The Measurement That Would Reveal The Universe As A Computer Simulation

One of modern physics’ most cherished ideas is quantum chromodynamics, the theory that describes the strong nuclear force, how it binds quarks and gluons into protons and neutrons, how these form nuclei that themselves interact. This is the universe at its most fundamental. So an interesting pursuit is to simulate quantum chromodynamics on a computer to see what kind of complexity arises. The promise is that simulating physics on such a fundamental level is more or less equivalent to simulating the universe itself. There are one or two challenges of course. The physics is mind-bogglingly complex and operates on a vanishingly small scale. That may not sound like much but the significant point is that the simulation is essentially indistinguishable from the real thing (at least as far as we understand it). It’s not hard to imagine that Moore’s Law-type progress will allow physicists to simulate significantly larger regions of space. First, some background. What they find is interesting.

Earth Earth is the third planet from the Sun. It is the densest and fifth-largest of the eight planets in the Solar System. It is also the largest of the Solar System's four terrestrial planets. It is sometimes referred to as the world or the Blue Planet.[23] Earth formed approximately 4.54 billion years ago, and life appeared on its surface within its first billion years.[24] Earth's biosphere then significantly altered the atmospheric and other basic physical conditions, which enabled the proliferation of organisms as well as the formation of the ozone layer, which together with Earth's magnetic field blocked harmful solar radiation, and permitted formerly ocean-confined life to move safely to land.[25] The physical properties of the Earth, as well as its geological history and orbit, have allowed life to persist. Name and etymology In general English usage, the name earth can be capitalized or spelled in lowercase interchangeably, either when used absolutely or prefixed with "the" (i.e. Heat

The Number 9 | The Secret Knowledge of The Ancients Number Nine Code 911 The number 9 is the last number in a base 10 system which is the last and limit of all that is. Nine is a number which has many interesting qualities that other numbers do not have and has been used to hold a hidden code that affects every person on earth. If you think nine is just another number, you are in for a big surprise. There are small coincidences that all add up to something universally amazing which was created for us then given to mankind through Enoch, which he wrote down on stone tablets and passed down to his great grandson Noah which built the arc. The 9 code is everywhere for us to see if we are willing to search for it. The Intelligent design of our universe is geometrical and congruent forming beautiful shapes and images with the number 9 as a proof of concept stamp on it given by God. Use this ancient method to get understanding and understanding why this happens is the key Mr. This is the first sentence of the Bible and the first truth of the law or order.

Astrological age There are two broad approaches about the effects upon the world due to the astrological ages. Some astrologers believe the changes upon Earth are caused and marked by the influences of the given astrological sign, associated with the Age, while other astrologers do not follow the causative model and believe it is a matter of synchronicity.[3] Many astrologers believe that the Age of Aquarius has arrived recently or will arrive in the near future. On the other hand, some believe that the Age of Aquarius arrived up to five centuries ago, or will not start until six centuries from now.[4] Despite all references provided by various sources, astrologers cannot agree upon exact dates for the beginning or ending of the ages. Various ages are described below, such as the Age of Aquarius. Overview[edit] Traditional western Zodiac signs There are three broad perspectives on the astrological ages: Contentious aspects of the astrological ages[edit] Consensus approach to the astrological ages[edit]

The Most Distant, Dark Galaxy Ever Found! : Starts With A Bang “One mustn’t look at the abyss, because there is at the bottom an inexpressible charm which attracts us.” -Gustave Flaubert The deepest depths of space, out beyond our atmosphere, our Solar System, and even our galaxy, hold the richness of the great Universe beyond. Image credit: R. In addition to the visible, luminous matter we see in the image above, there’s both non-luminous normal matter and dark matter. One of the easiest ways to figure this out and measure it is by looking at some chance locations in the Universe where there are two massive structures directly lined up, one-behind-the-other, relative to our line-of-sight. Image credit: ESA, NASA, K. Above is what happens when you have a galaxy cluster with both a quasar and a background galaxy directly behind it. It works the other way, too. The results are often breathtaking and, at least to me, always spectacular. Image credit: ESA/Hubble & NASA, retrieved from APOD. Image credit: Public Domain image, retrieved from Wikipedia.

Quark A quark (/ˈkwɔrk/ or /ˈkwɑrk/) is an elementary particle and a fundamental constituent of matter. Quarks combine to form composite particles called hadrons, the most stable of which are protons and neutrons, the components of atomic nuclei.[1] Due to a phenomenon known as color confinement, quarks are never directly observed or found in isolation; they can be found only within hadrons, such as baryons (of which protons and neutrons are examples), and mesons.[2][3] For this reason, much of what is known about quarks has been drawn from observations of the hadrons themselves. The quark model was independently proposed by physicists Murray Gell-Mann and George Zweig in 1964.[5] Quarks were introduced as parts of an ordering scheme for hadrons, and there was little evidence for their physical existence until deep inelastic scattering experiments at the Stanford Linear Accelerator Center in 1968.[6][7] Accelerator experiments have provided evidence for all six flavors. Classification[edit]

Supernova A supernova (abbreviated SN, plural SNe after "supernovae") is a stellar explosion that is more energetic than a nova. It is pronounced /ˌsuːpəˈnoʊvə/ with the plural supernovae /ˌsuːpəˈnoʊviː/ or supernovas. Supernovae are extremely luminous and cause a burst of radiation that often briefly outshines an entire galaxy, before fading from view over several weeks or months. During this interval a supernova can radiate as much energy as the Sun is expected to emit over its entire life span.[1] The explosion expels much or all of a star's material[2] at a velocity of up to 30,000 km/s (10% of the speed of light), driving a shock wave[3] into the surrounding interstellar medium. This shock wave sweeps up an expanding shell of gas and dust called a supernova remnant. Nova means "new" in Latin, referring to what appears to be a very bright new star shining in the celestial sphere; the prefix "super-" distinguishes supernovae from ordinary novae which are far less luminous. Discovery[edit]

Gamma-ray burst Artist's illustration showing the life of a massive star as nuclear fusion converts lighter elements into heavier ones. When fusion no longer generates enough pressure to counteract gravity, the star rapidly collapses to form a black hole. Theoretically, energy may be released during the collapse along the axis of rotation to form a gamma-ray burst. Gamma-ray bursts (GRBs) are flashes of gamma rays associated with extremely energetic explosions that have been observed in distant galaxies. Most observed GRBs are believed to consist of a narrow beam of intense radiation released during a supernova or hypernova as a rapidly rotating, high-mass star collapses to form a neutron star, quark star, or black hole. On November 21, 2013, NASA released detailed data about one of the strongest gamma-ray burst, designated GRB 130427A, that was observed on April 27, 2013.[7][8] History[edit] Positions on the sky of all gamma-ray bursts detected during the BATSE mission. Afterglow[edit]

Hypernova Eta Carinae, in the constellation of Carina, one of the nearer candidates for a future hypernova A hypernova (pl. hypernovae) is a type of supernova explosion with an energy substantially higher than that of standard supernovae. An alternative term for most hypernovae is "superluminous supernovae" (SLSNe). Such explosions are believed to be the origin of long-duration gamma-ray bursts.[1] Just like supernovae in general, hypernovae are produced by several different types of stellar explosion: some well modelled and observed in recent years, some still tentatively suggested for observed hypernovae, and some entirely theoretical. The word collapsar, short for collapsed star, was formerly used to refer to the end product of stellar gravitational collapse, a stellar-mass black hole. History of the term[edit] Before the 1990s, the term "hypernova" was used sporadically to describe the theoretical extremely energetic explosions of extremely massive population III stars. Gamma-ray bursts[edit]