Stanford Root

Schedule

Stanford Root

Schedule

PHYSICS 362

The Early Universe

UNITS:3
GRADING:Letter or Credit/No Credit
LEVEL:Graduate
GER:—

Intended to complement PHYSICS PHYSICS 361, this course will cover the earlier period in cosmology up to and including nucleosynthesis. The focus will be on high energy, early universe physics. This includes topics such as inflation and reheating including generation of density perturbations and primordial gravitational waves, baryogenesis mechanisms, out of equilibrium particle production processes in the early universe e.g. both thermal and non-thermal production mechanisms for dark matter candidates such as WIMPs and axions, and production of the light nuclei and neutrinos. Techniques covered include for example out of equilibrium statistical mechanics such as the Boltzmann equation, and dynamics of scalar fields in the expanding universe. Other possible topics if time permits may include cosmological phase transitions and objects such as monopoles and primordial black holes. We will use quantum field theory, although it will hopefully be accessible for those without much background in that area.

Syllabus for selected term:
View Spring 2027 Syllabus

Sections

1 Term
Lecture 1Open
ID: 25161
0 / 35 enrolled
DAYS:Monday, Wednesday, Friday
TIME:1:30 PM – 2:50 PM
LOCATION:TBD
INSTRUCTOR:
Susskind, Leonard
3units

PHYSICS 362: The Early Universe

3 units · Letter or Credit/No Credit

Intended to complement PHYSICS 361, this course will cover the earlier period in cosmology up to and including nucleosynthesis. The focus will be on high energy, early universe physics. This includes topics such as inflation and reheating including generation of density perturbations and primordial gravitational waves, baryogenesis mechanisms, out of equilibrium particle production processes in the early universe e.g. both thermal and non-thermal production mechanisms for dark matter candidates such as WIMPs and axions, and production of the light nuclei and neutrinos. Techniques covered include for example out of equilibrium statistical mechanics such as the Boltzmann equation, and dynamics of scalar fields in the expanding universe. Other possible topics if time permits may include cosmological phase transitions and objects such as monopoles and primordial black holes. We will use quantum field theory, although it will hopefully be accessible for those without much background in that area.

Offered in Spring 2027 at Stanford University.

Spring 2027 sections

  • Lecture — Monday Wednesday Friday 1:30 PM – 2:50 PM — Susskind, Leonard (Graduate)

More PHYSICS courses

  • PHYSICS 330: Quantum Field Theory I
  • PHYSICS 331: Quantum Field Theory II
  • PHYSICS 332: Quantum Field Theory III
  • PHYSICS 352: Physics Beyond the Standard Model of Particle Physics
  • PHYSICS 360: Modern Astrophysics
  • PHYSICS 361: Cosmology and Extragalactic Astrophysics
  • PHYSICS 363: Radiative Processes in Astrophysics
  • PHYSICS 364: Black Holes
  • PHYSICS 367: Special Topics in Astrophysics: Astrophysical Data Analysis with the Rubin Observatory
  • PHYSICS 368: High Energy Astrophysics and Stellar Evolution
  • PHYSICS 372: Condensed Matter Theory I
  • PHYSICS 373: Condensed Matter Theory II

All PHYSICS courses · All departments