A closer look at “Magnetic white dwarfs could exceed the Chandrasekhar limit, reshaping stellar evolution”, exactly as the source publishes it. A white dwarf is the dense, Earth-sized remnant left behind when a star like the sun exhausts its nuclear fuel and expels its outer layers. For a typical white dwarf, there is a firm upper mass limit of about 1.4 solar masses, known as the Chandrasekhar limit. Beyond this threshold, electron degeneracy pressure can no longer support the star against gravitational collapse, often leading to a Type Ia supernova.
However, new research suggests that strong magnetic fields could allow white dwarfs to grow beyond this limit, potentially changing our understanding of stellar death and supernova triggers. The study focuses on how intense magnetic fields alter the internal structure and stability of these remnants, providing extra support that counteracts gravity. For the complete material, the listing points back to the source inside the network.