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2026
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| Online Access: | https://doi.org/10.5281/zenodo.18984843 |
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| _version_ | 1866901642550444032 |
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| author | Bergmann, Gordon |
| author_facet | Bergmann, Gordon |
| contents | <p>The Bergmann Bounce Drive (BBD) was originally introduced as a reaction-mass-free spacecraft propulsion concept that utilizes controlled quantum-gravitational mini-bounces to generate directed spacetime expansion gradients. The first version (Zenodo DOI 10.5281/zenodo.18703627) theoretically achieved specific impulses of 10^{12}–10^{16} s but suffered from extremely high external energy requirements (10^{20}–10^{30} J per pulse), instability of the bounce region, and the lack of intrinsic navigation. A subsequent work (Zenodo DOI 10.5281/zenodo.18984399) calculated journey times to selected exoplanets assuming refueling at Stellar Bloom Stations in star-forming nebulae.</p> <p>With the integration of the Bergmann Chaos Field δ_chaos in BBD 2.0 (see separate manuscript), significant improvements emerge: stochastic amplification reduces external energy demand by factors of 10^3 to 10^6, retrocausal navigation optimizes trajectories, and Langevin stabilization provides intrinsic error correction. This paper recalculates the revised journey times to Proxima Centauri b, TRAPPIST-1 e, TOI-715 b, and Kepler-442 b under the new BBD 2.0 parameters and demonstrates that interstellar travel with chaos field amplification is no longer merely theoretical but becomes practically more realistic.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18984843 |
| institution | Zenodo |
| language | |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Rapid Interstellar Travel with BBD 2.0: Revised Journey Times with Chaos Field Amplification Bergmann, Gordon <p>The Bergmann Bounce Drive (BBD) was originally introduced as a reaction-mass-free spacecraft propulsion concept that utilizes controlled quantum-gravitational mini-bounces to generate directed spacetime expansion gradients. The first version (Zenodo DOI 10.5281/zenodo.18703627) theoretically achieved specific impulses of 10^{12}–10^{16} s but suffered from extremely high external energy requirements (10^{20}–10^{30} J per pulse), instability of the bounce region, and the lack of intrinsic navigation. A subsequent work (Zenodo DOI 10.5281/zenodo.18984399) calculated journey times to selected exoplanets assuming refueling at Stellar Bloom Stations in star-forming nebulae.</p> <p>With the integration of the Bergmann Chaos Field δ_chaos in BBD 2.0 (see separate manuscript), significant improvements emerge: stochastic amplification reduces external energy demand by factors of 10^3 to 10^6, retrocausal navigation optimizes trajectories, and Langevin stabilization provides intrinsic error correction. This paper recalculates the revised journey times to Proxima Centauri b, TRAPPIST-1 e, TOI-715 b, and Kepler-442 b under the new BBD 2.0 parameters and demonstrates that interstellar travel with chaos field amplification is no longer merely theoretical but becomes practically more realistic.</p> |
| title | Rapid Interstellar Travel with BBD 2.0: Revised Journey Times with Chaos Field Amplification |
| url | https://doi.org/10.5281/zenodo.18984843 |