406 research outputs found
Space Charge Effects in Cyclotron Gas Stopper
The cyclotron gas stopper is a newly proposed device to stop energetic rare
isotope ions from projectile fragmentation reactions in a helium-filled
chamber. The radioactive ions are slowed down by collisions with a buffer gas
inside a cyclotron-type magnet and are extracted via interactions with a Radio
Frequency (RF) field applied to a sequence of concentric electrodes (RF
carpet). The present study focuses on a detailed understanding of space charge
effects in the ion extraction region. The space charge is generated by the
ionized helium gas created by the stopping of the ions and eventually limits
the beam rate. Particle-in-cell simulations of a two-component
(electron-helium) plasma interacting via Coulomb forces were performed in the
space charge field created by the stopping beam.Comment: 9 pages, 2 tables, 8 figure
Dynamics of Planetary Systems within Star Clusters: Aspects of the Solar Systemâs Early Evolution
Most planetary systemsâincluding our ownâare born within stellar clusters, where interactions with neighboring stars can help shape the system architecture. This paper develops an orbit-averaged formalism to characterize the cluster's mean-field effects, as well as the physics of long-period stellar encounters. Our secular approach allows for an analytic description of the dynamical consequences of the cluster environment on its constituent planetary systems. We analyze special cases of the resulting Hamiltonian, corresponding to eccentricity evolution driven by planar encounters, as well as hyperbolic perturbations upon dissipative disks. We subsequently apply our results to the early evolution of our solar system, where the cluster's collective potential perturbs the solar system's plane, and stellar encounters act to increase the velocity dispersion of the Kuiper Belt. Our results are twofold. First, we find that cluster effects can alter the mean plane of the solar system by âŸ1° and are thus insufficient to explain the Ï â 6° obliquity of the Sun. Second, we delineate the extent to which stellar flybys excite the orbital dispersion of the cold classical Kuiper Belt and show that while stellar flybys may grow the cold belt's inclination by the observed amount, the resulting distribution is incompatible with the data. Correspondingly, our calculations place an upper limit on the product of the stellar number density and residence time of the Sun in its birth cluster, η Ï âŸ 2 Ă 10⎠Myr pcâ»Âł
Analytical treatment of planetary resonances
An ever-growing observational aggregate of extrasolar planets has revealed that systems of planets that reside in or near mean-motion resonances are relatively common. While the origin of such systems is attributed to protoplanetary disk-driven migration, a qualitative description of the dynamical evolution of resonant planets remains largely elusive. Aided by the pioneering works of the last century, we formulate an approximate, integrable theory for first-order resonant motion. We utilize the developed theory to construct an intuitive, geometrical representation of resonances within the context of the unrestricted three-body problem. Moreover, we derive a simple analytical criterion for the appearance of secondary resonances between resonant and secular motion. Subsequently, we demonstrate the onset of rapid chaotic motion as a result of overlap among neighboring first-order mean-motion resonances, as well as the appearance of slow chaos as a result of secular modulation of the planetary orbits. Finally, we take advantage of the integrable theory to analytically show that, in the adiabatic regime, divergent encounters with first-order mean-motion resonances always lead to persistent apsidal anti-alignment
The Mass, Orbit, and Tidal Evolution of the Quaoar-Weywot System
Here we present new adaptive optics observations of the Quaoar-Weywot system.
With these new observations we determine an improved system orbit. Due to a
0.39 day alias that exists in available observations, four possible orbital
solutions are available with periods of , , , and
days. From the possible orbital solutions, system masses of
kg are found. These observations provide an
updated density for Quaoar of 2.7-5.0{g cm^{-3}}. In all cases, Weywot's
orbit is eccentric, with possible values . We present a
reanalysis of the tidal orbital evolution of the Quoaor-Weywot system. We have
found that Weywot has probably evolved to a state of synchronous rotation, and
have likely preserved their initial inclinations over the age of the Solar
system. We find that for plausible values of the effective tidal dissipation
factor tides produce a very slow evolution of Weywot's eccentricity and
semi-major axis. Accordingly, it appears that Weywot's eccentricity likely did
not tidally evolve to its current value from an initially circular orbit.
Rather, it seems that some other mechanism has raised its eccentricity
post-formation, or Weywot formed with a non-negligible eccentricity.Comment: Accepted to Icarus, Nov. 8 201
Stable and habitable systems with two giant planets
We have studied planetary systems which are similar to the Solar System and
built up from three inner rocky planets (Venus, Earth, Mars) and two outer gas
giants. The stability of the orbits of the inner planets is discussed in the
cases of different masses of the gas planets. To demonstrate the results
stability maps were made and it was found that Jupiter could be four times and
Saturn could be three times more massive while the orbits of the inner planets
stay stable. Similar calculations were made by changing the mass of the Sun. In
this case the position of the rocky planets and the extension of the liquid
water habitable and the UV habitable zones were studied for different masses of
the Sun. It was found that the orbits of the planets were stable for values
greater than 0.33 M_Sun where M_Sun is the mass of the Sun and at lower masses
of the Sun (at about 0.8 M_Sun) only Venus, but for higher mass values (at
about 1.2 M_Sun) Earth and also Mars are located in both habitable zones.Comment: 8 page
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