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Defence mechanism Quote by John D. Barrow

“When one looks at the numbers, the situation becomes even more perplexing. The effect of lambda grows steadily with respect to the familiar Newtonian force of gravity as the Universe gets bigger. If it is only recently becoming the dominant force, after billions of years of expansion of the…” quote by John D. Barrow
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““When one looks at the numbers, the situation becomes even more perplexing. The effect of lambda grows steadily with respect to the familiar Newtonian force of gravity as the Universe gets bigger. If it is only recently becoming the dominant force, after billions of years of expansion of the Universe, it must have started out enormously smaller than the Newtonian force. The distance of that final minimum energy level in Figure 8.14 from the zero line in order to explain the value of lambda inferred from the supernova observations is bizarre: roughly 10^-120 - that is, 1 divided by 10 followed by 119 zeros! This is the smallest number ever encountered in science. Why is it not zero? How can the minimum level be tuned so precisely? If it were 10 followed by just 117 zeros, then the galaxies could not form. Extraordinary fine tuning is needed to explain such extreme numbers. Extraordinary fine tuning is needed to explain such extreme numbers. And, if this were not bad enough, the vacuum seems to have its own defence mechanism to prevent us finding easy answers to this problem. Even if inflation does have some magical property which we have so far missed that would set the vacuum energy exactly to zero when inflation ends, it would not stay like that. As the Universe keeps on expanding and cooling it passes through several temperatures at which the breaking of a symmetry occurs in a potential landscape, rather like that which occurs in the example of the magnet that we saw at the beginning of the chapter. Every time this happens, a new contribution to the vaccum energy is liberated and contributes to a new lambda term that is always vastly bigger than our observation allows. And, by 'vastly bigger' here, we don't just mean that it is a few times bigger than the value inferred from observations, so that in the future some small correction to the calculations, or change in the trend of the observations, might make theory and observation fit hand in glove. We are talking about an overestimate by a factor of about 10 followed by 120 zeros! You can't get much more wrong than that.””

John D. Barrow

About This Quote

Source Lecture: Cosmology and the Fine‑Tuning Problem, 2002

The cosmological constant is astonishingly tiny yet non‑zero, raising deep questions about fine‑tuning and vacuum energy.

In simple terms: The universe’s energy is tiny but not zero.

Key Takeaway

Explore why fundamental constants are finely balanced.

Themes

science philosophy cosmology

Mood

curious thought‑provoking

Type

scientific inquisitive

When to use this quote

  • theoretical physics research
  • educational seminars
  • science communication

Key Concepts

fine‑tuning vacuum energy anthropic principle

Questions to Reflect On

  • Why does the universe have such a small lambda?
  • What alternative explanations exist for fine‑tuning?
A Different Perspective

Current theories may lack empirical testability.

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