activity
20172026
most citedProspects for Galactic and stellar astrophysics with asteroseismology of giant stars in the Continuous Viewing Zones and beyond

50 citations · 270 across the 14 of their papers we have counts for

collaborators

14 papers

math.NA2026

Ordered Diffusion Kernels

Jack H. Soulsby, Andreas C. S. Jørgensen, Atiyo Ghosh +1

We introduce Ordered Diffusion Kernels (ODKs), a novel class of local kernels that can approximate the infinitesimal generator of an arbitrary Itô Stochastic Differential Equation…

astro-ph.SR2025

Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly III: stellar evolution at different metallicities

Yixiao Zhou, Jakob L. Rørsted, Achim Weiss +10

A major weakness in one-dimensional (1D) stellar structure and evolution modeling is the simplified treatment of convection, which leads to erroneous near-surface stratification an…

q-bio.QM2022

Data-driven spatio-temporal modelling of glioblastoma

Andreas Christ Sølvsten Jørgensen, Ciaran Scott Hill, Marc Sturrock +7

Mathematical oncology provides unique and invaluable insights into tumour growth on both the microscopic and macroscopic levels. This review presents state-of-the-art modelling tec…

astro-ph.GA2020★ 50 cited

Prospects for Galactic and stellar astrophysics with asteroseismology of giant stars in the Continuous Viewing Zones and beyond

J. Ted Mackereth, Andrea Miglio, Yvonne Elsworth +30

The NASA- mission presents a treasure trove for understanding the stars it observes and the Milky Way, in which they reside. We present a first look at the prospects for…

astro-ph.SR2020★ 24 cited

On the impact of the structural surface effect on global stellar properties and asteroseismic analyses

Andreas Christ Sølvsten Jørgensen, Josefina Montalbán, George C. Angelou +6

In a series of papers, we have recently demonstrated that it is possible to construct stellar structure models that robustly mimic the stratification of multi-dimensional radiative…

astro-ph.SR2020★ 32 cited

Investigating surface correction relations for RGB stars

Andreas Christ Sølvsten Jørgensen, Josefina Montalbán, Andrea Miglio +7

State-of-the-art stellar structure and evolution codes fail to adequately describe turbulent convection. For stars with convective envelopes, such as red giants, this leads to an i…

astro-ph.SR2019★ 36 cited

Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly II: Stellar Evolution and Asteroseismic Applications

Jakob Rørsted Mosumgaard, Andreas Christ Sølvsten Jørgensen, Achim Weiss +2

Models of stellar structure and evolution are an indispensable tool in astrophysics, yet they are known to incorrectly reproduce the outer convective layers of stars. In the first…

astro-ph.SR2019★ 10 cited

Bayesian inference of stellar parameters based on 1D stellar models coupled with 3D envelopes

Andreas Christ Sølvsten Jørgensen, George C. Angelou

Stellar models utilising one-dimensional (1D), heuristic theories of convection fail to adequately describe the energy transport in superadiabatic layers. The improper modelling le…

astro-ph.SR2019★ 20 cited

Overcoming the structural surface effect with a realistic treatment of turbulent convection in 1D stellar models

Andreas Christ Sølvsten Jørgensen, Achim Weiss

State-of-the-art one-dimensional (1D) stellar evolution codes rely on simplifying assumptions, such as mixing length theory, in order to describe superadiabatic convection. As a re…

astro-ph.SR2019★ 18 cited

Mending the structural surface effect of 1D stellar structure models with non-solar metallicities based on interpolated 3D envelopes

Andreas Christ Sølvsten Jørgensen, Achim Weiss, George Angelou +1

1D stellar evolution codes employ rudimentary treatments of turbulent convection. For stars with convective envelopes, this leads to systematic errors in the predicted oscillation…

astro-ph.SR2018★ 16 cited

Addressing the acoustic tachocline anomaly and the lithium depletion problem at the same time

Andreas Christ Sølvsten Jørgensen, Achim Weiss

Current standard solar models neither account properly for the photospheric lithium abundance nor reproduce the inferred solar sound speed profile. Diffusive overshooting at the ba…

astro-ph.SR2018★ 5 cited

A Semi-Analytical Computation of the Theoretical Uncertainties of the Solar Neutrino Flux

Andreas Christ Sølvsten Jørgensen, Jørgen Christensen-Dalsgaard

We present a comparison between Monte Carlo simulations and a semi-analytical approach that reproduces the theoretical probability distribution functions of the solar neutrino flux…

astro-ph.SR2018★ 35 cited

Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly I: A New Standard Solar Model

Andreas Christ Sølvsten Jørgensen, Jakob Rørsted Mosumgaard, Achim Weiss +2

Standard 1D stellar evolution models do not correctly reproduce the structure of the outermost layers of stars with convective envelopes. This has been a long-standing problem in s…

astro-ph.SR2017★ 24 cited

Theoretical oscillation frequencies for solar-type dwarfs from stellar models with -atmospheres

Andreas Christ Sølvsten Jørgensen, Achim Weiss, Jakob Rørsted Mosumgaard +2

We present a new method for replacing the outermost layers of stellar models with interpolated atmospheres based on results from 3D simulations, in order to correct for structural…