Published August 1, 2009 | Version v1
Journal article

Dark energy and Josephson junctions

  • 1. Department of Physics, University of Catania, Via Santa Sofia 64, I-95123, Catania (Italy)
  • 2. Scuola Superiore di Catania, Via S. Nullo 5/i, Catania (Italy)

Description

It has been recently claimed that dark energy can be (and has been) observed in laboratory experiments by measuring the power spectrum SI(ω) of the noise current in a resistively shunted Josephson junction and that in new dedicated experiments, which will soon test a higher frequency range, SI(ω) should show a deviation from the linear rising observed in the lower frequency region because higher frequencies should not contribute to dark energy. Based on previous work on theoretical aspects of the fluctuation-dissipation theorem, we carefully investigate these issues and show that these claims are based on a misunderstanding of the physical origin of the spectral function SI(ω). According to our analysis, dark energy has never been (and will never be) observed in Josephson junctions experiments. We also predict that no deviation from the linear rising behavior of SI(ω) will be observed in forthcoming experiments. Our findings provide new (we believe definite) arguments which strongly support previous criticisms

Availability note (English)

Available from http://dx.doi.org/10.1088/1475-7516/2009/08/011

Additional details

Publishing Information

Journal Title
Journal of Cosmology and Astroparticle Physics
Journal Volume
2009
Journal Issue
08
Journal Page Range
p. 011
ISSN
1475-7516

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
45094452
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ASTROPHYSICS; COSMOLOGY; ENERGY SPECTRA; EXPERIMENT PLANNING; FLUCTUATIONS; JOSEPHSON JUNCTIONS; NOISE; NONLUMINOUS MATTER; SPECTRAL FUNCTIONS
Descriptors DEC
FUNCTIONS; MATTER; PHYSICS; PLANNING; SPECTRA; SUPERCONDUCTING JUNCTIONS; VARIATIONS