16,376 research outputs found
Generating Functions, Polynomials and Vortices with Alternating Signs in Bose-Einstein Condensates
In this work, we construct suitable generating functions for vortices of
alternating signs in the realm of Bose-Einstein condensates. In addition to the
vortex-vortex interaction included in earlier fluid dynamics constructions of
such functions, the vortices here precess around the center of the trap. This
results in the generating functions of the vortices of positive charge and of
negative charge satisfying a modified, so-called, Tkachenko differential
equation. From that equation, we reconstruct collinear few-vortex equilibria
obtained in earlier work, as well as extend them to larger numbers of vortices.
Moreover, particular moment conditions can be derived e.g. about the sum of the
squared locations of the vortices for arbitrary vortex numbers. Furthermore,
the relevant differential equation can be generalized appropriately in the
two-dimensional complex plane and allows the construction e.g. of polygonal
vortex ring and multi-ring configurations, as well as ones with rings
surrounding a vortex at the center that are again connected to earlier
bibliography.Comment: 15 pages, no figure
Detection of the Red Giant Branch Stars in M82 Using the Hubble Space Telescope
We present color-magnitude diagrams and luminosity functions of stars in two
halo regions of the irregular galaxy in M82, based on F555W and F814W
photometry taken with the Hubble Space Telescope and Wide Field Planetary
Camera 2. The I-band luminosity function shows a sudden jump at I~23.95 mag,
which is identified as the tip of the red giant branch (TRGB). Adopting the Lee
et al. (1993) calibration of the TRGB based on the RR Lyrae distances to
Galactic globular clusters, we obtain the distance modulus of (m-M)_0=27.95 +-
0.14 (random) +- 0.16 (systematic) mag. This corresponds to a linear distance
of 3.9 +- 0.3 (random) +- 0.3 (systematicf) Mpc, which agrees well with the
distance of M81 deteremined from the HST observations of the Cepheid variable
stars. In addition, we observe a significant number of stars apparently
brighter than the TRGB. However, with the current data, we cannot rule out
whether these stars are blends of fainter stars, or are indeed intermediate-age
asymptotic giant branch stars.Comment: 8 figure
Collaboration technology and space science
A summary of available collaboration technologies and their applications to space science is presented as well as investigations into remote coaching paradigms and the role of a specific collaboration tool for distributed task coordination in supporting such teleoperations. The applicability and effectiveness of different communication media and tools in supporting remote coaching are investigated. One investigation concerns a distributed check-list, a computer-based tool that allows a group of people, e.g., onboard crew, ground based investigator, and mission control, to synchronize their actions while providing full flexibility for the flight crew to set the pace and remain on their operational schedule. This autonomy is shown to contribute to morale and productivity
Nimbus 7 Solar Backscatter Ultraviolet (SBUV) spectral scan solar irradiance and Earth radiance product user's guide
The archived tape products from the spectral scan mode measurements of solar irradiance (SUNC tapes) and Earth radiance (EARTH tapes) by the Solar Backscatter UV (SBUV) instrument aboard Nimbus 7 are described. Incoming radiation from 160 to 400 nm is measured at intervals of 0.2 nm. The scan-to-scan repeatability of the solar irradiance measurements ranges from approximately 0.5 to 1 percent longward of 280 nm, to 2 percent around 210 nm and 4 percent near 175 nm. The repeatability of the Earth radiance values ranges from 2 to 3 percent at longer wavelengths and low zenith angles to 10 percent at shorter wavelengths and high zenith angles. The tape formats are described in detail, including file structure and contents of each type of record. Catalogs of the tapes and the time period covered are provided, along with lists of the days lacking solar irradiance measurements and the days dedicated to Earth radiance measurements. The method for production of the tapes is outlined and quality control measures are described. How radiances and irradiances are derived from the raw counts, the corrections for changes in instrument sensitivity, and related uncertainties are discussed
Leptogenesis in models with keV sterile neutrino dark matter
We analyze leptogenesis in gauge extensions of the Standard Model with keV
sterile neutrino dark matter. We find that both the observed dark matter
abundance and the correct baryon asymmetry of the Universe can simultaneously
emerge in these models. Both the dark matter abundance and the leptogenesis are
controlled by the out of equilibrium decays of the same heavy right handed
neutrino.Comment: 6 pages, 1 figur
The FHD/ppsilon Epoch of Reionization Power Spectrum Pipeline
Epoch of Reionization data analysis requires unprecedented levels of accuracy
in radio interferometer pipelines. We have developed an imaging power spectrum
analysis to meet these requirements and generate robust 21 cm EoR measurements.
In this work, we build a signal path framework to mathematically describe each
step in the analysis, from data reduction in the FHD package to power spectrum
generation in the ppsilon package. In particular, we focus on the
distinguishing characteristics of FHD/ppsilon: highly accurate
spectral calibration, extensive data verification products, and end-to-end
error propagation. We present our key data analysis products in detail to
facilitate understanding of the prominent systematics in image-based power
spectrum analyses. As a verification to our analysis, we also highlight a
full-pipeline analysis simulation to demonstrate signal preservation and lack
of signal loss. This careful treatment ensures that the
FHD/ppsilon power spectrum pipeline can reduce radio
interferometric data to produce credible 21 cm EoR measurements.Comment: 21 pages, 10 figures, accepted by PAS
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