Researchers say they may have found a new way to describe how black holes behave under thermodynamics, addressing a problem that has remained unresolved for roughly 50 years. The work, highlighted by SciTechDaily, points to a revised measure of black hole entropy that could better match how these objects actually evolve.
The idea builds on Stephen Hawking’s black hole laws, which helped define how physicists think about energy, temperature and entropy in these extreme environments. According to the report, the new approach extends that framework rather than discarding it, with the goal of making it work for black holes that are not static.
That matters because real black holes are not perfectly unchanging systems. As the description suggests, they can grow when energy flows in, meaning their properties may shift over time. A thermodynamic model that accounts for ongoing change could give scientists a more realistic set of rules for studying black holes in the universe.
The research comes from Penn State and centers on redefining entropy in a way that can apply to black holes that keep evolving. If the approach holds up, it could sharpen a foundational area of theoretical physics and offer a fresh path for understanding how black holes store and transform information as they change.
