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Cosmic Hide and Seek: the Search for the Missing
Cosmic Hide and Seek: the Search for the Missing

... galaxies by measuring their brightness. When he used a different method to compute the mass of the same cluster of galaxies, he came up with a number that was 400 times his original estimate (1). This discrepancy in the observed and computed masses is now known as "the missing mass problem." Nobody ...
faster than light - Site officiel de l`Association Savoir sans
faster than light - Site officiel de l`Association Savoir sans

... a sort of plate, that they called THE GREAT WALL. In other words, in this "plate" there were lots of galaxies and around it it was empty? Page 3 As the years passed their observations became more precise. Today we know that galaxies, matter, are set around great empty bubbles of a hundred million li ...
pps - TUM
pps - TUM

... • One or more supernovae 2-3 Mys ago could be responsible (~40 pc distance) • Excess of 60Fe has also been found in lunar samples, but analysis still ongoing • Search for 60Fe in magnetofossils in marine sediment is ongoing ...
Science Implications of Various Servicing Options
Science Implications of Various Servicing Options

... Hubble Has Improved Over Time • Servicing missions have improved Hubble’s vision. • Hubble sees farther and with greater clarity than ...
Eternal Inflation
Eternal Inflation

... In the standard big bang theory there is no explanation whatever for this uniformity. In fact, one can even show that within the context of the standard big bang theory, no explanation for this uniformity is possible. To see this, we need to understand a little about how this cosmic background radia ...
Post-AGB stars in the Magellanic Clouds and neutron
Post-AGB stars in the Magellanic Clouds and neutron

... updated to those calculated by Lederer & Aringer (2009). Mass loss was included using the formula of Reimers (1975) during the RGB phase (with η = 0.4) and the formula of Vassiliadis & Wood (1993) during the AGB phase. Instantaneous mixing was used in convective zones, and the convective boundaries ...
Dark Energy: how the paradigm shifted
Dark Energy: how the paradigm shifted

... pave the way to the acceptance of dark energy. It would be tempting to think that the path to dark energy was now clear. However, astronomers realized that the mean mass density of the universe could still be as high as the critical density if there was a lot of extra dark matter hidden in the vast ...
The hot, early universe - Cosmology Block
The hot, early universe - Cosmology Block

... 4 The cosmic background radiation ...
n - Indico
n - Indico

... Reduce the nuclear physics uncertainty from 7% to 5% and measure CNO neutrinos (15O) with 10% uncertainty allow to determine solar metallicity with 17% accuracy (now >30%) ...
6 The Uncreated Universe - Mukto-mona
6 The Uncreated Universe - Mukto-mona

... force as far back in time as we have been able, so far, to peer. However, while we cannot look directly into the heart of the early universe, our existing knowledge can be used to infer the physical processes that took place within a tiny fraction of a second after the start of things––over ten bill ...
Neutron Density and Neutron Source Determination in Barium
Neutron Density and Neutron Source Determination in Barium

... Figure 1 displays a comparison of the observed MgH spectra of HO 178717 in the 5101 Aregion with synthetic spectra calculated for different distributions of the magnesium isotopes. The strength of C2 was estimated by fitting the profile of the C2 line at 5086 A. The calculation with the magnesium is ...
Dynamics of neutrino-driven winds: inclusion of accurate weak
Dynamics of neutrino-driven winds: inclusion of accurate weak

... Roberts et al. (2010). As can be seen, the mass outflow rate increases with the anti-neutrino luminosity, and the MF enhances the total mass of the NDW. r-element distribution patterns depend on the entropy, expansion timescale and electron fraction. For the nucleon entropy, we found that it changes ...
speech on dark matter
speech on dark matter

... problems with our comprehension of the universe that we exist in. Before my studies I (somewhat naively perhaps) assumed that after the existence and findings of great minds such as Aristotle, Galileo, and Einstein, that we’d pretty much figured everything out by now, and that a modern day physicist ...
Word - The Open University
Word - The Open University

... reduced. This has important implications for the ways in which the four fundamental interactions manifest themselves at different epochs. The four fundamental interactions, that is electromagnetic interaction, weak interaction, strong interaction and gravitational interaction, have very different st ...
CBO_Paper2_UnderstandingtheStoryOfTheUniverse
CBO_Paper2_UnderstandingtheStoryOfTheUniverse

