YaBeSH Engineering and Technology Library

    • Journals
    • PaperQuest
    • YSE Standards
    • YaBeSH
    • Login
    View Item 
    •   YE&T Library
    • ASME
    • Journal of Fluids Engineering
    • View Item
    •   YE&T Library
    • ASME
    • Journal of Fluids Engineering
    • View Item
    • All Fields
    • Source Title
    • Year
    • Publisher
    • Title
    • Subject
    • Author
    • DOI
    • ISBN
    Advanced Search
    JavaScript is disabled for your browser. Some features of this site may not work without it.

    Archive

    Turbulent Mixing, Viscosity, Diffusion, and Gravity in the Formation of Cosmological Structures: The Fluid Mechanics of Dark Matter

    Source: Journal of Fluids Engineering:;2000:;volume( 122 ):;issue: 004::page 830
    Author:
    C. H. Gibson
    DOI: 10.1115/1.1319156
    Publisher: The American Society of Mechanical Engineers (ASME)
    Abstract: Self-gravitational structure formation theory for astrophysics and cosmology is revised using nonlinear fluid mechanics. Gibson’s 1996–2000 theory balances fluid mechanical forces with gravitational forces and density diffusion with gravitational diffusion at critical viscous, turbulent, magnetic, and diffusion length scales termed Schwarz scales. Condensation and fragmentation occur for scales exceeding the largest Schwarz scale rather than LJ, the length scale introduced by Jeans in his 1902 inviscid-linear-acoustic theory. The largest Schwarz scale is often larger or smaller than LJ. From the new theory, the inner-halo (1021 m) dark-matter of galaxies comprises ∼105fossil-LJ-scale clumps of 1012 Earth-mass fossil-LSV-scale planets called primordial fog particles (PFPs) condensed soon after the cooling transition from plasma to neutral gas, 300,000 years after the Big Bang, with PFPs tidally disrupted from their clumps forming the interstellar medium. PFPs explain Schild’s 1996 “rogue planets[[ellipsis]]likely to be the missing mass” of a quasar lens-galaxy, inferred from twinkling frequencies of the quasar mirages, giving 30 million planets per star. The non-baryonic dark matter is super-diffusive and fragments at large LSD scales to form massive outer-galaxy-halos. In the beginning of structure formation 30,000 years after the Big Bang, with photon viscosity values ν of 5×1026 m2 s−1, the viscous Schwarz scale matched the horizon scale (LSV≈LH<LJ), giving 1046 kg proto-superclusters and finally 1042 kg proto-galaxies. Non-baryonic fluid diffusivities D∼1028 m2 s−1 from galaxy-outer-halo (LSD) scales (1022 m) measured in a dense galaxy cluster by Tyson, J. A., and Fischer, P., 1995, “Measurement of the Mass profile of Abell 1689,” Ap. J., 446, pp. L55–L58, indicate non-baryonic dark matter particles must have small mass (∼10−35 kg) to avoid detection. [S0098-2202(00)01504-2]
    keyword(s): Density , Force , Gravity (Force) , Fluid mechanics , Condensation , Diffusion (Physics) , Universe , Particulate matter , Matter , Turbulence , Viscosity , Cosmology , Plasmas (Ionized gases) , Big bang theory , Fluids AND Acoustics ,
    • Download: (95.64Kb)
    • Show Full MetaData Hide Full MetaData
    • Get RIS
    • Item Order
    • Go To Publisher
    • Statistics

      Turbulent Mixing, Viscosity, Diffusion, and Gravity in the Formation of Cosmological Structures: The Fluid Mechanics of Dark Matter

    URI
    https://yetl.yabesh.ir/yetl1/handle/yetl/123841
    Collections
    • Journal of Fluids Engineering

    Show full item record

    contributor authorC. H. Gibson
    date accessioned2017-05-09T00:02:38Z
    date available2017-05-09T00:02:38Z
    date copyrightDecember, 2000
    date issued2000
    identifier issn0098-2202
    identifier otherJFEGA4-27157#830_1.pdf
    identifier urihttp://yetl.yabesh.ir/yetl/handle/yetl/123841
    description abstractSelf-gravitational structure formation theory for astrophysics and cosmology is revised using nonlinear fluid mechanics. Gibson’s 1996–2000 theory balances fluid mechanical forces with gravitational forces and density diffusion with gravitational diffusion at critical viscous, turbulent, magnetic, and diffusion length scales termed Schwarz scales. Condensation and fragmentation occur for scales exceeding the largest Schwarz scale rather than LJ, the length scale introduced by Jeans in his 1902 inviscid-linear-acoustic theory. The largest Schwarz scale is often larger or smaller than LJ. From the new theory, the inner-halo (1021 m) dark-matter of galaxies comprises ∼105fossil-LJ-scale clumps of 1012 Earth-mass fossil-LSV-scale planets called primordial fog particles (PFPs) condensed soon after the cooling transition from plasma to neutral gas, 300,000 years after the Big Bang, with PFPs tidally disrupted from their clumps forming the interstellar medium. PFPs explain Schild’s 1996 “rogue planets[[ellipsis]]likely to be the missing mass” of a quasar lens-galaxy, inferred from twinkling frequencies of the quasar mirages, giving 30 million planets per star. The non-baryonic dark matter is super-diffusive and fragments at large LSD scales to form massive outer-galaxy-halos. In the beginning of structure formation 30,000 years after the Big Bang, with photon viscosity values ν of 5×1026 m2 s−1, the viscous Schwarz scale matched the horizon scale (LSV≈LH<LJ), giving 1046 kg proto-superclusters and finally 1042 kg proto-galaxies. Non-baryonic fluid diffusivities D∼1028 m2 s−1 from galaxy-outer-halo (LSD) scales (1022 m) measured in a dense galaxy cluster by Tyson, J. A., and Fischer, P., 1995, “Measurement of the Mass profile of Abell 1689,” Ap. J., 446, pp. L55–L58, indicate non-baryonic dark matter particles must have small mass (∼10−35 kg) to avoid detection. [S0098-2202(00)01504-2]
    publisherThe American Society of Mechanical Engineers (ASME)
    titleTurbulent Mixing, Viscosity, Diffusion, and Gravity in the Formation of Cosmological Structures: The Fluid Mechanics of Dark Matter
    typeJournal Paper
    journal volume122
    journal issue4
    journal titleJournal of Fluids Engineering
    identifier doi10.1115/1.1319156
    journal fristpage830
    journal lastpage835
    identifier eissn1528-901X
    keywordsDensity
    keywordsForce
    keywordsGravity (Force)
    keywordsFluid mechanics
    keywordsCondensation
    keywordsDiffusion (Physics)
    keywordsUniverse
    keywordsParticulate matter
    keywordsMatter
    keywordsTurbulence
    keywordsViscosity
    keywordsCosmology
    keywordsPlasmas (Ionized gases)
    keywordsBig bang theory
    keywordsFluids AND Acoustics
    treeJournal of Fluids Engineering:;2000:;volume( 122 ):;issue: 004
    contenttypeFulltext
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian
     
    DSpace software copyright © 2002-2015  DuraSpace
    نرم افزار کتابخانه دیجیتال "دی اسپیس" فارسی شده توسط یابش برای کتابخانه های ایرانی | تماس با یابش
    yabeshDSpacePersian