A page on LabLog, a review site (not the lab's official page)
Yamada Lab
Machine-translated · View original
A theoretical lab that unravels the mysteries of supernovae and black holes.

AboutAbout the lab
Theoretical astrophysics probing how stars end their lives
The Yamada Lab theoretically studies what happens at the end of a star's life.
The lab investigates the mechanism of gravitational collapse, in which the core of a star far more massive than the Sun collapses under its own gravity at the end of its evolution.
Using models and simulations, the lab studies the resulting supernova explosions and the formation of neutron stars and black holes.
The lab also works on high-energy phenomena in the universe, such as gamma-ray bursts and magnetars, which are neutron stars with extremely strong magnetic fields.
Key terms
- Gravitational collapse
- A phenomenon in which a star can no longer support its own weight and its core collapses rapidly
- Neutron star
- An extremely dense object formed after a star undergoes gravitational collapse
- Magnetar
- A special type of neutron star with an extremely strong magnetic field
NewsLab news
View More ↗ResearchResearch themes
The lab theoretically studies the process that begins with gravitational collapse, which occurs at the end of the evolution of stars far more massive than the Sun, and leads to supernova explosions and the formation of neutron stars and black holes. It also works to clarify the theoretical mechanisms of high-energy phenomena in the universe.
*Illustrative imageSupernova explosions and neutron star formation
Very massive stars undergo gravitational collapse at the end of their evolution, when the core collapses under its own gravity. The lab uses models and simulations to study how this leads to supernova explosions and neutron star formation.
*Illustrative imageTheory of black hole formation
When gravitational collapse forms a black hole, it cannot be seen in light, but it can still be observed through neutrinos and gravitational waves. The lab theoretically calculates the signals emitted during formation in order to probe the internal state of the star.
*Illustrative imageGamma-ray bursts and binary systems
Black hole formation can be accompanied by gamma-ray bursts. The lab studies what kinds of stars produce gamma-ray bursts, and how supernova explosions in binary systems affect their surroundings.
*Illustrative imagePhysics of magnetars
To understand the giant flares produced by magnetars, which are neutron stars with extremely strong magnetic fields, the lab studies from first principles the quantum-theoretical physical processes that take place under strong magnetic fields.
MembersFaculty
The members of the Yamada Lab consist of faculty, researchers, and doctoral, master's, and undergraduate students.
- ProfessorShoichi Yamada
VoicesStudent voices
Compiled from answers by students who were in the lab. Ratings and reviews reflect individual students' experiences, not the lab's official views.
Students who take part in an interview may receive a thank-you gift worth ¥1,000, regardless of what they say.
On a 4-point scale, ● marks where students' answers fall
Who is this lab for?
What's great about this lab?
What did you learn after joining?
What's the vibe, and what is the professor like?
Where do graduates go?
RelatedLabs similar to Yamada Lab
Tsujikawa LabSchool of Advanced Science and Engineering, Department of PhysicsAstrophysics, Theory of Relativity
Inoe LabSchool of Advanced Science and Engineering, Department of PhysicsObservational space astrophysics
Takano LabSchool of Advanced Science and Engineering, Department of PhysicsTheoretical nuclear physics
Takano LabSchool of Advanced Science and Engineering, Department of PhysicsBiophysicsThe information on this page is compiled by the LabLog team from the lab's public information and interviews. For corrections or removal requests, please contact LabLog, not the lab.
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. Cropped CC BY-SA images are provided under the same CC BY-SA license as the original (version shown on each line).
- Top image: “Keplers supernova” NASA/ESA/JHU/R.Sankrit & W.Blair / Public domain (cropped)
- Supernova explosions and neutron star formation: “Red onion cross section 04” Amada44 / CC BY-SA 3.0 (cropped)
- Theory of black hole formation: “Illustration of an Isolated Black Hole ( )” NASA Hubble / Public domain (cropped)
- Gamma-ray bursts and binary systems: “Artist’s impression of a gamma-ray burst shining through two young galaxies in the early Universe” ESO/L. Calçada / CC BY 4.0 (cropped)
- Physics of magnetars: “Artist’s impression of the magnetar in the star cluster Westerlund 1” ESO/L. Calçada / CC BY 4.0 (cropped)
- Related lab (辻川研究室): “Illustris Dark Matter and Gas” Illustris Collaboration / CC BY-SA 4.0 (cropped)
- Related lab (井上研究室): “Webb's First Deep Field” NASA, ESA, CSA, and STScI / Public domain (cropped)
- Related lab (鷹野研究室): “Crab Nebula” NASA, ESA, J. Hester and A. Loll (Arizona State University) / Public domain (cropped)
- Related lab (高野研究室): “Crowded cytosol” TimVickers / Public domain (cropped)
About LabLog
LabLog is a lab review app for students only. Student members at each university interview students in labs and publish what they say. Student voices can only be read by students who sign up with a university email address. Operated by bestiee Inc.
Learn more about LabLog ↗Search engines and AI may reference the basic lab info and rating summaries on this page and the description of LabLog. Student voices are for student members only. Automated collection by programs (scraping, or input to or training of AI) is prohibited under Article 8 of the Terms of Service. If you need data for research or analysis, please contact us.