C. Braggio
University of Ferrara
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Featured researches published by C. Braggio.
EPL | 2005
C. Braggio; G. Bressi; G. Carugno; C. Del Noce; G. Galeazzi; A. Lombardi; A. Palmieri; G. Ruoso; D. Zanello
In order to observe the Casimir radiation we propose a new experimental scheme with no mechanically moving mirror. In fact we estimate that the power required for a sustained mechanical vibration would be beyond present experimental possibilities. Our apparatus consists of a superconducting electromagnetic resonant cavity with a wall covered by a semiconductor layer whose reflectivity is driven by a laser at gigahertz frequencies. The semiconductor thus acts as a moving mirror. Preliminary laboratory tests showed that a semiconductor can indeed reflect microwaves as efficiently as a conductor. In this paper we present the complete scheme that we intend to set up for the detection of the Casimir radiation.
IEEE Transactions on Applied Superconductivity | 2011
Giovanni Giunchi; A. Figini Albisetti; C. Braggio; G. Carugno; G. Messineo; G. Ruoso; G. Galeazzi; F. Della Valle
The use of radio frequencies (RF) superconducting re-entrant cavities has been suggested in the framework of some research to detect photon generation from the vacuum, due to the dynamical Casimir effect. A thin semiconducting slab, put inside the cavity, will be excited by a train of laser pulses of a frequency twice the resonant frequency of the cavity, so that a periodic modulation of the dielectric constant of the slab will be realized. In order to produce a RF cavity that can safely work at temperatures larger than 4 K, we have designed and constructed a MgB2 re-entrant cavity having a resonant frequency in the range of 2-3 GHz. The cavity is made by a cylindrical cup of about 40 mm of internal diameter and 40 mm of height and on its base is standing a cylindrical coaxial nose on which the semiconductor slab will be deposited. The details of the construction of the MgB2 cavity will be presented as well as the measurements of its quality factor, as a function of the temperature.
IEEE Transactions on Applied Superconductivity | 2011
Giovanni Giunchi; A. Figini Albisetti; C. Braggio; G. Carugno; G. Messineo; G. Ruoso; G. Galeazzi; F. Della Valle
The use of radio frequencies (RF) superconducting re-entrant cavities has been suggested in the framework of some research to detect photon generation from the vacuum, due to the dynamical Casimir effect. A thin semiconducting slab, put inside the cavity, will be excited by a train of laser pulses of a frequency twice the resonant frequency of the cavity, so that a periodic modulation of the dielectric constant of the slab will be realized. In order to produce a RF cavity that can safely work at temperatures larger than 4 K, we have designed and constructed a MgB2 re-entrant cavity having a resonant frequency in the range of 2-3 GHz. The cavity is made by a cylindrical cup of about 40 mm of internal diameter and 40 mm of height and on its base is standing a cylindrical coaxial nose on which the semiconductor slab will be deposited. The details of the construction of the MgB2 cavity will be presented as well as the measurements of its quality factor, as a function of the temperature.
IEEE Transactions on Applied Superconductivity | 2011
Giovanni Giunchi; A. Figini Albisetti; C. Braggio; G. Carugno; G. Messineo; G. Ruoso; G. Galeazzi; F. Della Valle
The use of radio frequencies (RF) superconducting re-entrant cavities has been suggested in the framework of some research to detect photon generation from the vacuum, due to the dynamical Casimir effect. A thin semiconducting slab, put inside the cavity, will be excited by a train of laser pulses of a frequency twice the resonant frequency of the cavity, so that a periodic modulation of the dielectric constant of the slab will be realized. In order to produce a RF cavity that can safely work at temperatures larger than 4 K, we have designed and constructed a MgB2 re-entrant cavity having a resonant frequency in the range of 2-3 GHz. The cavity is made by a cylindrical cup of about 40 mm of internal diameter and 40 mm of height and on its base is standing a cylindrical coaxial nose on which the semiconductor slab will be deposited. The details of the construction of the MgB2 cavity will be presented as well as the measurements of its quality factor, as a function of the temperature.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2006
C. Braggio; G. Bressi; G. Carugno; E. Feltrin; G. Galeazzi
Physical Review A | 2013
G. Galeazzi; A. Lombardi; G. Ruoso; C. Braggio; G. Carugno; F. Della Valle; D. Zanello; V. V. Dodonov
New Journal of Physics | 2013
C. Braggio; G. Carugno; F. Della Valle; G. Galeazzi; A. Lombardi; G. Ruoso; D. Zanello
Physics Letters A | 2007
C. Braggio; G. Bressi; G. Carugno; A. V. Dodonov; V. V. Dodonov; G. Galeazzi; G. Ruoso; D. Zanello
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2007
C. Braggio; G. Bressi; G. Carugno; G. Galeazzi; A. Serafin
EPL | 2007
C. Braggio; G. Bressi; G. Carugno; C. Del Noce; G. Galeazzi; A. Lombardi; A. Palmieri; G. Ruoso; D. Zanello