The evidence is that Dark Energy is responsible for the rate of expansion of the universe. The name makes it sound like a spooky force, but, in fact, it’s the cosmological constant, Λ, that Einstein added to his theory of gravity back in 1917. Einstein regretted it, but we have been forced to put Λ back in the theory to fit the evidence. There is theoretical backing of a sort from quantum theory, which also predicts the presence of a cosmological constant, Λ, but with a value that is far off what we need. Finding a way to unify the predicted value of Λ by quantum theory, and the observed value of Λ from the expanding universe, would be a great discovery. But even the most sophisticated theory is constrained by observational evidence, which always will be imperfect and incomplete, and hence our theories always will be an approximation, never an account of ultimate reality, argues James Peebles.
The standard theory for explaining the expansion of the universe from a hot dense state requires the presence of Einstein's cosmological constant. The usual symbol for it is the Greek Λ, and today Λ is more commonly known as Dark Energy. Maybe the name is an improvement, but nothing else has changed. Our well-tested theory of the expanding universe needs something that acts like Λ, but we still do not know how this Λ fits in with our standard physics.
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Our model of the universe has been falsified
By Pavel Kroupa
It has been known since the 1930s that quantum physics naturally predicts the presence of a cosmological constant, Λ, but the predicted value is absurdly large. A quarter of a century ago, when we had much less evidence of how the universe is evolving, we tended to say that since the quantum estimate of Λ is clearly wrong, the only natural alternative is that Λ is zero. Einstein would have agreed with this hopeful argument; he regretted adding this term to his new theory of gravity, the general theory of relativity. But the accumulated evidence now makes a compelling case that we must learn to live with Λ, Dark Energy.
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