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Since 2012, we have initiated a new idea showing that the mass of highlymagnetized or modified Einstein's gravity induced white dwarfs could besignificantly super-Chandrasekhar with a different mass-limit. This discoveryhas several important consequences, including explanation of peculiar,over-luminous type Ia supernovae, soft gamma-ray repeaters and anomalous X-raypulsars without invoking extraordinarily strong, yet unobserved, magneticfields. It further argues for a possible second standard candle. Based onsimpler calculations, these white dwarfs are also shown to be much lessluminous than their standard counter-parts (of low magnetic fields). Thisdiscovery altogether initiates a new field of research.

Significantly super-Chandrasekhar limiting mass white dwarfs and their consequences