The expansion of the universe is accelerating and scientists do not seem to agree on its rate. Why?
All observers agree that the expansion of the universe is accelerating (owing to “dark energy”, whose nature we do not understand, but which represents the energy of vacuum without matter). But there is a debate regarding the expansion rate. We can infer the expansion rate that the universe should have today based on the data we have on the cosmic microwave background [cmb is an elusive radiation that emanated at or after the birth of the universe and extrapolating its trajectory to present time is one of the ways to calculate the expansion of the universe]. But some observers who measure the actual expansion rate today argue that their measured value disagrees with the expected value at a statistically significant level.
Some scientists are calling for new physics to explain the discrepancies. What could this new physics be?
The discrepancy in expansion rates could indicate some new physics or some unexpected behaviour of dark matter and dark energy between the time when the cosmic microwave background was produced (400,000 years after the Big Bang) and today. We do not know if that is the case. [Scientists estimate that 27 per cent of the universe is dark matter which does not absorb, emit or reflect light and whose existence is inferred only from the gravitational effect it seems to exert on visible matter.]
How close are we from understanding the true nature of dark energy and dark matter?
Diese Geschichte stammt aus der February 16, 2020-Ausgabe von Down To Earth.
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Diese Geschichte stammt aus der February 16, 2020-Ausgabe von Down To Earth.
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