Article
Astronomy & Astrophysics
R. O. Chametla, O. Chrenko
Summary: This study investigates the gravitational interaction between planets and pressure bumps in a gas-dust protoplanetary disc, exploring the changes in disc structure and planet migration. Through simulations, it is found that pressure bumps quickly merge into a single, wide bump, accompanied by the formation of vortices and density waves. The interaction between spiral waves generated by the vortex and the planet's waves leads to slower migration and increased orbital eccentricities for the planets.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Cristiano Longarini, Giuseppe Lodato, Giuseppe Bertin, Philip J. Armitage
Summary: Recent observations indicate that planet formation occurs in young systems, even when the protostar is still embedded in the molecular cloud and the accretion disc is massive. The dynamical evolution of the disc in such environments is determined by the crucial role of self-gravity and gravitational instability. This study investigates the role of drag force in self-gravitating discs for the formation of planetesimals during early protoplanetary stages, finding that the stability threshold depends on the local dust-to-gas density ratio, dust relative temperature, and relevant Stokes number.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Shangjia Zhang, Zhaohuan Zhu, Mingon Kang
Summary: We developed a neural network model called PGNets to infer planet mass accurately and quickly from radio dust continuum images. By utilizing substructures induced by young planets in protoplanetary discs, we were able to infer properties of potential young planets. Our approach is more efficient and preserves asymmetric features in discs compared to previous simulation methods.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Jamie F. Townsend, Shu-ichiro Inutsuka, Laszlo Konozsy, Karl W. Jenkins
Summary: This work assesses the dissipative properties of high-order numerical methods for relativistic hydrodynamics and investigates the numerical dissipation of high-order shock-wave capturing schemes. It provides insights into the relationship between the numerical dissipation and grid resolution, and highlights the presence of numerical artifacts in the simulation of relativistic Kelvin-Helmholtz instability. The study suggests that high-order schemes may offer advantages in terms of accuracy and computational cost compared to low-order schemes, particularly on coarser grid resolutions in the presence of physical viscosity.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
H. Andresen, R. Glas, H-Th Janka
Summary: The study compares gravitational-wave signals from core-collapse supernova simulations using different progenitors, finding that both numerical resolution and neutrino transport methods have significant impacts on the signals. However, resolution-dependent differences in the hydrodynamic behavior of models have a greater impact on the signals than consequences of different transport methods. Increasing resolution can reduce discrepancies between models with different neutrino transport.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
D. Tarczay-Nehez, K. Rozgonyi, Zs Regaly
Summary: Gas-rich dusty circumstellar discs observed around young stellar objects are believed to be the birthplace of planets and planetary systems. Recent observations revealed the presence of large-scale brightness asymmetries in transitional protoplanetary discs. Theoretical studies suggest that these brightness asymmetries could be caused by large-scale anticyclonic vortices triggered at the edges of the dead zone.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Kevin Chan, Sijme-Jan Paardekooper
Summary: Recent observations have shown the importance of including dust in modeling protoplanetary discs. However, simulating the interactions between dust and gas separately poses computational difficulties. This study proposes a single-fluid approach that incorporates the terminal velocity approximation to overcome these difficulties. Comparing this approach with a multifluid model, differences in dust density distribution are found for different planet masses. The terminal velocity approximation proves to be a valuable tool but caution is needed when dealing with shocks.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Nicolas P. Cimerman, Roman R. Rafikov
