Hydro-Gravitational Dynamics of Planets and Dark Energy
سال انتشار: 1391
نوع سند: مقاله ژورنالی
زبان: انگلیسی
مشاهده: 318
فایل این مقاله در 7 صفحه با فرمت PDF قابل دریافت می باشد
- صدور گواهی نمایه سازی
- من نویسنده این مقاله هستم
استخراج به نرم افزارهای پژوهشی:
شناسه ملی سند علمی:
JR_JAFM-2-2_005
تاریخ نمایه سازی: 27 دی 1400
چکیده مقاله:
Self gravitational fluid mechanical methods termed hydro-gravitational-dynamics (HGD) predict plasma fragmentation ۰.۰۳ Myr after the turbulent big bang to form protosuperclustervoids, turbulent protosuperclusters, and protogalaxies at the ۰.۳ Myr transition from plasma to gas. Linear protogalaxyclusters fragment at ۰.۰۰۳ Mpc viscous-inertial scales along turbulent vortex lines or in spirals, as observed. The plasma protogalaxies fragment on transition into white-hot planet-mass gas clouds (PFPs) in million-solar-mass clumps (PGCs) that become globular-star-clusters (GCs) from tidal forces or dark matter (PGCs) by freezing and diffusion into ۰.۳ Mpc halos with ۹۷% of the galaxy mass. The weakly collisional non-baryonic dark matter diffuses to > Mpc scales and fragments to form galaxy cluster halos. Stars and larger planets form by binary mergers of the trillion PFPs per PGC, mostly on ۰.۰۳ Mpc galaxy accretion disks. Stars deaths depend on rates of planet accretion and internal star mixing. Moderate accretion rates pro-duce white dwarfs that evaporate surrounding gas planets by spin-radiation to form planetary nebulae before Supernova Ia events, dimming some events to give systematic distance errors, the dark energy hypothesis, and overestimates of the universe age.
نویسندگان
C. H. Gibson
University of California San Diego, La Jolla, CA ۹۲۰۹۳-۰۴۱۱, USA
R. E. Schild
Center for Astrophysics, ۶۰ Garden Street, Cambridge, MA ۰۲۱۳۸, USA