ΔE–E Telescope for the Detection of Charged Particles Based on a Si Detector and a SiPM Array with Scintillation Crystals
The characteristics of a Δ E–E telescope, which is planned to be used in the experimental setup focused on few-nucleon reactions, are studied. The required parameters of the Δ E–E telescope were determined on the basis of the numerical modeling of probable reactions. The telescope comprises a Δ E de...
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Veröffentlicht in: | Physics of atomic nuclei 2018-12, Vol.81 (10), p.1471-1476 |
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creator | Mitcuk, V. V. Mordovskoy, M. V. |
description | The characteristics of a Δ
E–E
telescope, which is planned to be used in the experimental setup focused on few-nucleon reactions, are studied. The required parameters of the Δ
E–E
telescope were determined on the basis of the numerical modeling of probable reactions. The telescope comprises a Δ
E
detector, which is a totally depleted surface-barrier silicon detector with a diameter of 8 mm and a thickness of ~24 μm, and an
E
detector based on LFS-8 crystals and a 16-element SiPM ARRAYC-30035-16P-PCB array. The telescope is designed, in particular, for coincidence detection of two charged particles emitted at close angles. This is made possible by the matrix structure of the
E
detector. The time resolution of the Δ
E
detector and the time and amplitude resolutions of all cells of the
E
detector were determined. The standard method of detection of two γ quanta from the beta decay of
22
Na was used to measure the time resolution. Time coincidences of signals from the Δ
E
detector and a neutron detector based on a liquid scintillator (EJ-301) with its FWHM no worse than 1 ns were obtained. Similar measurements for the
E
-detector cells revealed time (less than 0.6 ns) and amplitude (~15% at an energy of ~1 MeV) resolutions that satisfy the experimental requirements for particle sorting and determination of their energy. The intrinsic background of the
E
detector, which arises from the radioactivity of LFS-8 crystals, was measured. The relative number of events corresponding to simultaneous triggering of two or more
E
-detector cells irradiated with α particles from a
226
Ra source was also determined. This value may help estimate the number of random coincidences in a real experiment. |
doi_str_mv | 10.1134/S1063778818100101 |
format | Article |
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E–E
telescope, which is planned to be used in the experimental setup focused on few-nucleon reactions, are studied. The required parameters of the Δ
E–E
telescope were determined on the basis of the numerical modeling of probable reactions. The telescope comprises a Δ
E
detector, which is a totally depleted surface-barrier silicon detector with a diameter of 8 mm and a thickness of ~24 μm, and an
E
detector based on LFS-8 crystals and a 16-element SiPM ARRAYC-30035-16P-PCB array. The telescope is designed, in particular, for coincidence detection of two charged particles emitted at close angles. This is made possible by the matrix structure of the
E
detector. The time resolution of the Δ
E
detector and the time and amplitude resolutions of all cells of the
E
detector were determined. The standard method of detection of two γ quanta from the beta decay of
22
Na was used to measure the time resolution. Time coincidences of signals from the Δ
E
detector and a neutron detector based on a liquid scintillator (EJ-301) with its FWHM no worse than 1 ns were obtained. Similar measurements for the
E
-detector cells revealed time (less than 0.6 ns) and amplitude (~15% at an energy of ~1 MeV) resolutions that satisfy the experimental requirements for particle sorting and determination of their energy. The intrinsic background of the
E
detector, which arises from the radioactivity of LFS-8 crystals, was measured. The relative number of events corresponding to simultaneous triggering of two or more
E
-detector cells irradiated with α particles from a
226
