Matches in SemOpenAlex for { <https://semopenalex.org/work/W2810911288> ?p ?o ?g. }
- W2810911288 abstract "The possibility to correlate ether-drift measurements in laboratory and direct CMB observations with satellites in space would definitely confirm the existence of a fundamental preferred frame for relativity. Today, the small residuals observed so far (from Michelson-Morley onward) are just considered typical instrumental effects in experiments with better and better sensitivity. Though, if the velocity of light propagating in the various interferometers is not exactly the same parameter c of Lorentz transformations, nothing would really prevent to observe an ether drift. Thus, for the Earth cosmic velocity v = 370 km/s, we argue that a fundamental 10-15 light anisotropy, as presently observed in vacuum and in solid dielectrics, is revealing a 10-9 difference in the vacuum effective refractivity between an apparatus in an ideal freely falling frame and an apparatus on the Earth surface. In this perspective, the stochastic nature of the physical vacuum could also explain the irregular character of the signal and the observed substantial reduction from its instantaneous 10-15 value to its statistical average 10-18 (or smaller). For the same v = 370 km/s the different refractivities, respectively, $ {O}(10^{-4})$ and $ {O}(10^{-5})$ for air or helium at atmospheric pressure, could also explain the observed light anisotropy, respectively $ {O}(10^{-10})$ and $ {O}(10^{-11})$ . However, for consistency, one should also understand the physical mechanism which enhances the signal in weakly bound gaseous matter but remains ineffective in solid dielectrics where the refractivity is $ {O}(1)$ . This mechanism is naturally identified in a non-local, tiny temperature gradient of a fraction of millikelvin which is found in all classical experiments and might ultimately be related to the CMB temperature dipole of ±3 mK or reflect the fundamental energy flow associated with a Lorentz-non-invariant vacuum state. The importance of the issue would deserve more stringent tests with dedicated experiments and significant improvements in the data analysis.-1" @default.
- W2810911288 created "2018-07-10" @default.
- W2810911288 creator A5028468294 @default.
- W2810911288 creator A5032482559 @default.
- W2810911288 date "2018-08-01" @default.
- W2810911288 modified "2023-10-17" @default.
- W2810911288 title "Cosmic Microwave Background and the issue of a fundamental preferred frame" @default.
- W2810911288 cites W1456881554 @default.
- W2810911288 cites W1507715885 @default.
- W2810911288 cites W1527803380 @default.
- W2810911288 cites W1622834184 @default.
- W2810911288 cites W1829727542 @default.
- W2810911288 cites W1867162130 @default.
- W2810911288 cites W1972659350 @default.
- W2810911288 cites W1975719162 @default.
- W2810911288 cites W1977980504 @default.
- W2810911288 cites W1979381070 @default.
- W2810911288 cites W1981117060 @default.
- W2810911288 cites W1981652120 @default.
- W2810911288 cites W1982771003 @default.
- W2810911288 cites W1985198621 @default.
- W2810911288 cites W1985872335 @default.
- W2810911288 cites W1993434643 @default.
- W2810911288 cites W1997708885 @default.
- W2810911288 cites W1999259346 @default.
- W2810911288 cites W2000627764 @default.
- W2810911288 cites W2002330551 @default.
- W2810911288 cites W2003764788 @default.
- W2810911288 cites W2007767613 @default.
- W2810911288 cites W2012328636 @default.
- W2810911288 cites W2015812648 @default.
- W2810911288 cites W2018451229 @default.
- W2810911288 cites W2018978561 @default.
- W2810911288 cites W2022279769 @default.
- W2810911288 cites W2024404550 @default.
- W2810911288 cites W2026217640 @default.
- W2810911288 cites W2026826893 @default.
- W2810911288 cites W2032495796 @default.
- W2810911288 cites W2034501415 @default.
- W2810911288 cites W2047349307 @default.
- W2810911288 cites W2056173066 @default.
- W2810911288 cites W2056462191 @default.
- W2810911288 cites W2057190492 @default.
- W2810911288 cites W2058175563 @default.
- W2810911288 cites W2062226247 @default.
- W2810911288 cites W2063175615 @default.
- W2810911288 cites W2069828439 @default.
- W2810911288 cites W2079147371 @default.
- W2810911288 cites W2079830513 @default.
- W2810911288 cites W2085155384 @default.
- W2810911288 cites W2086236442 @default.
- W2810911288 cites W2087319685 @default.
- W2810911288 cites W2087644519 @default.
- W2810911288 cites W2107971023 @default.
- W2810911288 cites W2149335174 @default.
- W2810911288 cites W2155022091 @default.
- W2810911288 cites W2162225920 @default.
- W2810911288 cites W2223094112 @default.
- W2810911288 cites W2226817661 @default.
- W2810911288 cites W2231387490 @default.
- W2810911288 cites W2272080338 @default.
- W2810911288 cites W2303806597 @default.
- W2810911288 cites W2324809081 @default.
- W2810911288 cites W2328274794 @default.
- W2810911288 cites W2564668010 @default.
- W2810911288 cites W3098897004 @default.
- W2810911288 cites W3098912427 @default.
- W2810911288 cites W3099212193 @default.
- W2810911288 cites W3099920396 @default.
- W2810911288 cites W3102420160 @default.
- W2810911288 cites W3102543262 @default.
- W2810911288 cites W3103017459 @default.
- W2810911288 cites W3103304485 @default.
- W2810911288 cites W3103435651 @default.
- W2810911288 cites W3188897366 @default.
- W2810911288 cites W4246936343 @default.
- W2810911288 cites W2080682421 @default.
- W2810911288 cites W2092881526 @default.
- W2810911288 cites W2165666695 @default.
- W2810911288 doi "https://doi.org/10.1140/epjp/i2018-12136-5" @default.
- W2810911288 hasPublicationYear "2018" @default.
- W2810911288 type Work @default.
- W2810911288 sameAs 2810911288 @default.
- W2810911288 citedByCount "5" @default.
- W2810911288 countsByYear W28109112882019 @default.
- W2810911288 countsByYear W28109112882021 @default.
- W2810911288 countsByYear W28109112882022 @default.
- W2810911288 countsByYear W28109112882023 @default.
- W2810911288 crossrefType "journal-article" @default.
- W2810911288 hasAuthorship W2810911288A5028468294 @default.
- W2810911288 hasAuthorship W2810911288A5032482559 @default.
- W2810911288 hasBestOaLocation W28109112882 @default.
- W2810911288 hasConcept C120665830 @default.
- W2810911288 hasConcept C121332964 @default.
- W2810911288 hasConcept C122966575 @default.
- W2810911288 hasConcept C207297109 @default.
- W2810911288 hasConcept C25587389 @default.
- W2810911288 hasConcept C74650414 @default.
- W2810911288 hasConcept C85725439 @default.
- W2810911288 hasConceptScore W2810911288C120665830 @default.