Summary: Young planets embedded in protoplanetary discs (PPDs) create gaps due to excitation of spiral density waves, resulting in the emergence of observable vortices at the gap edges via the Rossby wave instability (RWI). We study the time-scales for the development of vortices driven by low-mass planets in low-viscosity discs. By employing a semi-analytical theory, we predict the vortensity evolution near the planet and derive the radial profile of the planet-induced gap. We also analyze the linear stability of the gap edges against the RWI and present formulae for the time-scales of unstable modes and fully developed vortices.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Alexandros Ziampras, Richard P. Nelson, Roman R. Rafikov
Summary: ALMA observations of protoplanetary discs in dust continuum emission show various annular structures. These features are believed to be caused by embedded planets, as supported by hydrodynamical models. A new study compares previous models with local cooling to new models with cooling in the vertical direction and radiative diffusion in the disc plane, finding significant differences in how the disc responds to induced spiral waves and that the new models better reproduce observations. The study concludes that the treatment of radiation transport is crucial in interpreting ALMA observations using the planet-disc interaction scenario.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)
Article
Astronomy & Astrophysics
Sijme-Jan Paardekooper, Colin P. McNally, Francesco Lovascio
Summary: The paper presents a new approach to streaming instabilities, allowing for more accurate solutions to linear stability problems with lower computational costs. It also demonstrates techniques for reducing integral equations to complex polynomials and counting roots of dispersion relations inside contours. The methods described can reproduce and surpass the accuracy of previous results in the literature.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Tirso Marin-Gilabert, Milena Valentini, Ulrich P. Steinwandel, Klaus Dolag
Summary: The Kelvin-Helmholtz instability (KHI) is used as a test case to evaluate the accuracy of smoothed particle hydrodynamics (SPH) and meshless finite mass (MFM) methods. Results show that SPH is able to accurately reproduce the growth of KHI and recover the threshold level of physical viscosity required to fully suppress the instability.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Noemi Schaffer, Anders Johansen, Michiel Lambrechts
Summary: The streaming instability provides an efficient method to overcome growth barriers in early planet formation. Research shows that various factors do not significantly impact the efficiency and timing of filament formation in multispecies streaming instability. Additionally, the initial metallicity has a similar effect on critical metallicity values for filament formation under different conditions.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
N. Ndugu, O. P. Abedigamba, G. Andama
Summary: This study investigates how protoplanetary discs in stellar clusters are affected by background heating, disc truncation, and photoevaporation, and how disc truncation impacts planet formation. The findings show that disc truncation reduces disc mass and decreases the occurrence rates of gas giant planets, with hot Jupiters being more frequent than cold Jupiters.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Astronomy & Astrophysics
Dmitry A. Badjin, Semyon Glazyrin
Summary: This study investigates the influence of fluctuating magnetic fields on the structure formation and instabilities of radiatively cooling blast waves through analytical estimations and multidimensional simulations, highlighting the importance of thermal instability and its interaction with interstellar fields. It also explores the amplification of bending fluctuations by non-linear Vishniac instability in SNR regions, with instabilities driven by counter-directional pressure and density gradients limited to specific environments. Additionally, recommendations are made for numerical simulation techniques.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Vincent G. A. Boening, Aaron C. Birch, Laurent Gizon, Thomas L. Duvall
Summary: The research aimed to evaluate the validity of the existing upper limit of solar convective flow amplitudes at a depth of 0.96 solar radii using time-distance helioseismology and simplifying assumptions.
The results showed that the current procedure provides the correct order of magnitude of flow estimates for given flow fields, but may underestimate flow amplitudes at the largest scales by about two times.
It was concluded that the estimate obtained is indeed an upper limit when considering the scale dependence of the signal-to-noise ratio and the dependence of measurements on direction in Fourier space.
