Recent theoretical research suggests that the universe's end might occur sooner than previously anticipated. Traditionally, black holes were believed to evaporate over immense timescales via Hawking radiation. However, new studies indicate that even neutron stars could decay through similar mechanisms, potentially accelerating cosmic demise. This challenges existing models of cosmic longevity and underscores the need for further investigation into quantum gravitational effects on dense astrophysical objects. Observations of such phenomena could provide deeper insights into the universe's ultimate fate.
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