SHIPS EXPERIMENT OVERVIEW
The Solar Hidden Photon Search SHIPS is an
observational astroparticle experiment aiming at detecting the postulated Hidden
Photons (HPs) emitted by the Sun. The observational project - inspired by the
theoretical work of Javier Redondo and Andreas Ringwald - is carried out at the
Hamburger Sternwarte in collaboration with DESY.
Hidden Photons are presumably generated in vast numbers in the Sun's interior and atmosphere. In free space HPs can convert back into real photons through a mechanism analogous to neutrino flavor oscillations. The HP- hν resonant coupling is weak but finite. It can locally be suppressed by
the refractive index of the medium in the oscillation regime, such that a telescope operation in a vacuum is called for. Regenerated electromagnetic
photons propagate along the same trajectories as their HP progenitors,
suggesting the use of an imaging astronomical telescope. Since
secondary HP-photons emerging from the vacuum between the Sun and the
Earth cannot be distinguished from the overwhelming solar flux, the
HP-photon vacuum telescope must also be totally shielded from
parasitic solar and ambient light.
During the SHIPS experiment, the Sun is observed almost continuously in the 'light' of
the HPs with dedicated helioscopes: adapted astronomical telescopes employing
imaging optics and low-flux detectors in a vacuum chamber to achieve high
sensitivity, contrast and spatial resolution.
SHIPS is an offspring of the
ongoing ALPS (“Any Light Particle Search“) projects at DESY.
Unlike the laboratory experiments ALPS and ALPS II, SHIPS does not involve
magnetic fields.
The SHIPS helioscopes are located at the Bergedorf site.
Goals
Optical detection of Solar Hidden Photons
Determination of, resp. limits for HP mass
and HP- hν coupling parameterDevelopment of HP-Astronomy....
Project
The SHIPS experiment
is a part of the SFB676 Project C1 and supported by the State
Excellence Initiative (LEXI) Cluster 'Connecting Particles to the Cosmos'

© 2012 by GW, Hamburger Sternwarte, Universität Hamburg
© 2012 by GW, Hamburger Sternwarte, Universität Hamburg

