{"id":31,"date":"2019-05-07T16:19:54","date_gmt":"2019-05-07T16:19:54","guid":{"rendered":"https:\/\/ehrlich.physics.gmu.edu\/?page_id=31"},"modified":"2023-10-24T15:34:41","modified_gmt":"2023-10-24T15:34:41","slug":"tachyon-papers","status":"publish","type":"page","link":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/tachyon-papers\/","title":{"rendered":"tachyon papers"},"content":{"rendered":"\n

1. Ehrlich, R., “Implications for the Cosmic Ray Spectrum of a Negative Electron Neutrino Mass2<\/sup>, Physical Review D, 60<\/strong>, 17302 (1999) [July 1,1999], https:\/\/arxiv.org\/pdf\/astro-ph\/9807324.pdf<\/a><\/p>\n\n\n\n

2. Ehrlich, R., “Is There a 4.5 PeV Neutron Line in the Cosmic Ray Spectrum?,” Physical Review D, 60<\/strong>, 73005 (1999), https:\/\/arxiv.org\/pdf\/astro-ph\/9904290.pdf <\/a><\/p>\n\n\n\n

3. Ehrlich, R., “Neutrino Mass Inferred from the Cosmic Ray Spectrum and Tritium Beta Decay, Phys. Lett. B, 493<\/strong> (2000) 229-232, https:\/\/arxiv.org\/pdf\/hep-ph\/0009040.pdf <\/a><\/p>\n\n\n\n

4. Ehrlich, R., \u201cFaster-than-light speeds, tachyons, and the possibility of tachyonic neutrinos,\u201d Am. J. Phys., 71 (11) 1109-14 (2003), https:\/\/doi.org\/10.1119\/1.1590657 <\/a><\/p>\n\n\n\n

5. Ehrlich, R.,  \u201cEvidence for two neutrino mass eigenstates from SN 1987A and the possibility of superluminal neutrinos,\u201d  Astroparticle Physics 35 (2012), pp. 625-628 http:\/\/arxiv.org\/abs\/1111.0502<\/a><\/p>\n\n\n\n

6. Ehrlich, R. \u201cTachyonic neutrinos and the neutrino masses,\u201d Astropart. Phys., 41 (2013) 1\u20136, http:\/\/arxiv.org\/pdf\/1204.0484.pdf<\/a><\/p>\n\n\n\n

7. Chan, M .H. and Ehrlich, R., \u201cSterile neutrino fits to dark matter mass profiles in the Milky Way and in galaxy clusters,\u201d Astrophysics and Space Science, 349, (1), 407- 413, (<\/strong>2014), http:\/\/arxiv.org\/abs\/1301.6640 <\/a><\/p>\n\n\n\n

8. Ehrlich, R. Search for cosmic ray sources of neutral hadrons yielding a peak just above the knee, and possible evidence for a $5.86 PeV$ enhancement, http:\/\/arxiv.org\/abs\/1307.3944<\/a><\/p>\n\n\n\n

9. Ehrlich, R. “Could a reported 2007 analysis of Super-Kamiokande data have missed a detectable supernova signal from Andromeda?,” ISRN High Energy Physics, vol. 2014, Article ID 408508, 4 pages, 2014. doi:10.1155\/2014\/408508.  Also: http:\/\/arxiv.org\/abs\/1301.3390<\/a><\/p>\n\n\n\n

10. Ehrlich, R., \u201cSix observations consistent with the electron neutrino being a tachyon with mass: m2<\/sup> = – 0.11+0.02 eV2<\/sup> ,\u201d Astropart. Phys. 66, 11 (2015), http:\/\/arxiv.org\/pdf\/1408.2804v9.pdf<\/a><\/p>\n\n\n\n

11. Jentschura, U. and  Ehrlich, R., Lepton-pair _Cerenkov radiation emitted by tachyonic neutrinos:Lorentz-covariant approach and Ice Cube data, Advances in High Energy Physics, vol. 2016, Article ID 4764981; http:\/\/arxiv.org\/abs\/1607.00640<\/a><\/p>\n\n\n\n

