution Non-Commercial (CC-BY-3.0) true eng |
title |
Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source |
spellingShingle |
Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source Helmut Telle Timothy James |
title_short |
Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source |
title_full |
Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source |
title_fullStr |
Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source |
title_full_unstemmed |
Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source |
title_sort |
Monitoring of the operating parameters of the KATRIN Windowless Gaseous Tritium Source |
author_id_str_mv |
7f645d598f0afb573309bc5f86ea46fa 8a92e003a0ce92f67bba506d7f03344f |
author_id_fullname_str_mv |
7f645d598f0afb573309bc5f86ea46fa_***_Helmut Telle 8a92e003a0ce92f67bba506d7f03344f_***_Timothy James |
author |
Helmut Telle Timothy James |
author2 |
M Babutzka M Bahr J Bonn B Bornschein A Dieter G Drexlin K Eitel S Fischer F Glück S Grohmann M Hötzel T M James W Käfer M Leber B Monreal F Priester M Röllig M Schlösser U Schmitt F Sharipov M Steidl M Sturm H H Telle N Titov Helmut Telle Timothy James |
format |
Journal article |
container_title |
New Journal of Physics |
container_volume |
14 |
container_issue |
10 |
publishDate |
2012 |
institution |
Swansea University |
issn |
1367-2630 |
doi_str_mv |
10.1088/1367-2630/14/10/103046 |
college_str |
Faculty of Science and Engineering |
hierarchytype |
|
hierarchy_top_id |
facultyofscienceandengineering |
hierarchy_top_title |
Faculty of Science and Engineering |
hierarchy_parent_id |
facultyofscienceandengineering |
hierarchy_parent_title |
Faculty of Science and Engineering |
department_str |
School of Biosciences, Geography and Physics - Physics{{{_:::_}}}Faculty of Science and Engineering{{{_:::_}}}School of Biosciences, Geography and Physics - Physics |
document_store_str |
1 |
active_str |
0 |
description |
The KArlsruhe TRItium Neutrino (KATRIN) experiment will measure the absolute mass scale of neutrinos with a sensitivity of m<sub>nu</sub> = 200 meV/c<super>2</super> by high-precision spectroscopy close to the tritium beta-decay endpoint at 18.6 keV. Its Windowless Gaseous Tritium Source (WGTS) is a beta-decay source of high intensity (10<super>11</super> s−1) and stability, where high-purity molecular tritium at 30 K is circulated in a closed loop with a yearly throughput of 10 kg. To limit systematic effects the column density of the source has to be stabilized at the 10<super>−3</super> level. This requires extensive sensor instrumentation and dedicated control and monitoring systems for parameters such as the beam tube temperature, injection pressure, gas composition and so on. In this paper, we give an overview of these systems including a dedicated laser-Raman system as well as several beta-decay activity monitors. We also report on the results of the WGTS demonstrator and other large-scale test experiments giving proof-of-principle that all parameters relevant to the systematics can be controlled and monitored on the 10<super>−3</super> level or better. As a result of these works, the WGTS systematics can be controlled within stringent margins, enabling the KATRIN experiment to explore the neutrino mass scale with the design sensitivity. |
published_date |
2012-10-29T06:27:02Z |
_version_ |
1821385762640232448 |
score |
11.123827 |