857 research outputs found
Foreign direct investment and the political economy of protection
Trade Barriers;Foreign Investment
Repulsive Casimir and Casimir-Polder Forces
Casimir and Casimir-Polder repulsion have been known for more than 50 years.
The general "Lifshitz" configuration of parallel semi-infinite dielectric slabs
permits repulsion if they are separated by a dielectric fluid that has a value
of permittivity that is intermediate between those of the dielectric slabs.
This was indirectly confirmed in the 1970s, and more directly by Capasso's
group recently. It has also been known for many years that electrically and
magnetically polarizable bodies can experience a repulsive quantum vacuum
force. More amenable to practical application are situations where repulsion
could be achieved between ordinary conducting and dielectric bodies in vacuum.
The status of the field of Casimir repulsion with emphasis on recent
developments will be surveyed. Here, stress will be placed on analytic
developments, especially of Casimir-Polder (CP) interactions between
anisotropically polarizable atoms, and CP interactions between anisotropic
atoms and bodies that also exhibit anisotropy, either because of anisotropic
constituents, or because of geometry. Repulsion occurs for wedge-shaped and
cylindrical conductors, provided the geometry is sufficiently asymmetric, that
is, either the wedge is sufficiently sharp or the atom is sufficiently far from
the cylinder.Comment: 24 pages, 14 figures, contribution to the special issue of J. Phys. A
honoring Stuart Dowker. This revision corrects typos and adds additional
references and discussio
Methanol Masers as Tracers of Circumstellar Disks
We show that in many methanol maser sources the masers are located in lines,
with a velocity gradient along them which suggests that the masers are situated
in edge-on circumstellar, or protoplanetary, disks. We present VLBI
observations of the methanol maser source G309.92+0.48, in the 12.2 GHz
transition, which confirm previous observations that the masers in this source
lie along a line. We show that such sources are not only linear in space but,
in many cases, also have a linear velocity gradient. We then model these and
other data in both the 6.7 GHz and the 12.2 GHz transition from a number of
star formation regions, and show that the observed spatial and velocity
distribution of methanol masers, and the derived Keplerian masses, are
consistent with a circumstellar disk rotating around an OB star. We consider
this and other hypotheses, and conclude that about half of these methanol
masers are probably located in edge-on circumstellar disks around young stars.
This is of particular significance for studies of circumstellar disks because
of the detailed velocity information available from the masers.Comment: 38 pages, 13 figures accepted by Ap
Rotating and infalling motion around the high-mass young stellar object Cepheus A-HW2 observed with the methanol maser at 6.7 GHz
We have measured the internal proper motions of the 6.7 GHz methanol masers
associated with Cepheus A (Cep A) HW2 using Very Long Baseline Interferometery
(VLBI) observations. We conducted three epochs of VLBI monitoring observations
of the 6.7 GHz methanol masers in Cep A-HW2 with the Japanese VLBI Network
(JVN) over the period between 2006-2008. In 2006, we were able to use
phase-referencing to measure the absolute coordinates of the maser emission
with an accuracy of a few milliarcseconds. We compared the maser distribution
with other molecular line observations that trace the rotating disk. We
measured the internal proper motions for 29 methanol maser spots, of which 19
were identified at all three epochs and the remaining ten at only two epochs.
The magnitude of proper motions ranged from 0.2 to 7.4 km/s, with an average of
3.1 km/s. Although there are large uncertainties in the observed internal
proper motions of the methanol maser spots in Cep A, they are well fitted by a
disk that includes both rotation and infall velocity components. The derived
rotation and infall velocities at the disk radius of 680 au are 0.5 +- 0.7 and
1.8 +- 0.7 km/s, respectively. Assuming that the modeled disk motion accurately
represents the accretion disk around the Cep A-HW2 high-mass YSO, we estimated
the mass infall rate to be 3 x 10^{-4} n_8 Msun/yr (n_8 is the gas volume
density in units of 10^{8} cm^{-3}). The combination of the estimated mass
infall rate and the magnitude of the fitted infall velocity suggests that Cep
A-HW2 is at an evolutionary phase of active gas accretion from the disk onto
the central high-mass YSO. The infall momentum rate is estimated to be 5 x
10^{-4} n_8 Msun/yr km/s, which is larger than the estimated stellar radiation
pressure of the HW2 object, supporting the hypothesis that this object is in an
active gas accretion phase.Comment: 16 pages, 6 figures, 5 tables, accepted for publication in Astronomy
& Astrophysic
A high-sensitivity 6.7 GHz methanol maser survey toward H2O sources
We present the results of a high sensitivity survey for 6.7 GHz methanol
masers towards 22 GHz water maser using the 100 m Efflesberg telescope. A total
of 89 sources were observed and 10 new methanol masers were detected. The new
detections are relatively faint with peak flux densities between 0.5 and 4.0
Jy. A nil detection rate from low-mass star forming regions enhances the
conclusion that the masers are only associated with massive star formation.
Even the faintest methanol maser in our survey, with a luminosity of 1.1
is associated with massive stars as inferred from its
infrared luminosity.Comment: Accepted for publication in A&
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