June 30, 2016 to July 1, 2016
Other Institutes
Europe/Zurich timezone

Contribution List

185 / 185
Dr Francesco Sette (ESRF), Sergio Bertolucci (Istituto Nazionale Fisica Nucleare Frascati (IT))
6/30/16, 8:30 AM
Sergio Bertolucci (Istituto Nazionale Fisica Nucleare Frascati (IT))
6/30/16, 10:00 AM
Cinzia Da Via (University of Manchester (GB))
6/30/16, 11:00 AM
Jan Jakubek (ADVACAM)
6/30/16, 11:15 AM
Dr Enrico Perelli Cippo (CNR & Università Milano-Bicocca (IT))
6/30/16, 11:30 AM
Claudio Gatti (Istituto Nazionale Fisica Nucleare Frascati (IT))
6/30/16, 11:45 AM
Gianluca Valentino (University of Malta (MT))
6/30/16, 12:00 PM
Marcel Stanitzki (Rutherford Appleton Laboratory)
6/30/16, 12:15 PM
Prof. Javier Solana (ESADE)
6/30/16, 2:00 PM
Ruud Vullers (Teledyne Dalsa)
6/30/16, 2:30 PM
Michael Deveaux (University Frankfurt)
6/30/16, 2:45 PM
Ivan Vila Alvarez (Universidad de Cantabria (ES))
6/30/16, 3:00 PM
Walter Ruetten (Philips Research / Philips Electronics Nederland BV)
6/30/16, 3:15 PM
Ricardo Graciani Diaz (University of Barcelona (ES))
6/30/16, 3:30 PM
Lucio Pancheri (University of Trento)
6/30/16, 3:45 PM
Roberto Mendicino (UNITN)
6/30/16, 4:00 PM
Hanno Perrey (Lund University)
6/30/16, 4:15 PM
Niels van Bakel (Nikhef)
6/30/16, 5:00 PM
Dr Marco Endrizzi (University College London)
6/30/16, 5:30 PM
Mrs Alessia Matruglio (IOM-CNR)
6/30/16, 5:45 PM
Piet Verwilligen (Universita e INFN, Bari (IT))
6/30/16, 6:00 PM
Jens Biegert (ICFO - The Institute of Photonic Sciences)
6/30/16, 6:15 PM
Carlo Fiorini (Politecnico di Milano - INFN Milano)
6/30/16, 6:30 PM
Christopher Hall (Australian Synchrotron)
6/30/16, 6:45 PM
6/30/16, 7:00 PM
Palma Rita Altieri (Universita e INFN, Bari (IT))
7/1/16, 8:30 AM
Pietro Albicocco (Istituto Nazionale Fisica Nucleare Frascati (IT))
7/1/16, 8:45 AM
Lodovico Ratti (Universita e INFN, Pavia (IT))
7/1/16, 9:00 AM
Harry Van Der Graaf (Nikhef National institute for subatomic physics (NL))
7/1/16, 9:15 AM
Gianluca Lamanna (Istituto Nazionale Fisica Nucleare Frascati (IT))
7/1/16, 9:30 AM
Dr Christoph Posch (Chronocam)
7/1/16, 9:45 AM
Davide Pinci (Universita e INFN, Roma I (IT))
7/1/16, 10:00 AM
Dr Gabriele Croci (Università degli studi di Milano Bicocca and INFN)
7/1/16, 10:15 AM
Jacopo Ferretti (INFN - National Institute for Nuclear Physics)
7/1/16, 11:15 AM
Alessandro Curioni (Politecnico di Milano (IT))
7/1/16, 11:30 AM
Massimiliano Fiorini (Universita di Ferrara & INFN (IT))
7/1/16, 11:45 AM
Prof. Elisabeth Koffeman (Nikhef)
7/1/16, 12:00 PM
Giulio Aielli (Universita e INFN Roma Tor Vergata (IT))
7/1/16, 12:15 PM
Lauri PARKKONEN (Aalto University)
7/1/16, 1:30 PM
Joao F.C.A. Veloso (Uni Aveiro)
7/1/16, 1:45 PM
Aristoteles Kyriakis (Nat. Cent. for Sci. Res. Demokritos (GR))
7/1/16, 2:15 PM
Mr Marco Lazzarino (IOM-CNR)
7/1/16, 2:30 PM
Defne Us (Tampere University of Technology)
7/1/16, 2:45 PM
Aleksandra Biegun (KVI-Center for Advanced Radiation Technology, University of Groningen)
7/1/16, 3:30 PM
Dr Carina Höglund (1Department of Physics, Chemistry, and Biology (IFM), Thin Film Physics Division, Linköping University, SE-581 83 Linköping, Sweden; 2European Spallation Source ERIC, P.O Box 176, SE-221 00 Lund, Sweden)
7/1/16, 3:45 PM
Gerasimos Konstantatos (ICFO - Institut de Ciencies Fotoniques)
7/1/16, 4:00 PM
Guobin Jia (Leibniz Institute of Photonic Technology)
7/1/16, 4:15 PM
Patrick Van Esch
7/1/16, 4:30 PM
Lars Hufnagel (EMBL Heidelberg)
7/1/16, 4:45 PM
Benoit Dupont (Pyxalis)
7/1/16, 5:00 PM
7/1/16, 5:30 PM
Antonio Polosa (Universita' La Sapienza, Roma - Italy), Dr Francesco Giazotto (NEST, Istituto Nanoscienze-CNR and Scuola Normale Superiore), Gianluca Cavoto (Universita e INFN, Roma I (IT)), Jacopo Ferretti (INFN - National Institute for Nuclear Physics), Dr Ludovico Capparelli (UCLA), Paolo Spagnolo (Universita di Pisa & INFN (IT))

We discuss an improved detection scheme for a light-shining-through-wall (LSW) experiment for axion-like particle searches [Capparelli, Cavoto, Ferretti, Giazotto, Polosa and Spagnolo, arXiv: 1510.06892]. We propose to use: extremely intense photon fluxes (from 100 kW to 1MW) from gyrotron sources at frequencies around 30 GHz; single photon detectors in this frequency domain, with efficiency...