
An effect where primordial black holes retain information, slowing evaporation and influencing oscillations.The memory burden effect is a proposed phenomenon in which a black hole's evaporation is slowed down because the black hole retains information about its initial state. This effect is particularly relevant for primordial black holes, which are hypothesized to have formed in the early universe. The memory burden could influence their evaporation rate and even their role as dark matter candidates.
The concept is relatively recent, emerging from studies on black hole information paradox and quantum gravity. It has been explored in the context of primordial black holes and their potential to explain dark matter, with key contributions from researchers like Dvali and others in the late 2010s and 2020s.
When a black hole evaporates via Hawking radiation, it loses mass and eventually disappears. The memory burden effect suggests that as the black hole emits radiation, it also encodes information about its initial configuration. This information storage creates a 'burden' that resists further evaporation, effectively slowing the process. This could lead to longer-lived black holes and alter their observable signatures, such as gravitational wave emissions.
The memory burden effect is used in theoretical models to predict the abundance and mass distribution of primordial black holes, which could be detected through gravitational waves or microlensing events.
The memory burden effect might explain why primordial black holes have not yet been observed to evaporate, even though they should have by now if they were light enough.











