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100 | 1 | _ | |a Ringwald, Andreas |0 P:(DE-H253)PIP1001650 |b 0 |e Corresponding author |
245 | _ | _ | |a Revealing the cosmic history with gravitational waves |
260 | _ | _ | |a Melville, NY |c 2022 |b Inst. |
264 | _ | 1 | |3 online |2 Crossref |b American Physical Society (APS) |c 2022-09-30 |
264 | _ | 1 | |3 print |2 Crossref |b American Physical Society (APS) |c 2022-09-01 |
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520 | _ | _ | |a The characteristics of the cosmic microwave background provide circumstantial evidence that the hot radiation-dominated epoch in the early Universe was preceded by a period of inflationary expansion. Here, we show how a measurement of the stochastic gravitational wave background can reveal the cosmic history and the physical conditions during inflation, subsequent pre- and reheating, and the beginning of the hot big bang era. This is exemplified with a particularly well-motivated and predictive minimal extension of the Standard Model, which is known to provide a complete model for particle physics—up to the Planck scale—and for cosmology—back to inflation. |
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542 | _ | _ | |i 2022-09-30 |2 Crossref |u https://creativecommons.org/licenses/by/4.0/ |
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650 | _ | 7 | |a gravitational radiation: background |2 INSPIRE |
650 | _ | 7 | |a gravitational radiation: stochastic |2 INSPIRE |
650 | _ | 7 | |a scale: Planck |2 INSPIRE |
650 | _ | 7 | |a inflation |2 INSPIRE |
650 | _ | 7 | |a history |2 INSPIRE |
650 | _ | 7 | |a cosmic background radiation |2 INSPIRE |
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650 | _ | 7 | |a reheating |2 INSPIRE |
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650 | _ | 7 | |a space-time: expansion |2 INSPIRE |
650 | _ | 7 | |a preheating |2 INSPIRE |
650 | _ | 7 | |a new physics |2 INSPIRE |
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787 | 0 | _ | |a Ringwald, Andreas et.al. |d 2022 |i IsParent |0 PUBDB-2022-01343 |r DESY-22-037 ; arXiv:2203.00621 ; TUM-HEP-1389-22 |t Revealing the Cosmic History with Gravitational Waves |
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