10s 10--10s 10-1"s 10s 10s 10 s 100 s 3x 10° y 10° y 10° y TOE GUT 10" Gev 10" Gev 100 Gev 1 Gev Figure 34.9 The evolution of the universe from the Big Bang onward is intimately tied to the laws of physics, especially those of particle physics at the earliest stages. The universe is relativistic throughout its history. Theories of the unification of forces at high energies may be verified by their shaping of the universe and its evolution. 1dentical particles SUIQud 'suosog ypaA Spontaneous symmetry preaking. Inflation Leptons, quarks, W', Z°, photons Electroweak Loptons, hadrons, photons o Light nuclei Atoms Stars, protogalaxies, galaxies MON A o0L
10s 10--10s 10-1"s 10s 10s 10 s 100 s 3x 10° y 10° y 10° y TOE GUT 10" Gev 10" Gev 100 Gev 1 Gev Figure 34.9 The evolution of the universe from the Big Bang onward is intimately tied to the laws of physics, especially those of particle physics at the earliest stages. The universe is relativistic throughout its history. Theories of the unification of forces at high energies may be verified by their shaping of the universe and its evolution. 1dentical particles SUIQud 'suosog ypaA Spontaneous symmetry preaking. Inflation Leptons, quarks, W', Z°, photons Electroweak Loptons, hadrons, photons o Light nuclei Atoms Stars, protogalaxies, galaxies MON A o0L
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Question
If the smallest meaningful time interval is greater than zero, will the lines in Figure 34.9 ever meet?
![10s
10--10s
10-1"s 10s 10s 10 s 100 s 3x 10° y 10° y 10° y
TOE GUT
10" Gev
10" Gev
100 Gev
1 Gev
Figure 34.9 The evolution of the universe from the Big Bang onward is intimately tied to the laws of physics, especially those of particle
physics at the earliest stages. The universe is relativistic throughout its history. Theories of the unification of forces at high energies may be
verified by their shaping of the universe and its evolution.
1dentical particles
SUIQud 'suosog ypaA
Spontaneous symmetry
preaking. Inflation
Leptons, quarks, W', Z°, photons
Electroweak
Loptons, hadrons, photons o
Light nuclei
Atoms
Stars,
protogalaxies, galaxies
MON A o0L](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F14a5113b-c960-47eb-9359-51fb7a426b4d%2F0b528c03-3ea3-49d4-827a-71539a8fe69a%2Faq477ca_processed.png&w=3840&q=75)
Transcribed Image Text:10s
10--10s
10-1"s 10s 10s 10 s 100 s 3x 10° y 10° y 10° y
TOE GUT
10" Gev
10" Gev
100 Gev
1 Gev
Figure 34.9 The evolution of the universe from the Big Bang onward is intimately tied to the laws of physics, especially those of particle
physics at the earliest stages. The universe is relativistic throughout its history. Theories of the unification of forces at high energies may be
verified by their shaping of the universe and its evolution.
1dentical particles
SUIQud 'suosog ypaA
Spontaneous symmetry
preaking. Inflation
Leptons, quarks, W', Z°, photons
Electroweak
Loptons, hadrons, photons o
Light nuclei
Atoms
Stars,
protogalaxies, galaxies
MON A o0L
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