https://arxiv.org/abs/2006.07125 close this message Accessible arXiv Do you navigate arXiv using a screen reader or other assistive technology? Are you a professor who helps students do so? We want to hear from you. Please consider signing up to share your insights as we work to make arXiv even more open. Share Insights Skip to main content Cornell University We gratefully acknowledge support from the Simons Foundation and member institutions. arxiv logo > gr-qc > arXiv:2006.07125 [ ] Help | Advanced Search [All fields ] Search arXiv logo Cornell University Logo [ ] GO quick links * Login * Help Pages * About General Relativity and Quantum Cosmology arXiv:2006.07125 (gr-qc) [Submitted on 12 Jun 2020 (v1), last revised 10 Aug 2020 (this version, v2)] Title:Breaking the Warp Barrier: Hyper-Fast Solitons in Einstein-Maxwell-Plasma Theory Authors:Erik W. Lentz Download PDF Abstract: Solitons in space--time capable of transporting time-like observers at superluminal speeds have long been tied to violations of the weak, strong, and dominant energy conditions of general relativity. The negative-energy sources required for these solitons must be created through energy-intensive uncertainty principle processes as no such classical source is known in particle physics. This paper overcomes this barrier by constructing a class of soliton solutions that are capable of superluminal motion and sourced by purely positive energy densities. The solitons are also shown to be capable of being sourced from the stress-energy of a conducting plasma and classical electromagnetic fields. This is the first example of hyper-fast solitons resulting from known and familiar sources, reopening the discussion of superluminal mechanisms rooted in conventional physics. Comments: 14 pages, 5 figures, comments welcome General Relativity and Quantum Cosmology (gr-qc); High Subjects: Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics - Phenomenology (hep-ph) Cite as: arXiv:2006.07125 [gr-qc] (or arXiv:2006.07125v2 [gr-qc] for this version) https://doi.org/10.48550/arXiv.2006.07125 Focus to learn more arXiv-issued DOI via DataCite Submission history From: Erik Lentz [view email] [v1] Fri, 12 Jun 2020 12:33:05 UTC (6,896 KB) [v2] Mon, 10 Aug 2020 14:55:58 UTC (5,323 KB) Full-text links: Download: * PDF * Other formats (license) Current browse context: gr-qc < prev | next > new | recent | 2006 Change to browse by: astro-ph astro-ph.HE hep-ph References & Citations * INSPIRE HEP * NASA ADS * Google Scholar * Semantic Scholar a export bibtex citation Loading... Bibtex formatted citation x [loading... ] Data provided by: Bookmark BibSonomy logo Mendeley logo Reddit logo ScienceWISE logo (*) Bibliographic Tools Bibliographic and Citation Tools [ ] Bibliographic Explorer Toggle Bibliographic Explorer (What is the Explorer?) [ ] Litmaps Toggle Litmaps (What is Litmaps?) [ ] scite.ai Toggle scite Smart Citations (What are Smart Citations?) ( ) Code & Data Code and Data Associated with this Article [ ] arXiv Links to Code Toggle arXiv Links to Code & Data (What is Links to Code & Data?) ( ) Demos Demos [ ] Replicate Toggle Replicate (What is Replicate?) ( ) Related Papers Recommenders and Search Tools [ ] Connected Papers Toggle Connected Papers (What is Connected Papers?) [ ] Core recommender toggle CORE Recommender (What is CORE?) [ ] IArxiv recommender toggle IArxiv Recommender (What is IArxiv?) ( ) About arXivLabs arXivLabs: experimental projects with community collaborators arXivLabs is a framework that allows collaborators to develop and share new arXiv features directly on our website. Both individuals and organizations that work with arXivLabs have embraced and accepted our values of openness, community, excellence, and user data privacy. arXiv is committed to these values and only works with partners that adhere to them. Have an idea for a project that will add value for arXiv's community? Learn more about arXivLabs and how to get involved. Which authors of this paper are endorsers? | Disable MathJax (What is MathJax?) * About * Help * Click here to contact arXiv Contact * Click here to subscribe Subscribe * Copyright * Privacy Policy * Web Accessibility Assistance * arXiv Operational Status Get status notifications via email or slack