Number of times the word "universe" appears on this lecture notes by Daniel Baumann. Blog post about this: The hoax called "cosmology"
| Page | Quote | Possible meaning |
|---|---|---|
| [64-01] | It describes a wide range of phenomena, from falling apples and planetary orbits to the expansion of the universe and black holes. | Cosmos |
| [71-02] | This describes an exponentially expanding universe | Cosmos |
| [84-03] | to exist for real black holes in the Universe | Cosmos |
| [94-04] | the equations governing the evolution of the entire Universe. | universe as a whole |
| [94-05] | the coarse-grained properties of the Universe | Cosmos |
| [94-06] | the Universe looks homogeneous | Cosmos |
| [94-07] | This leads to a simple mathematical description of the Universe | Cosmos |
| [94-08] | The spatial homogeneity and isotropy of the Universe | Cosmos |
| [94-09] | which describes the expansion of the universe. | Cosmos |
| [94-10] | scale factor is related to the matter content of the Universe. | Cosmos |
| [94-11] | The spacetime of the Universe | Cosmos |
| [95-12] | Notice that the symmetries of the Universe | Cosmos |
| [97-13] | On large scales, the expansion of the Universe | Cosmos |
| [98-14] | the preferred frame of the Universe, | Cosmos |
| [98-15] | The left-hand side describes the expansion rate of the universe | Cosmos |
| [98-16] | These are rough estimates for the size of the observable universe | observable universe |
| [99-17] | As the Universe expands | Cosmos |
| [99-18] | the energy densities of the three main components in our Universe. | Cosmos |
| [99-19] | We see that the Universe is often dominated by a single component: | Cosmos |
| [99-20] | This shows how the Universe expands | Cosmos |
| [99-21] | 7.3 Our Universe | Cosmos |
| [99-21] | hence determine the composition of the Universe. | Cosmos |
| [100-22] | A flat universe | Cosmos |
| [100-23] | so the Universe is pretty empty. | Cosmos |
| [101-24] | We see that most of the stuff in the Universe | Cosmos |
| [111-25] | all the stars in all the galaxies in the Universe put together | Cosmos |
| [137-26] | 4. Friedmann Universes | multiple wholes |
| [137-27] | Consider a universe with a cosmological constant, | Cosmos |
| [137-28] | Assuming that the universe “starts” with da/dt >0 near a= 0, | Cosmos |
| [137-29] | how many times can the photon circle the universe | Cosmos |
| [137-30] | before the universe ends? | Cosmos |
| [145-31] | Suppose you are a flatlander living in a universe | Cosmos |
| [145-32] | Assume that the universe is filled with a perfect fluid | Cosmos |
| [147-33] | the wormhole and the ones corresponding to the two universes | multiple wholes |