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Yoshida Lab
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A theoretical astrophysics lab that investigates the equilibrium configurations and properties of neutron stars with magnetic fields.

AboutAbout the lab
Modeling magnetized neutron stars through theory.
The Yoshida Lab studies magnetized neutron stars from the standpoint of theoretical astrophysics.
Neutron stars are considered to be central objects in high-energy astrophysical phenomena, but our understanding of their internal magnetic fields remains insufficient, in both observation and theory.
The lab develops formulations and numerical codes to efficiently compute theoretically self-consistent models of magnetized neutron stars within the framework of general relativity.
Key terms
- Neutron star
- One of the objects considered to be central to high-energy astrophysical phenomena. Our understanding of its internal structure, especially its magnetic field, is still insufficient.
- Magnetized neutron star
- A neutron star accompanied by a magnetic field. This lab studies its equilibrium configurations using the theory of general relativity.
- Equilibrium solution
- A solution of the equations that describes a state in which a star is in balance and keeps its shape. It is the starting point for studying stability.
ResearchResearch themes
Our understanding of the internal structure of neutron stars, and especially of their internal magnetic fields, is still insufficient in both observation and theory. The lab develops formulations and numerical codes to efficiently compute models of magnetized neutron stars within the framework of general relativity, with the aim of clarifying their basic properties.
View More ↗MembersFaculty
- Assistant ProfessorShijun Yoshida
VoicesStudent voices
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Report an errorAbout the images
The top and research theme images are illustrative and were not taken at the lab. They are cropped from Wikimedia Commons images.
- Top image: “The Star with a Secret Identity” X-ray: NASA/CXC/Huntingdon Inst. for X-ray Astronomy/G.Garmire, Optical: ESO/VLT / Public domain (cropped)
- Equilibrium Configurations of Magnetized Neutron Stars in General Relativity: “Artist’s impression of the magnetar in the star cluster Westerlund 1” ESO/L. Calçada / CC BY 4.0 (cropped)
- Related lab (Toma Lab): “Artist’s illustration of galaxy with jets from a supermassive black hole” ESA/Hubble, L. Calçada (ESO) / CC BY 4.0 (cropped)
- Related lab (Fujibayashi Lab): “Vela Supernova Remnant - Noirlab2406a” CTIO/NOIRLab/DOE/NSF/AURA Image Processing: T.A. Rector (University of Alaska Anchorage/NSF’s NOIRLab), M. Zamani & D. de Martin (NSF’s NOIRLab) / CC BY 4.0 (cropped)
- Related lab (Noda Lab): “Chandra X-Ray Observatory (noirlab2427c)” NASA/CXC & J.Vaughan / CC BY 4.0 (cropped)
- Related lab (Kimura Lab): “Anatomy of an Active Galactic Nucleus (SVS14922 - Jet illustrated Loop v01 00001 print)” NASA's Scientific Visualization Studio - NASA’s Goddard Space Flight Center’s Conceptual Image Lab / Public domain (cropped)
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