Preprint Open Access

CYGNO Conceptual Design Report

Baracchini E.; Bedogni R.; Bellini F.; Benussi L.; Bianco S.; Bignell L.; Caponero M.; Cavoto G.; Di Marco E.; Eldridge C.; Ezeribe A.; Gargan R.; Gamble T.; Gregorio G.; Lane G.; Loomba D.; Lynch W.; Maccarrone G.; Marafini M.; Mazzitelli G.; Messina A.; Mills A.; Miuchi K.; Petrucci F.; Piccolo D.; Pinci D.; Phan N.; Renga F.; Saviano G.; Spooner N.; Thorpe T.; Tommassini S.; Vahsen S.

DataCite XML Export

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  <identifier identifierType="DOI">10.15161/oar.it/73356</identifier>
  <creators>
    <creator>
      <creatorName>Baracchini E.</creatorName>
      <affiliation>Gran Sasso Science Institute L'Aquila, I-67100, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Bedogni R.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Bellini F.</creatorName>
      <affiliation>Dipartimento di Fisica Sapienza Università di Roma, I-00185, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Benussi L.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Bianco S.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Bignell L.</creatorName>
      <affiliation>Australian National University, Canberra ACT 0200, Australia</affiliation>
    </creator>
    <creator>
      <creatorName>Caponero M.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-000, ENEA, Frascati, Frascati (RM), I-00044, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Cavoto G.</creatorName>
      <affiliation>ENEA, Frascati, Frascati (RM), I-00044, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Di Marco E.</creatorName>
      <affiliation>Dipartimento di Fisica Sapienza Università di Roma, I-00185, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Eldridge C.</creatorName>
      <affiliation>University of Sheffield, S10 2TN, UK</affiliation>
    </creator>
    <creator>
      <creatorName>Ezeribe A.</creatorName>
      <affiliation>University of Sheffield, S10 2TN, UK</affiliation>
    </creator>
    <creator>
      <creatorName>Gargan R.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Gamble T.</creatorName>
      <affiliation>University of Sheffield, S10 2TN, UK</affiliation>
    </creator>
    <creator>
      <creatorName>Gregorio G.</creatorName>
      <affiliation>University of Sheffield, S10 2TN, UK</affiliation>
    </creator>
    <creator>
      <creatorName>Lane G.</creatorName>
      <affiliation>Australian National University, Canberra ACT 0200, Australia</affiliation>
    </creator>
    <creator>
      <creatorName>Loomba D.</creatorName>
      <affiliation>University of New Mexico, Albuquerque, NM 87131, USA</affiliation>
    </creator>
    <creator>
      <creatorName>Lynch W.</creatorName>
      <affiliation>University of Sheffield, S10 2TN, UK</affiliation>
    </creator>
    <creator>
      <creatorName>Maccarrone G.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Marafini M.</creatorName>
      <affiliation>Museo Storico della Fisica e Centro Studi e Ricerche "Enrico Fermi" Piazza del Viminale 1, Roma, I-00184, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Mazzitelli G.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Messina A.</creatorName>
      <affiliation>Dipartimento di Fisica Sapienza Università di Roma, I-00185, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Mills A.</creatorName>
      <affiliation>University of New Mexico, Albuquerque, NM 87131, USA</affiliation>
    </creator>
    <creator>
      <creatorName>Miuchi K.</creatorName>
      <affiliation>Kobe University, Hyogo Prefecture 657-0013, Japan</affiliation>
    </creator>
    <creator>
      <creatorName>Petrucci F.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Sezione di Roma TRE, I-00154, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Piccolo D.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Pinci D.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Sezione di Roma, I-00185, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Phan N.</creatorName>
      <affiliation>University of New Mexico, Albuquerque, NM 87131, USA</affiliation>
    </creator>
    <creator>
      <creatorName>Renga F.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Sezione di Roma, I-00185, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Saviano G.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy, Dipartimento di Ingegneria Chimica, Materiali e Ambiente Sapienza Università di Roma, I-00185, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Spooner N.</creatorName>
      <affiliation>University of Sheffield, S10 2TN, UK</affiliation>
    </creator>
    <creator>
      <creatorName>Thorpe T.</creatorName>
      <affiliation>University of Hawaii, Honolulu, U</affiliation>
    </creator>
    <creator>
      <creatorName>Tommassini S.</creatorName>
      <affiliation>Istituto Nazionale di Fisica Nucleare Laboratori Nazionali di Frascati, I-00040, Italy</affiliation>
    </creator>
    <creator>
      <creatorName>Vahsen S.</creatorName>
      <affiliation>University of Hawaii, Honolulu, US</affiliation>
    </creator>
  </creators>
  <titles>
    <title>CYGNO Conceptual Design Report</title>
  </titles>
  <publisher>INFN Open Access Repository</publisher>
  <publicationYear>2019</publicationYear>
  <subjects>
    <subject>CYGNO</subject>
    <subject>Project</subject>
    <subject>Nota interna</subject>
    <subject>Sezione Roma 1</subject>
    <subject>INFN-19-06/ROMA1</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2019-03-20</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Preprint</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://www.openaccessrepository.it/record/73356</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.15161/oar.it/73355</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://www.openaccessrepository.it/communities/cygno_it</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://www.openaccessrepository.it/communities/infn</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/">Creative Commons Attribution 4.0</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;The conceptual design of the experiment named CYGNO (a CYGNUs module withOptical readout) is presented here. CYGNO aims to make significant advances in the technology of single phase gas-only time projection chambers (TPC) for the specific application of rare scattering events detection. In particular it will focus on a read-out technique based on the GEM amplification of the ionisation and on the visible light collection with a sub-mm position resolution by sCMOS camera. This type of readout - in conjunction with a fast light detection - will allow to reconstruct three dimensional (3D) images of the recoiling particles with high precision, offering new ways to distinguish the electron and nuclear recoils. The recoil direction resolution is also being investigated as a further tool to reject neutral background in the detection of Galactic Dark Matter (DM) particles. The final goal is to build and operate a high resolution gas TPC detector at the 50 kg scale for the directional search of a DM signal, in underground Laboratori Nazionali del Gran Sasso. In order to achieve this very demanding goal, we are going to develop firstly a 1 m&lt;sup&gt;3&lt;/sup&gt; volume, 1 kg mass detector based on these concepts, to assess on a real underground experiment the design performances and capabilities of our approach, while at the same time testing innovative techniques and methods to reach the 50 kg scale. This project is part of the world-wide effort of the CYGNUS collaboration to define an optimal DM detection scheme sensitive to DM direction, towards a one-ton gas TPC nuclear recoils Sobservatory.&lt;/p&gt;</description>
  </descriptions>
</resource>
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Publication date:
March 20, 2019
DOI:
10.15161/oar.it/73356

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CYGNO Project Nota interna Sezione Roma 1 INFN-19-06/ROMA1
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