Ra source was also determined. This value may help estimate the number of random coincidences in a real experiment.</description><identifier>ISSN: 1063-7788</identifier><identifier>EISSN: 1562-692X</identifier><identifier>DOI: 10.1134/S1063778818100101</identifier><language>eng</language><publisher>Moscow: Pleiades Publishing</publisher><subject>Alpha particles ; Alpha rays ; Amplitudes ; Background radiation ; Beta decay ; Charged particles ; Crystals ; Engineering Design of Nuclear Physics Equipment ; Mathematical models ; Neutron counters ; Particle and Nuclear Physics ; Particle sorting ; Physics ; Physics and Astronomy ; Radioactivity ; Radium 226 ; Scintillation counters ; Sensors ; Silicon ; Sodium 22 ; Telescopes</subject><ispartof>Physics of atomic nuclei, 2018-12, Vol.81 (10), p.1471-1476</ispartof><rights>Pleiades Publishing, Ltd. 2018</rights><rights>Copyright Springer Nature B.V. 2018</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c316t-1cc2b47c04551b41740802a27b8016d26d6c3fc8625777b813b187fe4a8b97343</citedby><cites>FETCH-LOGICAL-c316t-1cc2b47c04551b41740802a27b8016d26d6c3fc8625777b813b187fe4a8b97343</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1134/S1063778818100101$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1134/S1063778818100101$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,778,782,27907,27908,41471,42540,51302</link.rule.ids></links><search><creatorcontrib>Mitcuk, V. V.</creatorcontrib><creatorcontrib>Mordovskoy, M. V.</creatorcontrib><title>ΔE–E Telescope for the Detection of Charged Particles Based on a Si Detector and a SiPM Array with Scintillation Crystals</title><title>Physics of atomic nuclei</title><addtitle>Phys. Atom. Nuclei</addtitle><description>The characteristics of a Δ
E–E
telescope, which is planned to be used in the experimental setup focused on few-nucleon reactions, are studied. The required parameters of the Δ
E–E
telescope were determined on the basis of the numerical modeling of probable reactions. The telescope comprises a Δ
E
detector, which is a totally depleted surface-barrier silicon detector with a diameter of 8 mm and a thickness of ~24 μm, and an
E
detector based on LFS-8 crystals and a 16-element SiPM ARRAYC-30035-16P-PCB array. The telescope is designed, in particular, for coincidence detection of two charged particles emitted at close angles. This is made possible by the matrix structure of the
E
detector. The time resolution of the Δ
E
detector and the time and amplitude resolutions of all cells of the
E
detector were determined. The standard method of detection of two γ quanta from the beta decay of
22
Na was used to measure the time resolution. Time coincidences of signals from the Δ
E
detector and a neutron detector based on a liquid scintillator (EJ-301) with its FWHM no worse than 1 ns were obtained. Similar measurements for the
E
-detector cells revealed time (less than 0.6 ns) and amplitude (~15% at an energy of ~1 MeV) resolutions that satisfy the experimental requirements for particle sorting and determination of their energy. The intrinsic background of the
E
detector, which arises from the radioactivity of LFS-8 crystals, was measured. The relative number of events corresponding to simultaneous triggering of two or more
E
-detector cells irradiated with α particles from a
226
Ra source was also determined. This value may help estimate the number of random coincidences in a real experiment.</description><subject>Alpha particles</subject><subject>Alpha rays</subject><subject>Amplitudes</subject><subject>Background radiation</subject><subject>Beta decay</subject><subject>Charged particles</subject><subject>Crystals</subject><subject>Engineering Design of Nuclear Physics Equipment</subject><subject>Mathematical models</subject><subject>Neutron counters</subject><subject>Particle and Nuclear Physics</subject><subject>Particle sorting</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Radioactivity</subject><subject>Radium 226</subject><subject>Scintillation counters</subject><subject>Sensors</subject><subject>Silicon</subject><subject>Sodium 22</subject><subject>Telescopes</subject><issn>1063-7788</issn><issn>1562-692X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp1kMtKAzEUhoMoWKsP4C7gejQnM5OkyzrWC1QstIK7IZPJtCnjTE1SpODCd9Dn8iF8EtMLuBBX5_J__3_gIHQK5BwgTi7GQFjMuRAggBAgsIc6kDIasR592g99kKO1foiOnJsHBERKOujt63Pw_f4xwBNda6fahcZVa7GfaXylvVbetA1uK5zNpJ3qEo-k9UYFFF9KF-agSjw2Ozg4ZVNuNqN73LdWrvCr8TM8Vqbxpq7lJi-zK-dl7Y7RQRWKPtnVLnq8Hkyy22j4cHOX9YeRioH5CJSiRcIVSdIUigR4QgShkvJCEGAlZSVTcaUEoynnYQlxAYJXOpGi6PE4ibvobJu7sO3LUjufz9ulbcLJnIIQbJ3LAwVbStnWOaurfGHNs7SrHEi-fnL-58nBQ7ceF9hmqu1v8v-mHx2Zfdo</recordid><startdate>20181201</startdate><enddate>20181201</enddate><creator>Mitcuk, V. V.</creator><creator>Mordovskoy, M. V.