Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Guilherme Sebastiao Pinheiro Lopes"'
Autor:
Fernando Domingues Amaro, Rita Antonietti, Elisabetta Baracchini, Luigi Benussi, Stefano Bianco, Francesco Borra, Cesidio Capoccia, Michele Caponero, Danilo Santos Cardoso, Gianluca Cavoto, Igor Abritta Costa, Emiliano Dané, Giorgio Dho, Flaminia Di Giambattista, Emanuele Di Marco, Giulia D’Imperio, Joaquim Marques Ferreira dos Santos, Giovanni Grilli di Cortona, Francesco Iacoangeli, Ernesto Kemp, Herman Pessoa Lima Júnior, Guilherme Sebastiao Pinheiro Lopes, Amaro da Silva Lopes Júnior, Giovanni Maccarrone, Rui Daniel Passos Mano, Robert Renz Marcelo Gregorio, David José Gaspar Marques, Giovanni Mazzitelli, Alasdair Gregor McLean, Pietro Meloni, Andrea Messina, Cristina Maria Bernardes Monteiro, Rafael Antunes Nobrega, Igor Fonseca Pains, Emiliano Paoletti, Luciano Passamonti, Sandro Pelosi, Fabrizio Petrucci, Stefano Piacentini, Davide Piccolo, Daniele Pierluigi, Davide Pinci, Atul Prajapati, Francesco Renga, Rita Cruz Roque, Filippo Rosatelli, Alessandro Russo, Giovanna Saviano, Neil John Curwen Spooner, Roberto Tesauro, Sandro Tomassini, Samuele Torelli, Donatella Tozzi
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 83, Iss 10, Pp 1-23 (2023)
Abstract The nature of dark matter is still unknown and an experimental program to look for dark matter particles in our Galaxy should extend its sensitivity to light particles in the GeV mass range and exploit the directional information of the DM p
Externí odkaz:
https://doaj.org/article/7eb270706d154696b0109ed07eab3e5b
Autor:
Fernando Domingues Amaro, Elisabetta Baracchini, Luigi Benussi, Stefano Bianco, Cesidio Capoccia, Michele Caponero, Danilo Santos Cardoso, Gianluca Cavoto, André Cortez, Igor Abritta Costa, Rita Joanna da Cruz Roque, Emiliano Dané, Giorgio Dho, Flaminia Di Giambattista, Emanuele Di Marco, Giovanni Grilli di Cortona, Giulia D’Imperio, Francesco Iacoangeli, Herman Pessoa Lima Júnior, Guilherme Sebastiao Pinheiro Lopes, Amaro da Silva Lopes Júnior, Giovanni Maccarrone, Rui Daniel Passos Mano, Michela Marafini, Robert Renz Marcelo Gregorio, David José Gaspar Marques, Giovanni Mazzitelli, Alasdair Gregor McLean, Andrea Messina, Cristina Maria Bernardes Monteiro, Rafael Antunes Nobrega, Igor Fonseca Pains, Emiliano Paoletti, Luciano Passamonti, Sandro Pelosi, Fabrizio Petrucci, Stefano Piacentini, Davide Piccolo, Daniele Pierluigi, Davide Pinci, Atul Prajapati, Francesco Renga, Filippo Rosatelli, Alessandro Russo, Joaquim Marques Ferreira dos Santos, Giovanna Saviano, Neil John Curwen Spooner, Roberto Tesauro, Sandro Tomassini, Samuele Torelli
Publikováno v:
Instruments, Vol 6, Iss 1, p 6 (2022)
The search for a novel technology able to detect and reconstruct nuclear and electron recoil events with the energy of a few keV has become more and more important now that large regions of high-mass dark matter (DM) candidates have been excluded. Mo
Externí odkaz:
https://doaj.org/article/74f041d5ac714048a0faffb1c9fbaafb
Autor:
Fernando Domingues Amaro, Elisabetta Baracchini, Luigi Benussi, Stefano Bianco, Cesidio Capoccia, Michele Caponero, Danilo Santos Cardoso, Gianluca Cavoto, André Cortez, Igor Abritta Costa, Emiliano Dané, Giorgio Dho, Flaminia Di Giambattista, Emanuele Di Marco, Giulia D’Imperio, Francesco Iacoangeli, Herman Pessoa Lima, Guilherme Sebastiao Pinheiro Lopes, Giovanni Maccarrone, Rui Daniel Passos Mano, Robert Renz Marcelo Gregorio, David José Gaspar Marques, Giovanni Mazzitelli, Alasdair Gregor McLean, Andrea Messina, Cristina Maria Bernardes Monteiro, Rafael Antunes Nobrega, Igor Fonseca Pains, Emiloano Paoletti, Luciano Passamonti, Sandro Pelosi, Fabrizio Petrucci, Stefano Piacentini, Davide Piccolo, Daniele Pierluigi, Davide Pinci, Atul Prajapati, Francesco Renga, Rita Joanna da Cruz Roque, Filippo Rosatelli, Alessandro Russo, Joaquim Marques Ferreira dos Santos, Giovanna Saviano, Neil John Curwen Spooner, Roberto Tesauro, Sandro Tommasini, Samuele Torelli
The CYGNO project aims at the development of a high precision optical readout gaseous Tima Projection Chamber (TPC) for directional dark matter (DM) searches, to be hosted at Laboratori Nazionali del Gran Sasso (LNGS). CYGNO employs a He:CF$_4$ gas m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::51022fdbaa233e3140ffc224a53e335c
https://hdl.handle.net/11573/1681502
https://hdl.handle.net/11573/1681502
Autor:
Fernando Domingues Amaro, Elisabetta Baracchini, Luigi Benussi, Stefano Bianco, Cesidio Capoccia, Michele Caponero, Danilo Santos Cardoso, Gianluca Cavoto, André Cortez, Igor Abritta Costa, Emiliano Dané, Giorgio Dho, Flaminia Di Giambattista, Emanuele Di Marco, Giulia D’Imperio, Francesco Iacoangeli, Herman Pessoa Lima Júnior, Guilherme Sebastiao Pinheiro Lopes, Giovanni Maccarrone, Rui Daniel Passos Mano, Robert Renz Marcelo Gregorio, David José Gaspar Marques, Giovanni Mazzitelli, Alasdair Gregor McLean, Andrea Messina, Cristina Maria Bernardes Monteiro, Rafael Antunes Nobrega, Igor Fonseca Pains, Emiliano Paoletti, Luciano Passamonti, Sandro Pelosi, Fabrizio Petrucci, Stefano Piacentini, Davide Piccolo, Daniele Pierluigi, Davide Pinci, Atul Prajapati, Francesco Renga, Rita Joanna da Cruz Roque, Filippo Rosatelli, Alessandro Russo, Joaquim Marques Ferreira dos Santos, Giovanna Saviano, Neil John Curwen Spooner, Roberto Tesauro, Sandro Tomassini, Samuele Torelli
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 1051:168207
The CYGNO experiment aims at the development of a large gaseous TPC with GEM-based amplification and an optical readout by means of PMTs and scientific CMOS cameras for 3D tracking down to O(keV) energies, for the directional detection of rare events