12. R. Ehrlich, 3 neutrino mass experiments fit a strange 3 + 3 model, but will KATRIN reveal the model’s unique 3-part signature? R. Ehrlich, Astropart. Phys., 85, 43-49 (2016; https:\/\/arxiv.org\/abs\/1602.09043<\/a><\/p>\n\n\n\n

13. Jentschura, U., Nandori, I, and Ehrlich, R., Calculation of the Decay Rate of Tachyonic Neutrinos against Charged-Lepton-Pair and Neutrino-Pair Cerenkov Radiation”, J. Phys. G: Nucl. Part. Phys. 44 105201 (2017); https:\/\/arxiv.org\/abs\/1709.07711<\/a><\/p>\n\n\n\n

14. R. Ehrlich, The Mont Blanc neutrinos from SN 1987A: Could they have been monochromatic (8 MeV) tachyons with m 2 <\/sup>= -0.38 keV2<\/sup>?, Astropart. Phys.,99, 21-29 (2018); https:\/\/arxiv.org\/abs\/1701.00488<\/a> <\/p>\n\n\n\n

15. R. Ehrlich. A review of the empirical evidence for superluminal particles and the 3 + 3 model of the neutrino masses, Advances in Astronomy Volume 2019, Article ID 2820492, http:\/\/arXiv:1711.09897<\/a><\/p>\n\n\n\n

16. R. Ehrlich. First results of the KATRIN neutrino mass experiment and their consistency with an exotic 3+3 model, Lett. in High Energy Phys., vol 4, no 4, (2019)  http:\/\/journals.andromedapublisher.com\/index.php\/LHEP\/article\/view\/139\/76<\/a><\/p>\n\n\n\n

17. R. Ehrlich. The Tachyon Nexus: An Educational Resource on Tachyons and Time Travel, to appear in the Journal of College Science Teaching, Vol. 52, Issue 3, Jan\/ Feb 2023 (2022) https:\/\/arxiv.org\/pdf\/2001.00225.pdf<\/a><\/p>\n\n\n\n

18. R. Ehrlich, 5 Reasons to expect an 8 MeV line in the SN 1987A neutrino spectrum, Lett. in High En. Phys., LHEP-199, 2021<\/a> https:\/\/arxiv.org\/pdf\/2101.08128.pdf<\/a><\/p>\n\n\n\n

19. R, Ehrlich, A Review of Searches for Evidence of Tachyons, Symmetry<\/em>\u00a02022<\/strong>,\u00a014<\/em>(6), 1198, Symmetry | Free Full-Text | A Review of Searches for Evidence of Tachyons | HTML (mdpi.com)<\/a><\/p>\n\n\n\n

20. R. Ehrlich, Tachyonic Neutrinos: From the Cosmic Rays to Extragalactic Supernovae<\/a>, Symmetry<\/em>\u00a02023<\/strong>,\u00a015<\/em>(9), 1624;\u00a0https:\/\/doi.org\/10.3390\/sym15091624<\/a>\u00a0<\/p>\n\n\n\n

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1. Ehrlich, R., “Implications for the Cosmic Ray Spectrum of a Negative Electron Neutrino Mass2, Physical Review D, 60, 17302 (1999) [July 1,1999], https:\/\/arxiv.org\/pdf\/astro-ph\/9807324.pdf 2. Ehrlich, R., “Is There a 4.5 PeV Neutron Line in the Cosmic Ray Spectrum?,” Physical Review D, 60, 73005 (1999), https:\/\/arxiv.org\/pdf\/astro-ph\/9904290.pdf 3. Ehrlich, R., “Neutrino Mass Inferred from the Cosmic […]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-31","page","type-page","status-publish","czr-hentry"],"_links":{"self":[{"href":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/wp-json\/wp\/v2\/pages\/31","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/wp-json\/wp\/v2\/comments?post=31"}],"version-history":[{"count":28,"href":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/wp-json\/wp\/v2\/pages\/31\/revisions"}],"predecessor-version":[{"id":726,"href":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/wp-json\/wp\/v2\/pages\/31\/revisions\/726"}],"wp:attachment":[{"href":"https:\/\/ehrlich.physics.gmu.edu\/index.php\/wp-json\/wp\/v2\/media?parent=31"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}