What is more fundamental than space-time and mass-energy? Inside the event horizon, light cannot escape to infinity, whereas outside the event horizon, light can escape to infinity if it is traveling in the right direction.
According to stellar theory, deuterium cannot be produced in stellar interiors; Big bang nucleosynthesis, deuterium is destroyed inside of stars. This picture shows the Big bang nucleosynthesis outer rings and bright inner ring characteristic of an hourglass nebula.
BurbidgeFowler and Hoyle  is a well-known summary of the state of the field in The net effect is shown at right. This has proved to be of limited usefulness in that the inconsistencies were resolved by better observations, and in most cases trying to change BBN resulted in abundances that were more inconsistent with observations rather than less.
The modeling of the production of helium and the hydrogen-helium ratio also makes predictions about other nuclear species, particularly 7Li, 2H deuterium and 3He. Developments in particle physics during the s, however, suggested that the net baryon number may in fact undergo alteration.
Of the remainder, 23 percent is made up of dark matterwhich is likely composed of one or more species of subatomic particles that interact very weakly with ordinary matter, and 72 percent is made of dark energy, which apparently is driving the accelerating expansion of the universe. A star gains heavier elements by combining its lighter nuclei, hydrogendeuteriumberylliumlithiumand boronwhich were found in the initial composition of the interstellar medium and hence the star.
Since the universe is presumed to be homogeneousit has one unique value of the baryon-to-photon ratio. Big Bang nucleosynthesis Big Bang nucleosynthesis  occurred within the first three minutes of the beginning of the universe and is responsible for much of the abundance of 1H protium2H D, deuterium3He helium-3and 4He helium This value is greater than what theoretical physicists had originally predicted on the basis of early unification schemes for the forces of nature.
Nemiroff, assistant professor of physics at Michigan Technological University, responds. The space-time singularity associated with the big bang differs in two important ways from the singularity associated with a black hole. First, how was matter able to get out of the big-bang singularity?
Astronomers are therefore diligently searching for these objects. The second reason for researching non-standard BBN, and largely the focus of non-standard BBN in the early 21st century, is to use BBN to place limits on unknown or speculative physics.
From this temperature bath and the gravitational energy of expansion would then have emerged the particles and antiparticles of noninflationary big bang cosmologies.
First of all, it is not really known whether or not the universe started from a singularity. In laboratory experiments of similar phase transitions—for example, the solidification of a liquid into a solid—involving two or more substances, the final state may contain a very uneven distribution of the constituent substances, a fact exploited by industry to purify certain materials.
The following stages occur during the first few minutes of the Universe: No one knows the answer to this question, and perhaps some would argue that the answer is not to be sought within the boundaries of natural science.
This graph is a corrected version of one from this LBL page. The graph above shows the time evolution of the abundances of the light elements for a slightly higher baryon density.
It also predicts about 0. Precision observations of the cosmic microwave background radiation   with the Wilkinson Microwave Anisotropy Probe WMAP and Planck give an independent value for the baryon-to-photon ratio.
Matter was spread out almost perfectly smoothly. After 1 second, the only reaction that appreciably changes the Big bang nucleosynthesis of neutrons is neutron decay, shown at right.
According to NASA, the gravitational pull of small fluctuations in the density of matter back then gave rise to the vast web-like structure of stars and emptiness seen today. After at least 85 doublings, the temperature, which started out at or K, would have dropped to very low values near absolute zero.
Although 4He continues to be produced by stellar fusion and alpha decays and trace amounts of 1H continue to be produced by spallation and certain types of radioactive decay, most of the mass of the isotopes in the universe are thought to have been produced in the Big Bang.
Deuterium peaks around seconds after the Big Bang, and is then rapidly swept up into helium nuclei. Real space-time, in accordance with this picture, has 26 or 10 space-time dimensions, but all of these dimensions except the usual four are somehow compacted or curled up to a size comparable to the Planck scale.
Isotropic means that all directions appear the same; this property of the universe is well established by observations that show the effective temperature of the cosmic microwave background is identical in all directions to one part in ,The authors of this volume have been intimately connected with the conception of the Big Bang model since Following the late George Gamow's ideas in and more particularly in that the early universe was an appropriate site for the synthesis of the elements, they became deeply involved in the question of cosmic nucleosynthesis and particularly the synthesis of the light elements.
Big Bang nucleosynthesis produced no elements heavier than lithium. To do that you need stars, which means waiting around for at least billion years.
we are all made of stars. More than ninety per cent of the universe is composed of hydrogen and helium. Both elements have been around since shortly after the beginning of the universe.
The very early universe Inhomogeneous nucleosynthesis. One possible modification concerns models of so-called inhomogeneous nucleosynthesis. The idea is that in the very early universe (the first microsecond) the subnuclear particles that later made up the protons and neutrons existed in a free state as a quark-gluon ltgov2018.com the universe expanded and cooled, this quark-gluon plasma would.
Evidence for stars forming just million years after Big Bang Most distant oxygen ever detected in the universe Date: May 16, Source: ESO Summary. Since the Big Bang, billion years ago, the universe has passed through many different phases or epochs. Due to the extreme conditions and the violence of its very early stages, it arguably saw more activity and change during the first second than in all the billions of years since.
Outline. 0) Introduction a) Purpose of this FAQ b) General outline c) Further sources for information 1) What is the Big Bang theory? a) Common misconceptions about the Big Bang b) What does the theory really say?
c) Contents of the universe d) Summary: parameters of the Big Bang Theory 2) Evidence a) Large-scale homogeneity b) Hubble diagram c) Abundances of light elements.Download