Heating and atom loss during upward ramps of Feshbach resonance levels in Bose-Einstein condensates
The production of pairs of fast atoms leads to a pronounced loss of atoms during upward ramps of Feshbach resonance
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Heating Field Theory the ``Environmentally Friendly'' Way!
We discuss how to implement an ``environmentally friendly'' renormalization in the context of finite temperature field theory. Environmentally friendly renormalization
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Heating-free I-V of the `intrinsic' Josephson effect
I present arguments favouring linearity of the intrinsic (heating-free) I-V of the `intrinsic' Josephson effect.
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Heating of a two-dimensional electron gas by the electric field of a surface acoustic wave
The heating of a two-dimensional electron gas by an rf electric field generated by a surface acoustic wave, which can
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Heating of Gas in Galaxy Groups and Clusters
Was the diffuse gas in galaxy groups and clusters heated at high redshift before it entered a massive halo, or
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Heating of Oil Well by Hot Water Circulation
When highly viscous oil is produced at low temperatures, large pressure drops will significantly decrease production rate. One of possible
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Heating the Gas in Photodissociation Fronts
ISO has provided us with a new perspective on gas temperatures in photodissociation regions through measurements of line emission from
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Heating the O(N) nonlinear sigma model
The thermodynamics of the O(N) nonlinear sigma model in 1+1 dimensions is studied. We calculate the finite temperature effective potential
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Heating the Quiet Corona by Nanoflares: Evidence and Problems
The content of coronal material in the quiet Sun is not constant as soft X-ray and high-temperature EUV line observations
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Accretion Disk Models with Self-Consistent Advective Cooling and Heating
We present solutions to the accretion disk structure equations in which advective cooling is accounted for in a self-consistent way.
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AD Leo from X-Rays to Radio: Are Flares Responsible for the Heating of Stellar Coronae?
In spring 1999, a long coordinated observing campaign was performed on the flare star AD Leo, including {\it EUVE}, {\it
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Alfven heating in optical filaments in cooling flows
One of the major problems concerning cooling flows is the nature of the mechanism powering the emission lines of the
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Anomalous Temperature Dependence of Heat Capacity During a Cooling-Heating Cycle in Glassy Systems
Anomalous temperature dependence of heat capacity of glassy systems during a cooling-heating cycle has remained an ill-understood problem for a
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Compressional Heating of Accreting White Dwarfs in CV's
In recent years several Dwarf Novae (DN) systems have been observed in quiescence, when the accretion rate is low and
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Cooling Flows or Heating Flows?
It is now clear that AGN heat cooling flows, largely by driving winds. The winds may contain a relativistic component
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Coronal heating and emission mechanisms in AGN
Popular models for the formation of X-ray spectra in AGN assume that a large fraction of the disk's angular momentum
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Coronal Heating versus Solar Wind Acceleration
Parker's initial insights from 1958 provided a key causal link between the heating of the solar corona and the acceleration
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Current heating of a magnetic 2DEG in HgMnTe/HgCdTe quantum wells
Heating caused by electrons with excess kinetic energy has been investigated in a magnetic two-dimensional electron gas, M2DEG, in HgMnTe/HgCdTe(001)
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Differential neutrino heating and reduced $^4$He production from decaying particles in the early universe
A decaying particle that dominates the energy density of the universe and then decays with a lifetime $\sim 10^{-1}$ sec
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Disk heating and stellar migration in galaxies
The paper claimed that significant radial migration of stars in a stellar disk like that of the Milky Way could
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Evidence for the Heating of Atomic Interstellar Gas by PAHs
We report a strong correlation between the [CII] 158 micron cooling line and the mid-infrared flux in the 5-10 micron
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Giant planet formation from disk instability; cooling and heating
We present the results of high resolution SPH simulations of the evolution of gravitationally unstable protoplanetary disks. We report on
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Grain Size Distributions and Photo-Electric Heating in Ionized Regions
In this paper we present results obtained with the new grain code in Cloudy which underline the strong effect of
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Group Scaling Relations From a Cosmological Hydrodynamic Simulation: No Pre-heating Required?
We investigate the X-ray vs. optical scaling relations of poor groups to small clusters (sigma~100-700 km/s) identified in a cosmological
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