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Τετάρτη 2 Αυγούστου 2017

The Dark Side of the Universe Dark Matter and Dark Energy 1-4

            



The Dark Side of the Universe Dark Matter and Dark Energy 1-4

Δημοσιεύτηκε στις 29 Απρ 2013
The Dark Side of the Universe: Dark Matter and Dark Energy (1/4)
© CERN
Author(s) Turner, Michael (speaker)
Corporate author(s) CERN. Geneva
Imprint 2010-03-09. - Streaming video.
Series (Academic Training Lecture Regular Programme ; 2009-2010)
Lecture note on 2010-03-09T11:00:00
Presented at Academic Training Lectures
Subject category Academic Training Lecture Regular Programme
Abstract Lecture 1 : State of Cosmology Today

http://cds.cern.ch/record/1248220/
ANAΡΤΗΣΗ ΑΠΟ ΤΟ YOUTUBE 3/8/2017

Negative mass, Dark matter, Dark Energy, Bullet Cluster, Antigravity -2

            

Negative mass, Dark matter, Dark Energy, Bullet Cluster, Antigravity -2

Δημοσιεύτηκε στις 5 Ιουλ 2010

From
the observance of the HSS team and SCP team in 1998, they gained the
mass density of the negative(HSS: Ω_m = - 0.38(±0.22), SCP: Ω_m = -
0.4(±0.1) ), using field equations which do not have the cosmological
constant. The quantity of the mass couldn't be negative value in they
thought, the value was discarded.

In the world of positive mass,
ground state is a point that energy is low, but in case of negative
mass, ground state is a point that energy is the highest. Accordingly,
in the world of negative mass, energy level is filled from the highest
to the lowest, and stable state means the highest energy state, so the
catastrophe to energy level of minus infinity never happens even if
negative mass spontaneously emits energy. Assuming that negative mass
exists, Newton's Law of motion was derived in between negative and
positive masses and also between negative and negative masses.

Assuming
that negative mass(energy) and positive mass(energy) were born together
at the beginning of universe, it satisfies the various problems that
previous dark matter and dark energy possess, such as, centripetal force
effects of galaxy and galaxy clusters from previous dark matters, mass
effects that is proportional to the distance r, repulsive force needed
for expansion, dark energy that has positive values, low interaction
between dark matter when collision occurs between dark matter,
decelerating expansion and accelerating expansion of universe, formation
of void, inflation mechanism, fine tuning problem of mass density,
collision of Bullet cluster, universe's age, universe's size, the reason
of that dark energy seems to has a small and non-zero value.
Also, we prove to the dark energy observation value(10^(-47)GeV^4.

As a result, the necessity of observation focusing on exact computation and detection of negative mass is stated.
========

**Paper2 : Commemoration of the 100th Anniversary of General Relativity: On Problems and Solutions of General Relativity

https://www.researchgate.net/publicat...
ANAΡΤΗΣΗ ΑΠΟ ΤΟ YOUTUBE 3/8/2017


Two possibilities of NEGATIVE MASS

           

Two possibilities of NEGATIVE MASS

Δημοσιεύτηκε στις 7 Οκτ 2015

how
negative mass behaves in a gravitational field?what properties does it
have?maybe it's the same as dark energy or dark matter?maybe there is a
parallel universe?

Center Of Mass 11 Negative mass system

              



Center Of Mass 11 Negative mass system





ANAΡΤΗΣΗ ΑΠΟ ΤΟ YOUTUBE 3/8/2017

Moment of Inertia: Thick Cylinder (negative mass)

              

Moment of Inertia: Thick Cylinder (negative mass)

Δημοσιεύτηκε στις 2 Φεβ 2017

Re-deriving I for a cylinder of inner radius Ri and outer radius Ro, using the idea of shape-subtracting and negative mass

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    ANAΡΤΗΣΗ ΑΠΟ ΤΟ YOUTUBE 3/8/2017


Dark energy in the zero energy universe negative mass negative energy...

             



Dark energy in the zero energy universe  negative mass   negative energy...



ANAΡΤΗΣΗ ΑΠΟ ΤΟ YOUTUBE 3/8/2017

InterPlanetary Project Panel Discussion

            

InterPlanetary Project Panel Discussion

Δημοσιεύτηκε στις 31 Ιουλ 2017

Scientists,
science fiction authors, explorers, and artists meet for a conversation
at the historic Lensic theater in downtown Santa Fe on July 18, 2017.
Panelists discuss issues around the core questions: What will it take to
become an InterPlanetary civilization? How should we address the most
pressing problems of Earth to tackle a challenge at this scale? What is
holding humanity back, and what do we all need to achieve in terms of
novel governance, new technologies, shared resources, and global
cooperation to achieve this goal?

Panelists include: -Sandra
Moore Faber (UC Santa Cruz), a professor of astronomy and astrophysics
and the project investigator for the DEEP2 survey of 50,000 distant
galaxies using the Keck Observatory telescopes in Hawaii -Science
and technology journalist Kate Greene, who spent four months on a
simulated Mars mission for NASA -Transdisciplinary artist,
researcher, writer, teacher, and citizen scientist Dario Robleto
(Artist-in-residence at the SETI Institute) -Digital media executive
Scott Ross, who led George Lucas' companies in the 1980s and is a
co-founder, along with James Cameron and Stan Winston, of Digital
Domain, Inc. -Neal Stephenson, author of Seveneves, Cryptonomicon,
Snow Crash, and other works of speculative fiction who is is currently a
Miller Scholar at the Santa Fe Institute -Geoffrey West, a
complexity scientist whose 25+ years of research into mathematical
scaling laws have recently been published in the widely-acclaimed book
Scale: The Universal Laws of Growth, Innovation, Sustainability, and the
Pace of Life in Organisms, Cities, Economies, and Companies.

The event features images and ambient sounds by Thomas Ashcraft and Nate Metheny.

ANAΡΤΗΣΗ ΑΠΟ ΤΟ YOUTUBE 2/8/2017