19,101 research outputs found

    Electrical power dissipation in carbon nanotubes on single crystal quartz and amorphous SiO2

    Full text link
    Heat dissipation in electrically biased semiconducting carbon nanotubes (CNTs) on single crystal quartz and amorphous SiO2 is examined with temperature profiles obtained by spatially resolved Raman spectroscopy. Despite the differences in phonon velocities, thermal conductivity and van der Waals interactions with CNTs, on average, heat dissipation into single crystal quartz and amorphous SiO2 is found to be similar. Large temperature gradients and local hot spots often observed underscore the complexity of CNT temperature profiles and may be accountable for the similarities observed

    State Public Nuisance Claims and Climate Change Adaptation

    Get PDF
    This Article explores the potential for state public nuisance claims to facilitate adaptation, resource protection, and other climate change responses by coastal communities in California. The California public nuisance actions represent just the latest chapter in efforts to spur responses to climate change and attribute responsibility for climate change through the common law. Part II of this Article describes the California public nuisance lawsuits and situates them in the context of common law actions directed against climate change. Part III considers the preliminary defenses that defendants have raised and could raise in the California public nuisance lawsuits, including the existence of state common law in this context, separation of powers and the political question doctrine, displacement and preemption, and standing. Part IV considers the potential merits of the plaintiffs’ public nuisance claims under California law

    Estimating shallow recharge and discharge in northeastern Illinois using GIS and pattern recognition procedure

    Get PDF
    U.S. Department of the InteriorU.S. Geological Surve

    Conformation-networks of two-dimensional lattice homopolymers

    Full text link
    The effect of different Monte Carlo move sets on the the folding kinetics of lattice polymer chains is studied from the geometry of the conformation-network. The networks have the characteristics of small- world. The Monte Carlo move, rigid rotation, has drastic effect on the geometric properties of the network. The move not only change the connections but also reduce greatly the shortest path length between conformations. The networks are as robust as random network

    Swift Observations of the Be/X-ray Transient System 1A 1118-615

    Full text link
    We report results of Swift observations for the high mass Be/X-ray binary system 1A 1118-615, during an outburst stage in January, 2009 and at a flaring stage in March, 2009. Using the epoch-folding method, we successfully detected a pulsed period of 407.69(2) sec in the outburst of January and of 407.26(1) sec after the flare detection in March. We find that the spectral detection for the source during outburst can be described by a blackbody model with a high temperature (kT ~ 1-3 keV) and a small radius (R ~ 1 km), indicating that the emission results from the polar cap of the neutron star. On the other hand, the spectra obtained after the outburst can further be described by adding an additional component with a lower temperature (kT ~ 0.1-0.2 keV) and a larger emission radius (R ~ 10-500 km), which indicates the emission from around the inner region of an accretion disk. We find that the thermal emission from the hot spot of the accreting neutron star dominates the radiation in outburst; the existence of both this X-ray contribution and the additional soft component suggest that the polar cap and the accretion disk emission might co-exist after the outburst. Because the two-blackbody signature at the flaring stage is a unique feature of 1A 1118-615, our spectral results may provide a new insight to interpret the X-ray emission for the accreting neutron star. The time separation between the three main outbursts of this system is ~17 years and it might be related to the orbital period. We derive and discuss the associated physical properties by assuming the elongated orbit for this specific Be/X-ray transient.Comment: 9 pages, 3 figures and 4 tables; accepted by MNRA
    corecore