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Can we go beyond the Chandrasekhar limit? New evidence from mathematical simulations

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The Chandrasekhar limit is defined as the maximum mass a white dwarf star can have, which is 1.44 times the mass of the Sun (M☉). According to theory, any star that exceeds this limit must collapse in...

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Research Matters
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Saturday, 17 October 2026, 11:43 am IST
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