</creator><general>Pleiades Publishing</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope></search><sort><creationdate>20181201</creationdate><title>ΔE–E Telescope for the Detection of Charged Particles Based on a Si Detector and a SiPM Array with Scintillation Crystals</title><author>Mitcuk, V. V. ; Mordovskoy, M. V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c316t-1cc2b47c04551b41740802a27b8016d26d6c3fc8625777b813b187fe4a8b97343</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Alpha particles</topic><topic>Alpha rays</topic><topic>Amplitudes</topic><topic>Background radiation</topic><topic>Beta decay</topic><topic>Charged particles</topic><topic>Crystals</topic><topic>Engineering Design of Nuclear Physics Equipment</topic><topic>Mathematical models</topic><topic>Neutron counters</topic><topic>Particle and Nuclear Physics</topic><topic>Particle sorting</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Radioactivity</topic><topic>Radium 226</topic><topic>Scintillation counters</topic><topic>Sensors</topic><topic>Silicon</topic><topic>Sodium 22</topic><topic>Telescopes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Mitcuk, V. V.</creatorcontrib><creatorcontrib>Mordovskoy, M. V.</creatorcontrib><collection>CrossRef</collection><jtitle>Physics of atomic nuclei</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mitcuk, V. V.</au><au>Mordovskoy, M. V.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>ΔE–E Telescope for the Detection of Charged Particles Based on a Si Detector and a SiPM Array with Scintillation Crystals</atitle><jtitle>Physics of atomic nuclei</jtitle><stitle>Phys. Atom. Nuclei</stitle><date>2018-12-01</date><risdate>2018</risdate><volume>81</volume><issue>10</issue><spage>1471</spage><epage>1476</epage><pages>1471-1476</pages><issn>1063-7788</issn><eissn>1562-692X</eissn><abstract>The characteristics of a Δ
E–E
telescope, which is planned to be used in the experimental setup focused on few-nucleon reactions, are studied. The required parameters of the Δ
E–E
telescope were determined on the basis of the numerical modeling of probable reactions. The telescope comprises a Δ
E
detector, which is a totally depleted surface-barrier silicon detector with a diameter of 8 mm and a thickness of ~24 μm, and an
E
detector based on LFS-8 crystals and a 16-element SiPM ARRAYC-30035-16P-PCB array. The telescope is designed, in particular, for coincidence detection of two charged particles emitted at close angles. This is made possible by the matrix structure of the
E
detector. The time resolution of the Δ
E
detector and the time and amplitude resolutions of all cells of the
E
detector were determined. The standard method of detection of two γ quanta from the beta decay of
22
Na was used to measure the time resolution. Time coincidences of signals from the Δ
E
detector and a neutron detector based on a liquid scintillator (EJ-301) with its FWHM no worse than 1 ns were obtained. Similar measurements for the
E
-detector cells revealed time (less than 0.6 ns) and amplitude (~15% at an energy of ~1 MeV) resolutions that satisfy the experimental requirements for particle sorting and determination of their energy. The intrinsic background of the
E
detector, which arises from the radioactivity of LFS-8 crystals, was measured. The relative number of events corresponding to simultaneous triggering of two or more
E
-detector cells irradiated with α particles from a
226
Ra source was also determined. This value may help estimate the number of random coincidences in a real experiment.</abstract><cop>Moscow</cop><pub>Pleiades Publishing</pub><doi>10.1134/S1063778818100101</doi><tpages>6</tpages></addata></record> |
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language | eng |
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source | Springer Nature - Complete Springer Journals |
subjects | Alpha particles Alpha rays Amplitudes Background radiation Beta decay Charged particles Crystals Engineering Design of Nuclear Physics Equipment Mathematical models Neutron counters Particle and Nuclear Physics Particle sorting Physics Physics and Astronomy Radioactivity Radium 226 Scintillation counters Sensors Silicon Sodium 22 Telescopes |
title | ΔE–E Telescope for the Detection of Charged Particles Based on a Si Detector and a SiPM Array with Scintillation Crystals |
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