Search Results - "Simon, Jacob"
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1
The Streaming Instability Cannot Form Planetesimals from Millimeter-size Grains in Pressure Bumps
Published in Astrophysical journal. Letters (01-07-2022)“…Abstract We present evidence that it is unlikely that the streaming instability (SI) can form planetesimals from millimeter grains inside axisymmetric pressure…”
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THE MASS AND SIZE DISTRIBUTION OF PLANETESIMALS FORMED BY THE STREAMING INSTABILITY. I. THE ROLE OF SELF-GRAVITY
Published in The Astrophysical journal (01-05-2016)“…ABSTRACT We study the formation of planetesimals in protoplanetary disks from the gravitational collapse of solid over-densities generated via the streaming…”
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3
Monoaminergic Neuromodulation of Sensory Processing
Published in Frontiers in neural circuits (10-07-2018)“…All neuronal circuits are subject to neuromodulation. Modulatory effects on neuronal processing and resulting behavioral changes are most commonly reported for…”
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Complementary Roles for Primate Frontal and Parietal Cortex in Guarding Working Memory from Distractor Stimuli
Published in Neuron (Cambridge, Mass.) (02-07-2014)“…Prefrontal cortex (PFC) and posterior parietal cortex are important for maintaining behaviorally relevant information in working memory. Here, we challenge the…”
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5
Demographics of Planetesimals Formed by the Streaming Instability
Published in The Astrophysical journal (01-11-2019)“…The streaming instability (SI) is a mechanism to aerodynamically concentrate solids in protoplanetary disks and facilitate the formation of planetesimals…”
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Turbulence in the TW Hya Disk
Published in The Astrophysical journal (01-04-2018)“…Turbulence is a fundamental parameter in models of grain growth during the early stages of planet formation. As such, observational constraints on its…”
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Strongly magnetized accretion discs: structure and accretion from global magnetohydrodynamic simulations
Published in Monthly notices of the Royal Astronomical Society (01-02-2020)“…ABSTRACT We use global magnetohydrodynamic simulations to study the influence of net vertical magnetic fields on the structure of geometrically thin…”
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Accretion disc dynamo activity in local simulations spanning weak-to-strong net vertical magnetic flux regimes
Published in Monthly notices of the Royal Astronomical Society (21-03-2016)“…Strongly magnetized accretion discs around black holes have attractive features that may explain enigmatic aspects of X-ray binary behaviour. The structure and…”
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Magnetically driven accretion in protoplanetary discs
Published in Monthly notices of the Royal Astronomical Society (21-11-2015)“…We characterize magnetically driven accretion at radii between 1 and 100 au in protoplanetary discs, using a series of local non-ideal magnetohydrodynamic…”
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10
Turbulence Regulates the Rate of Planetesimal Formation via Gravitational Collapse
Published in The Astrophysical journal (01-12-2020)“…We study how the interaction between the streaming instability (SI) and intrinsic gas-phase turbulence affects planetesimal formation via gravitational…”
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The Mass and Size Distribution of Planetesimals Formed by the Streaming Instability. II. The Effect of the Radial Gas Pressure Gradient
Published in The Astrophysical journal (04-10-2019)“…The streaming instability concentrates solid particles in protoplanetary disks, leading to gravitational collapse into planetesimals. Despite its key role in…”
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12
On the Numerical Robustness of the Streaming Instability: Particle Concentration and Gas Dynamics in Protoplanetary Disks
Published in The Astrophysical journal (20-07-2018)“…The streaming instability (SI) is a mechanism to concentrate solids in protoplanetary disks. Nonlinear particle clumping from the SI can trigger gravitational…”
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A Three-dimensional View of Turbulence: Constraints on Turbulent Motions in the HD 163296 Protoplanetary Disk Using DCO
Published in The Astrophysical journal (10-07-2017)“…Gas kinematics are an important part of the planet formation process. Turbulence influences planetesimal growth and migration from the scale of submicron dust…”
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14
Emergent mesoscale phenomena in magnetized accretion disc turbulence
Published in Monthly notices of the Royal Astronomical Society (01-05-2012)“…We study how the structure and variability of magnetohydrodynamic (MHD) turbulence in accretion discs converge with domain size. Our results are based on a…”
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15
Measuring Turbulent Motion in Planet-forming Disks with ALMA: A Detection around DM Tau and Nondetections around MWC 480 and V4046 Sgr
Published in The Astrophysical journal (01-06-2020)“…Turbulence is a crucial factor in many models of planet formation, but it has only been directly constrained among a small number of planet-forming disks…”
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Origin of Weak Turbulence in the Outer Regions of Protoplanetary Disks
Published in The Astrophysical journal (20-09-2018)“…The mechanism behind angular momentum transport in protoplanetary disks, and whether this transport is turbulent in nature, is a fundamental issue in planet…”
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TURBULENCE IN THE OUTER REGIONS OF PROTOPLANETARY DISKS. II. STRONG ACCRETION DRIVEN BY A VERTICAL MAGNETIC FIELD
Published in The Astrophysical journal (20-09-2013)“…We carry out a series of local, vertically stratified shearing box simulations of protoplanetary disks that include ambipolar diffusion and a net vertical…”
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18
Relating magnitudes: the brain's code for proportions
Published in Trends in cognitive sciences (01-03-2012)“…Whereas much is known about how we categorize and reason based on absolute quantity, data exploring ratios of quantities, as in proportions and fractions, are…”
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19
Dopamine Receptors Differentially Enhance Rule Coding in Primate Prefrontal Cortex Neurons
Published in Neuron (Cambridge, Mass.) (17-12-2014)“…Flexibly applying abstract rules is a hallmark feature of executive functioning represented by prefrontal cortex (PFC) neurons. Prefrontal networks are…”
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EFFICIENCY OF PARTICLE TRAPPING IN THE OUTER REGIONS OF PROTOPLANETARY DISKS
Published in The Astrophysical journal (20-03-2014)“…We investigate the strength of axisymmetric local pressure maxima (zonal flows) in the outer regions of protoplanetary disks, where ambipolar diffusion reduces…”
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