ASTRONOMY & ASTROPHYSICS
(2021)
Article
Astronomy & Astrophysics
Min-Kai Lin
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2019)
Article
Astronomy & Astrophysics
He-Feng Hsieh, Min-Kai Lin
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2020)
Article
Astronomy & Astrophysics
Jiaqing Bi, Min-Kai Lin, Ruobing Dong
Summary: Dust gaps and rings are commonly found in bright protoplanetary disks, with some sharp dust rings indicating settlement of sub-millimeter-sized dust grains. Planets massive enough to open gas gaps can stir small dust grains to high disk elevations, attributed to meridional gas flows induced by the planet. Three-dimensional simulations are crucial for obtaining the vertical distribution of sub-millimeter-sized grains around gas gaps opened by massive planets.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Michael Hammer, Min-Kai Lin, Kaitlin M. Kratter, Paola Pinilla
Summary: Studies have shown that low-mass planets in some protoplanetary discs can trigger multiple generations of vortices leading to dust asymmetries, while vortices with H/r = 0.08 exhibit longer survival periods. These results help explain certain observed phenomena in celestial bodies.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
Can Cui, Min-Kai Lin
Summary: The study conducted linear analyses of the VSI in magnetized discs with Ohmic resistivity, finding that magnetism has a stabilizing effect to dampen the VSI, with surface modes easier to vanish compared to body modes as magnetization increases. When considering resistivity, the MRI grows more efficiently at small radial wavenumbers in surface layers of PPDs, while the VSI dominates over the MRI under certain conditions.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2021)
Article
Astronomy & Astrophysics
M. Lehmann, M-K Lin
Summary: The standard core accretion model for planetesimal formation in protoplanetary discs faces challenges due to the vertical settling of dust against turbulent stirring. The vertical shear instability (VSI), sustaining turbulence in the outer regions of PPDs, drives the formation of long-lived vortices that can collect dust and potentially trigger the streaming instability (SI). The presence of pressure bumps in the discs can lead to the formation of dusty vortices with high dust-to-gas ratios, impacting the vertical mass flow profile and alpha viscosity values.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Sayantan Auddy, Ramit Dey, Min-Kai Lin, Cassandra Hall
Summary: This study introduces the architecture of DPNNet-2.0, a neural network model designed to predict exoplanet masses directly from simulated images of protoplanetary disks. The model combines a convolutional neural network (CNN, specifically ResNet50) and a multilayer perceptron to process both image data and disk parameters, allowing for training using images directly and considering hydrodynamic parameters from simulations. This work lays the foundation for using computer vision techniques to extract exoplanet masses from observations of planetary gaps in dust density maps.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Min-Kai Lin, Chun-Yen Hsu
Summary: The streaming instability can remain effective inside dust-trapping pressure bumps in accreting disks, and can be stabilized by magnetic perturbations. Dust feedback can dampen the magneto-rotational instability, while Alfven waves can be destabilized by dust-gas drift, but this requires nearly ideal conditions.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Sayantan Auddy, Ramit Dey, Min-Kai Lin, Daniel Carrera, Jacob B. Simon
Summary: In this study, a Bayesian deep-learning network, DPNNet-Bayesian, is introduced to predict planet mass from disk gaps and provide uncertainties associated with the prediction. The unique feature of this approach is its ability to distinguish between uncertainty related to the deep-learning architecture and uncertainty due to measurement noise in the input data. The results show that the network's predictions are comparable to those from other studies based on specialized simulations.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Chun-Yen Hsu, Min-Kai Lin
Summary: The streaming instability (SI) is a promising mechanism for triggering planetesimal formation. Understanding its operation in protoplanetary disks (PPDs) is crucial. In this study, we present the first nonlinear simulations of the azimuthal drift SI (AdSI) and find that it can drive turbulence and the formation of dust filaments, potentially increasing local dust densities.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Pin-Gao Gu, Che-Yu Chen, Emma Shen, Chien-Chang Yen, Min-Kai Lin
Summary: In this study, we investigate the drag instability in 1D isothermal C-shocks using nonideal magnetohydrodynamic simulations. The results confirm the presence of the drag instability and show that the simulated perturbations match the linear analysis, indicating the validity of the drag instability.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
Jiaqing Bi, Min-Kai Lin, Ruobing Dong
Summary: By using three-dimensional dust-and-gas disk simulations, we find that gap-opening planets can widen dust rings by perturbing the pressure bump, even when the dust-to-gas ratio is close to unity and the dust back-reaction is considered. We quantitatively demonstrate the planet-related widening effect on dust rings using diffusion-advection theory, and propose a generalized criterion for determining the equilibrium width of dust rings in three-dimensional disk models. We also suggest estimating the ring width using the gas turbulent viscosity alpha (turb), with caution regarding the Schmidt number being greater than unity.
ASTROPHYSICAL JOURNAL
(2023)
Article
Astronomy & Astrophysics
Min-Kai Lin
Summary: The research suggests that the streaming instability between dust and gas in protoplanetary disks can be captured through vertically global linear stability analyses, driven primarily by the vertical gradient in the rotation velocity of the dust-gas mixture and requiring partial coupling. This helps in understanding the mechanism of planetesimal formation.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Sayantan Auddy, Min-Kai Lin
ASTROPHYSICAL JOURNAL
(2020)
Article
Astronomy & Astrophysics
Kan Chen, Min-Kai Lin
ASTROPHYSICAL JOURNAL
(2020)