1,716 research outputs found
AF-algebras and topology of mapping tori
A covariant functor from the category of mapping tori to a category of
AF-algebras is constructed; the functor takes continuous maps between such
manifolds to stable homomorphisms between the corresponding AF-algebras. We use
this functor to develop an obstruction theory for the torus bundles of
dimension 2, 3 and 4.Comment: to appear Czechoslovak Math.
The Embedded Super Star Cluster of SBS0335-052
We analyze the infrared (6-100 micron) spectral energy distribution of the
blue compact dwarf and metal-poor (Z=Z_solar/41) galaxy SBS0335-052. With the
help of DUSTY (Ivezic et al. 1999), a program that solves the radiation
transfer equations in a spherical environment, we evaluate that the infrared
(IR) emission of SBS0335-052 is produced by an embedded super-star cluster
(SSC) hidden under 10^5 M_solar of dust, causing 30 mag of visual extinction.
This implies that one cannot detect any stellar emission from the 2x10^6
M_solar stellar cluster even at near-infrared (NIR) wavelengths. The derived
grain size distribution departs markedly from the widely accepted size
distribution inferred for dust in our galaxy (the so-called MRN distribution,
Mathis et al. 1977), but resembles what is seen around AGNs, namely an absence
of PAH and smaller grains, and grains that grow to larger sizes (around 1
micron). The fact that a significant amount of dust is present in such a
low-metallicity galaxy, hiding from UV and optical view most of the star
formation activity in the galaxy, and that the dust size distribution cannot be
reproduced by a standard galactic law, should be borne in mind when
interpreting the spectrum of primeval galaxies.Comment: 32 pages, 3 figures,accepted for publication in A
Overview of NASARTI (NASA Radiation Track Image) Program: Highlights of the Model Improvement and the New Results
This presentation summarizes several years of research done by the co-authors developing the NASARTI (NASA Radiation Track Image) program and supporting it with scientific data. The goal of the program is to support NASA mission to achieve a safe space travel for humans despite the perils of space radiation. The program focuses on selected topics in radiation biology that were deemed important throughout this period of time, both for the NASA human space flight program and to academic radiation research. Besides scientific support to develop strategies protecting humans against an exposure to deep space radiation during space missions, and understanding health effects from space radiation on astronauts, other important ramifications of the ionizing radiation were studied with the applicability to greater human needs: understanding the origins of cancer, the impact on human genome, and the application of computer technology to biological research addressing the health of general population. The models under NASARTI project include: the general properties of ionizing radiation, such as particular track structure, the effects of radiation on human DNA, visualization and the statistical properties of DSBs (DNA double-strand breaks), DNA damage and repair pathways models and cell phenotypes, chromosomal aberrations, microscopy data analysis and the application to human tissue damage and cancer models. The development of the GUI and the interactive website, as deliverables to NASA operations teams and tools for a broader research community, is discussed. Most recent findings in the area of chromosomal aberrations and the application of the stochastic track structure are also presented
Conservatively treated glassy cell carcinoma of the cervix
<p>Abstract</p> <p>Background</p> <p>Very little data about the conservative treatment of early stage glassy cell cervical cancer have been reported.</p> <p>Case presentation</p> <p>A 30-year old patient, nulligravida was admitted to the Gynecologic Oncology Unit of the Catholic University of Campobasso for irregular post-coital vaginal bleeding. The patients was staged as having FIGO stage IB1 (tumor diameter = 2 cm) squamous cervical cancer. After extensive counseling of the patient and her family, laparoscopic pelvic lymphadenectomy and cold knife conization were performed. The final diagnosis was FIGO Stage IB1 glassy cell carcinoma. Currently, after a follow-up of 38 months, she has no evidence of disease.</p> <p>Conclusion</p> <p>We reported a case of early stage glassy cell cancer patient, who was conservatively treated by conization and laparoscopic pelvic lymphadenectomy.</p
Study of nuclear recoils in liquid argon with monoenergetic neutrons
For the development of liquid argon dark matter detectors we assembled a
setup in the laboratory to scatter neutrons on a small liquid argon target. The
neutrons are produced mono-energetically (E_kin=2.45 MeV) by nuclear fusion in
a deuterium plasma and are collimated onto a 3" liquid argon cell operating in
single-phase mode (zero electric field). Organic liquid scintillators are used
to tag scattered neutrons and to provide a time-of-flight measurement. The
setup is designed to study light pulse shapes and scintillation yields from
nuclear and electronic recoils as well as from {\alpha}-particles at working
points relevant to dark matter searches. Liquid argon offers the possibility to
scrutinise scintillation yields in noble liquids with respect to the
populations of the two fundamental excimer states. Here we present experimental
methods and first results from recent data towards such studies.Comment: 9 pages, 8 figures, proceedings of TAUP 2011, to be published in
Journal of Physics: Conference Series (JCPS
3D Position Sensitive XeTPC for Dark Matter Search
The technique to realize 3D position sensitivity in a two-phase xenon time
projection chamber (XeTPC) for dark matter search is described. Results from a
prototype detector (XENON3) are presented.Comment: Presented at the 7th UCLA Symposium on "Sources and Detection of Dark
Matter and Dark Energy in the Universe
Constraints on inelastic dark matter from XENON10
It has been suggested that dark matter particles which scatter inelastically
from detector target nuclei could explain the apparent incompatibility of the
DAMA modulation signal (interpreted as evidence for particle dark matter) with
the null results from CDMS-II and XENON10. Among the predictions of
inelastically interacting dark matter are a suppression of low-energy events,
and a population of nuclear recoil events at higher nuclear recoil equivalent
energies. This is in stark contrast to the well-known expectation of a falling
exponential spectrum for the case of elastic interactions. We present a new
analysis of XENON10 dark matter search data extending to E keV
nuclear recoil equivalent energy. Our results exclude a significant region of
previously allowed parameter space in the model of inelastically interacting
dark matter. In particular, it is found that dark matter particle masses
GeV are disfavored.Comment: 8 pages, 4 figure
First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory
The XENON10 experiment at the Gran Sasso National Laboratory uses a 15 kg
xenon dual phase time projection chamber (XeTPC) to search for dark matter
weakly interacting massive particles (WIMPs). The detector measures
simultaneously the scintillation and the ionization produced by radiation in
pure liquid xenon, to discriminate signal from background down to 4.5 keV
nuclear recoil energy. A blind analysis of 58.6 live days of data, acquired
between October 6, 2006 and February 14, 2007, and using a fiducial mass of 5.4
kg, excludes previously unexplored parameter space, setting a new 90% C.L.
upper limit for the WIMP-nucleon spin-independent cross-section of 8.8 x
10^{-44} cm^2 for a WIMP mass of 100 GeV/c^2, and 4.5 x 10^{-44} cm^2 for a
WIMP mass of 30 GeV/c^2. This result further constrains predictions of
supersymmetric models.Comment: accepted for publication in Phys. Rev. Let
A search for light dark matter in XENON10 data
We report results of a search for light (<10 GeV) particle dark matter with
the XENON10 detector. The event trigger was sensitive to a single electron,
with the analysis threshold of 5 electrons corresponding to 1.4 keV nuclear
recoil energy. Considering spin-independent dark matter-nucleon scattering, we
exclude cross sections \sigma_n>3.5x10^{-42} cm^2, for a dark matter particle
mass m_{\chi}=8 GeV. We find that our data strongly constrain recent elastic
dark matter interpretations of excess low-energy events observed by CoGeNT and
CRESST-II, as well as the DAMA annual modulation signal.Comment: Manuscript identical to v2 (published version) but also contains
erratum. Note v3==v2 but without \linenumber
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