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

Contribution List

185 / 185
Dr Francesco Sette (ESRF) , Sergio Bertolucci (Istituto Nazionale Fisica Nucleare Frascati (IT))
30/06/2016, 08:30
Sergio Bertolucci (Istituto Nazionale Fisica Nucleare Frascati (IT))
30/06/2016, 10:00
Cinzia Da Via (University of Manchester (GB))
30/06/2016, 11:00
Jan Jakubek (ADVACAM)
30/06/2016, 11:15
Dr Enrico Perelli Cippo (CNR & Università Milano-Bicocca (IT))
30/06/2016, 11:30
Claudio Gatti (Istituto Nazionale Fisica Nucleare Frascati (IT))
30/06/2016, 11:45
Gianluca Valentino (University of Malta (MT))
30/06/2016, 12:00
Marcel Stanitzki (Rutherford Appleton Laboratory)
30/06/2016, 12:15
Prof. Javier Solana (ESADE)
30/06/2016, 14:00
Ruud Vullers (Teledyne Dalsa)
30/06/2016, 14:30
Michael Deveaux (University Frankfurt)
30/06/2016, 14:45
Ivan Vila Alvarez (Universidad de Cantabria (ES))
30/06/2016, 15:00
Walter Ruetten (Philips Research / Philips Electronics Nederland BV)
30/06/2016, 15:15
Ricardo Graciani Diaz (University of Barcelona (ES))
30/06/2016, 15:30
Lucio Pancheri (University of Trento)
30/06/2016, 15:45
Roberto Mendicino (UNITN)
30/06/2016, 16:00
Hanno Perrey (Lund University)
30/06/2016, 16:15
Niels van Bakel (Nikhef)
30/06/2016, 17:00
Dr Marco Endrizzi (University College London)
30/06/2016, 17:30
Mrs Alessia Matruglio (IOM-CNR)
30/06/2016, 17:45
Piet Verwilligen (Universita e INFN, Bari (IT))
30/06/2016, 18:00
Jens Biegert (ICFO - The Institute of Photonic Sciences)
30/06/2016, 18:15
Carlo Fiorini (Politecnico di Milano - INFN Milano)
30/06/2016, 18:30
Christopher Hall (Australian Synchrotron)
30/06/2016, 18:45
30/06/2016, 19:00
Palma Rita Altieri (Universita e INFN, Bari (IT))
01/07/2016, 08:30
Pietro Albicocco (Istituto Nazionale Fisica Nucleare Frascati (IT))
01/07/2016, 08:45
Lodovico Ratti (Universita e INFN, Pavia (IT))
01/07/2016, 09:00
Harry Van Der Graaf (Nikhef National institute for subatomic physics (NL))
01/07/2016, 09:15
Gianluca Lamanna (Istituto Nazionale Fisica Nucleare Frascati (IT))
01/07/2016, 09:30
Dr Christoph Posch (Chronocam)
01/07/2016, 09:45
Davide Pinci (Universita e INFN, Roma I (IT))
01/07/2016, 10:00
Dr Gabriele Croci (Università degli studi di Milano Bicocca and INFN)
01/07/2016, 10:15
Jacopo Ferretti (INFN - National Institute for Nuclear Physics)
01/07/2016, 11:15
Alessandro Curioni (Politecnico di Milano (IT))
01/07/2016, 11:30
Massimiliano Fiorini (Universita di Ferrara & INFN (IT))
01/07/2016, 11:45
Prof. Elisabeth Koffeman (Nikhef)
01/07/2016, 12:00
Giulio Aielli (Universita e INFN Roma Tor Vergata (IT))
01/07/2016, 12:15
Lauri PARKKONEN (Aalto University)
01/07/2016, 13:30
Joao F.C.A. Veloso (Uni Aveiro)
01/07/2016, 13:45
Aristoteles Kyriakis (Nat. Cent. for Sci. Res. Demokritos (GR))
01/07/2016, 14:15
Mr Marco Lazzarino (IOM-CNR)
01/07/2016, 14:30
Defne Us (Tampere University of Technology)
01/07/2016, 14:45
Aleksandra Biegun (KVI-Center for Advanced Radiation Technology, University of Groningen)
01/07/2016, 15:30
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)
01/07/2016, 15:45
Gerasimos Konstantatos (ICFO - Institut de Ciencies Fotoniques)
01/07/2016, 16:00
Guobin Jia (Leibniz Institute of Photonic Technology)
01/07/2016, 16:15
Patrick Van Esch
01/07/2016, 16:30
Lars Hufnagel (EMBL Heidelberg)
01/07/2016, 16:45
Benoit Dupont (Pyxalis)
01/07/2016, 17:00
01/07/2016, 17:30
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...