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Inflation ASTR/PHYS 4080: Intro to Cosmology Week 9 ASTR/PHYS - PowerPoint PPT Presentation

Inflation ASTR/PHYS 4080: Intro to Cosmology Week 9 ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 1 Successes of the Hot Big Bang Model Consists of: General relativity Cosmological principle Known


  1. Inflation ASTR/PHYS 4080: Intro to Cosmology Week 9 ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 1

  2. Successes of the Hot Big Bang Model Consists of: • General relativity • Cosmological principle • Known atomic/nuclear/particle physics • successful theory supported by observation • clear understanding of what happened from Explains: t~1s to t~13.7Gyr ~4x10 17 s • dark night sky • may speculate what happened as early as • Hubble expansion Planck time (t~10 -43 s) based on known physics • age of the universe • CMB (existence + blackbody spectrum) • light element abundances • … much more! ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 2

  3. “Problems” with the Hot Big Bang Model Unable to explain • baryon asymmetry (Extension of particle physics) • horizon problem (Why so homogeneous) • flatness problem (Why so flat) • monopole problem (Why so rare) • small scale inhomogeneities (What gives rise to it? the origin of irregularities) • … probably so more stu ff ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 3

  4. Lack a Complete Theory: these are clues… The problems and the need for extension • NOT a demonstrable failure to fit observation by standard model • BUT its incomplete explanatory power • or perhaps unsatisfying Analogy - particle standard model • successful, but unable to explain particle mass spectrum, dark matter, dark energy, ... • extension(s): SUSY, String Theory, TOE, ... Extension to standard big bang model: INFLATION ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 4

  5. Flatness Problem (Why is the curvature so fine-tuned?) Observed: Friedmann Equation: ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 5

  6. Horizon Problem (How can the universe be homogeneous and isotropic on the largest scales?) ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 6

  7. Monopole Problem (Where are all the topological defects, like magnetic monopoles and cosmic strings?) At larger energies, “fundamental” forces unify or equivalently, as energy decreases a phase transition occurs causing a break in symmetry ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 7

  8. Topological Defects Monopoles are predicted by GUTs, expect 1 per horizon zone (causally-connected volumes when the phase transition occurred) ASTR/PHYS 4080: Introduction to Cosmology Spring 2018: Week 12 8

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