... is hydrogen itself.7 Through observations, astronomers realized that the abundance of baryonic particles are proportional to each other. By studying the amount of different baryonic particles in the Universe, cosmologists realized that not all matter must be baryonic. Therefore, cosmologists believe ...
Evolution of the universe
Evolution of the universe

... chemical elements in stars. ...
1/2 - Indico
1/2 - Indico

... since then is equal to the ratio of galaxy’s distance and its velocity. Since this ratio is 1/H which is same for all the galaxies, all of them must have been crowded together at the same ancient time. In other words, at some unique time in the past all the matter in the universe was compressed to a ...
Lec16_2D
Lec16_2D

...  Since the galaxies are moving away from each other, gravity will not necessarily cause a big collapse. So a finite universe is possible.  The larger the distance, the larger the velocity. Galaxies at the other end of the universe have their light Doppler shifted out of the optical. No wonder the ...
What is the Shape of the Universe?
What is the Shape of the Universe?

... distance, all stars 2 billion L.Y. away are receding at a rate of 1/7 of a L.Y. per year  Thus, these stars, too, must have been where we were 14 billion years ago ...
Document
Document

... Meteorites can provide accurate information on elemental abundances in the presolar nebula. More precise than solar spectra if data in some cases. Principal source for isotopic information. But some gases escape and cannot be determined this way (for example hydrogen, or noble gases) Not all meteori ...
Light n-Capture Element Abundances in Metal
Light n-Capture Element Abundances in Metal

... origins. The lightest of these, Hydrogen, Helium and a fraction of the Universe’s Lithium were made within a few minutes after the Big Bang. Beryllium and Boron are created in the interstellar clouds of gas and dust during collisions between cosmic rays and gas nuclei. The other elements were create ...
Astronomy 112: The Physics of Stars Class 8 Notes: Nuclear
Astronomy 112: The Physics of Stars Class 8 Notes: Nuclear

... Z C, where A is the atomic weight, Z is the atomic number, and C is the symbol for that element. This is slightly redundant, since a chemical symbol C uniquely identifies the atomic number Z. However, writing out the numbers explicitly makes it easier to keep track of the charges, and to assure ours ...
Nuclear Structure Studies of Neutron
Nuclear Structure Studies of Neutron

... CH2 target placed at the center of the Cristal Ball gamma array [22]. It decayed in-flight by the emission of a neutron (26 F (3+ ) →25 F+n ), that was detected at forward angles in the segmented neutron array LAND. The momentum vector of the residue 25 F, determined at the dispersive focal plane of ...
Document
Document

... does now and hasn’t changed. The trouble is that the night sky would be completely lit up because of the billions of stars, but it’s not, so… The “Big Bang” theory This theory states that the universe started off with an explosion and everything has been moving away ever since. There are two main pi ...
Nucleosynthesis of heavy elements in gamma ray bursts
Nucleosynthesis of heavy elements in gamma ray bursts

... central engine gives rise to the powerful, ultra-relativistic jets that are responsible for energetic gamma ray emission, as well as to the winds launched with smaller velocities from the accretion disk. We consider the hyperaccreting disks and outflows from Gamma Ray Bursts. The torus is composed o ...
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Big Bang nucleosynthesis

In physical cosmology, Big Bang nucleosynthesis (abbreviated BBN, also known as primordial nucleosynthesis) refers to the production of nuclei other than those of the lightest isotope of hydrogen (hydrogen-1, 1H, having a single proton as a nucleus) during the early phases of the universe. Primordial nucleosynthesis is believed by most cosmologists to have taken place from 10 seconds to 20 minutes after the Big Bang, and is calculated to be responsible for the formation of most of the universe's helium as the isotope helium-4 (4He), along with small amounts of the hydrogen isotope deuterium (2H or D), the helium isotope helium-3 (3He), and a very small amount of the lithium isotope lithium-7 (7Li). In addition to these stable nuclei, two unstable or radioactive isotopes were also produced: the heavy hydrogen isotope tritium (3H or T); and the beryllium isotope beryllium-7 (7Be); but these unstable isotopes later decayed into 3He and 7Li, as above.Essentially all of the elements that are heavier than lithium and beryllium were created much later, by stellar nucleosynthesis in evolving and exploding stars.
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