标题： 显著超钱德拉塞卡极限质量的白矮星及其后果 显示英文标题

标题： Significantly super-Chandrasekhar limiting mass white dwarfs and their consequences

摘要： 自2012年以来，我们提出了一种新思路，表明高度磁化或修改的爱因斯坦引力诱导的白矮星的质量可能显著超过钱德拉塞卡质量极限，具有不同的质量限制。 这一发现有几个重要的后果，包括解释了特殊的超明亮Ia型超新星、软伽马射线重复暴和异常X射线脉冲星，而无需引入极其强但尚未观测到的磁场。 它进一步支持了可能存在第二个标准烛光的可能性。 基于更简单的计算，这些白矮星也被证明比低磁场的标准对应物要暗得多。 这一发现共同开启了一个新的研究领域。 显示英文摘要

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