In-Pile 4He Source for UCN Production at the ESS
ESS will be a premier neutron source facility. Unprecedented neutron beam intensities are ensured by spallation reactions of a 5 MW, 2.0 GeV proton beam impinging on a tungsten target equipped with advanced moderators. The work presented here aims at investigating possibilities for installing an ult...
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Main Authors: | , , , , , , |
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Format: | Article |
Language: | English |
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Wiley
2014-01-01
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Series: | Advances in High Energy Physics |
Online Access: | http://dx.doi.org/10.1155/2014/241639 |
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author | Esben Klinkby Konstantin Batkov Ferenc Mezei Eric Pitcher Troels Schönfeldt Alan Takibayev Luca Zanini |
author_facet | Esben Klinkby Konstantin Batkov Ferenc Mezei Eric Pitcher Troels Schönfeldt Alan Takibayev Luca Zanini |
author_sort | Esben Klinkby |
collection | DOAJ |
description | ESS will be a premier neutron source facility. Unprecedented neutron beam intensities are ensured by spallation reactions of a 5 MW, 2.0 GeV proton beam impinging on a tungsten target equipped with advanced moderators. The work presented here aims at investigating possibilities for installing an ultra cold neutron (UCN) source at the ESS. One consequence of using the recently proposed flat moderators is that they take up less space than the moderators originally foreseen and thus leave more freedom to design a UCN source, close to the spallation hotspot. One of the options studied is to place a large 4He UCN source in a through-going tube which penetrates the shielding below the target. First calculations of neutron flux available for UCN production are given, along with heat-load estimates. It is estimated that the flux can give rise to a UCN production at a rate of up to 1.5·108 UCN/s. A production in this range potentially allows for a number of UCN experiments to be carried out at unprecedented precision, including, for example, quantum gravitational spectroscopy with UCNs which rely on high phase-space density. |
format | Article |
id | doaj-art-143ab4bdae5a415a97fe1ace749bc753 |
institution | Kabale University |
issn | 1687-7357 1687-7365 |
language | English |
publishDate | 2014-01-01 |
publisher | Wiley |
record_format | Article |
series | Advances in High Energy Physics |
spelling | doaj-art-143ab4bdae5a415a97fe1ace749bc7532025-02-03T06:07:00ZengWileyAdvances in High Energy Physics1687-73571687-73652014-01-01201410.1155/2014/241639241639In-Pile 4He Source for UCN Production at the ESSEsben Klinkby0Konstantin Batkov1Ferenc Mezei2Eric Pitcher3Troels Schönfeldt4Alan Takibayev5Luca Zanini6European Spallation Source ESS AB, P.O. Box 176, 221 00 Lund, SwedenEuropean Spallation Source ESS AB, P.O. Box 176, 221 00 Lund, SwedenEuropean Spallation Source ESS AB, P.O. Box 176, 221 00 Lund, SwedenEuropean Spallation Source ESS AB, P.O. Box 176, 221 00 Lund, SwedenEuropean Spallation Source ESS AB, P.O. Box 176, 221 00 Lund, SwedenEuropean Spallation Source ESS AB, P.O. Box 176, 221 00 Lund, SwedenEuropean Spallation Source ESS AB, P.O. Box 176, 221 00 Lund, SwedenESS will be a premier neutron source facility. Unprecedented neutron beam intensities are ensured by spallation reactions of a 5 MW, 2.0 GeV proton beam impinging on a tungsten target equipped with advanced moderators. The work presented here aims at investigating possibilities for installing an ultra cold neutron (UCN) source at the ESS. One consequence of using the recently proposed flat moderators is that they take up less space than the moderators originally foreseen and thus leave more freedom to design a UCN source, close to the spallation hotspot. One of the options studied is to place a large 4He UCN source in a through-going tube which penetrates the shielding below the target. First calculations of neutron flux available for UCN production are given, along with heat-load estimates. It is estimated that the flux can give rise to a UCN production at a rate of up to 1.5·108 UCN/s. A production in this range potentially allows for a number of UCN experiments to be carried out at unprecedented precision, including, for example, quantum gravitational spectroscopy with UCNs which rely on high phase-space density.http://dx.doi.org/10.1155/2014/241639 |
spellingShingle | Esben Klinkby Konstantin Batkov Ferenc Mezei Eric Pitcher Troels Schönfeldt Alan Takibayev Luca Zanini In-Pile 4He Source for UCN Production at the ESS Advances in High Energy Physics |
title | In-Pile 4He Source for UCN Production at the ESS |
title_full | In-Pile 4He Source for UCN Production at the ESS |
title_fullStr | In-Pile 4He Source for UCN Production at the ESS |
title_full_unstemmed | In-Pile 4He Source for UCN Production at the ESS |
title_short | In-Pile 4He Source for UCN Production at the ESS |
title_sort | in pile 4he source for ucn production at the ess |
url | http://dx.doi.org/10.1155/2014/241639 |
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