Cost-Benefit Analysis of the Greenland Offshore Shrimp Fishery

This paper examines the social economic value of the Greenland off-shore shrimp fishery. The contribution of the fishery to the economy is examined us-ing a cost-benefit analysis where the objective of the report is to examine the current state of the fishery rather than possible changes, which are a political decision. The analysis is undertaken by examining the state and development of the off-shore shrimp fishery in Greenland, as well as the changes in profits, sales and production in the years 2006 and 2007. Financial accounts and costs data pro-vided by the companies fishing in Greenland have contributed to estimating the net value of the industry. The management cost is included as well in the analysis. The paper concludes that there is a positive economic benefit from the shrimp fishery in Greenland, which is believed to be caused by the efficient manage-ment system of the fishery (based on Individual Transferable Quotas). It is fur-ther shown that the companies and the crew gains nearly the whole net-benefit from the fishery, while the public finance are not gaining much. Acknowledgements. We want to thank the contact persons from the companies and Greenland Statistics: Søren Brandt (Qajaq Trawl), Carl Christensen (Niisa Trawl), Jens Bisgaard (Royal Greenland and Ice Trawl), Henrik Krogh and Kjeld Holmstrup (Polar Seafood) and Gert Schmidt, Per Lyster Pedersen and Lars Geraa from Greenland Statistics. We also want to thank Henrik Leth and Jens K. Lyberth from the Confederation of Greenland Employers for good discussions and help during the project as well as financial support. The study was made possible thanks to financial support from the Confederation of Greenland Employers.Greenland, shrimp, fishery, Cost-Benefit Analysis, economic rent

Creation of long-term coherent optical memory via controlled nonlinear interactions in Bose-Einstein condensates

A Bose-Einstein condensate confined in an optical dipole trap is used to generate long-term coherent memory for light, and storage times of more than one second are observed. Phase coherence of the condensate as well as controlled manipulations of elastic and inelastic atomic scattering processes are utilized to increase the storage fidelity by several orders of magnitude over previous schemes. The results have important applications for creation of long-distance quantum networks and for generation of entangled states of light and matter.Comment: published version of the pape

High Redshift Standard Candles: Predicted Cosmological Constraints

We investigate whether future measurements of high redshift standard candles (HzSCs) will be a powerful probe of dark energy, when compared to other types of planned dark energy measurements. Active galactic nuclei and gamma ray bursts have both been proposed as potential HzSC candidates. Due to their high luminosity, they can be used to probe unexplored regions in the expansion history of the universe. Information from these regions can help constrain the properties of dark energy, and in particular, whether it varies over time. We consider both linear and piecewise parameterizations of the dark energy equation of state, $w(z)$, and assess the optimal redshift distribution a high-redshift standard-candle survey could take to constrain these models. The more general the form of the dark energy equation of state $w(z)$ being tested, the more useful high-redshift standard candles become. For a linear parameterization of $w(z)$, HzSCs give only small improvements over planned supernova and baryon acoustic oscillation measurements; a wide redshift range with many low redshift points is optimal to constrain this linear model. However to constrain a general, and thus potentially more informative, form of $w(z)$, having many HzSCs can significantly improve limits on the nature of dark energy.Comment: Accepted MNRAS, 27 Pages, 15 figures, matches published versio

Downsizing of supermassive black holes from the SDSS quasar survey (II). Extension to z~4

Starting from the quasar sample of the Sloan Digital Sky Survey (SDSS) for which the CIV line is observed, we use an analysis scheme to derive the z-dependence of the maximum mass of active black holes, which overcomes the problems related to the Malmquist bias. The same procedure is applied to the low redshift sample of SDSS quasars for which Hbeta measurements are available. Combining with the results from the previously studied MgII sample, we find that the maximum mass of the quasar population increases as (1+z)^(1.64+/-0.04) in the redshift range 0.1<z<4, which includes the epoch of maximum quasar activity.Comment: 9 pages, 8 figures. To appear in MNRA

X-ray Emission from the Radio Jet in 3C 120

We report the discovery of X-ray emission from a radio knot at a projected distance of 25" from the nucleus of the Seyfert galaxy, 3C 120. The data were obtained with the ROSAT High Resolution Imager (HRI). Optical upper limits for the knot preclude a simple power law extension of the radio spectrum and we calculate some of the physical parameters for thermal bremsstrahlung and synchrotron self-Compton models. We conclude that no simple model is consistent with the data but if the knot contains small regions with flat spectra, these could produce the observed X-rays (via synchrotron emission) without being detected at other wavebands.Comment: 6 pages latex plus 3 ps/eps figures. Uses 10pt.sty and emulateapj.sty. Accepted for publication in the ApJ (6 Jan 99