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Product description

💎💎💎About Moissanite 👉 Harder than emerald, ruby, or sapphire and more brilliant than diamond, moissanite is a gemstone unlike any other. Discovered in a meteorite crater and re-created by the innovators, this stunning stone is known worldwide as The World’s Most Brilliant Gem. With this gem’s hardness second only to diamond, it’s extremely resistant to scratching, abrasion, breaking, or chipping. Each and every piece comes with a Limited Lifetime Warranty which guarantees that every stone will maintain its fire, beauty and brilliance to last forever. Eco-friendly, conflict-free, and affordable, moissanite is truly the brilliant alternative to a diamond. Bid with Confidence Each amp; every Diamond Tester will show as 100 % 9.25 Hardness. COMMENT : No Nicks Or Scratches On The Stone. ◇Moissanite can pass the test of the diamond selector. ◇No One can easily clarify amp; be sure is Diamond or Moissanite. ◇Natural Diamond Hardness is 10 : Moissanite Diamond Hardness is 9.25 : Rubyamp;Emerald 9. ◇Diamond amp; Moissanite maintains its clarity and sparkle throughout a lifetime. ◇Diamond amp; Moissanite has the Same Process for Polish Diamond as a manually. ◇It will not look like a piece of rock salt, like cubic zirconia, after two weeks. ◇The carat is the traditional unit of measurement for a diamond’s weight. Moissanite is not measured in carats because it weighs approximately 10-12 percent less than diamond. For example, a 6.5mm round diamond would weigh 1.0 ct, while a 6.5mm round moissanite would weigh only 0.88 ct. The two stones would be the same size – 6.5mm in diameter. Our moissanite gemstones are listed with their size in mm and may include the diamond equivalent weight(DEW) in carats for comparison purposes. ● We take order for the engagement ring, pendants, necklaces, earrings, bracelets and many more. -Any question, just let me know. :) Thank you..💎💎💎

ERAA Jewel Loose Moissanite 1.50CT, Real Colorless Diamond, VVS1

Institute for Computational Cosmology
The Institute for Computational Cosmology (ICC) is a leading international centre for research into the origin and evolution of the Universe at Durham University . We address some of the most fundamental questions in science: What were the first objects in the Universe? How do galaxies form? What is the nature of the dark matter and dark energy? Where does the large-scale structure of the universe come from? What is the fate of the Universe?

Ernest Rutherford Fellowship Applications 2021
We welcome applications for STFC Ernest Rutherford Fellowships. There are quota limits on ERF applications and so we require all applicants to submit a CV using the STFC narrative CV template, publication list, and a short (*strict* 1 page limit) research outline, including a brief additional paragraph (not counted within the 1 page limit) on why Durham and how the project connects to Durham. In addition, please identify (and contact) a member of staff to be your academic host to support you in the preparation of your application. Please ensure that the name of your academic host is included at the top of the research outline. The deadline for these documents is the 5th August 2021 and they should be submitted to astro.secretary@durham.ac.uk.

A summary of our various Fellowship opportunties can be found here.

The ICC is part of the Ogden Centre for Fundamental Physics and interacts closely with the Centre for Extragalactic Astronomy and the Centre for Advanced Instrumentation in the Department of Physics. We offer both PhD and Msc postgraduate studentships.

In November 2016, the ICC moved into the brand new Ogden Centre for Fundamental Physics building, designed by the world renowned Studio Daniel Libeskind. The new building now houses all three astronomy groups in the Department of Physics, including the Centre for Advanced Instrumentation and the Centre for Extragalactic Astronomy, as well as the Institute for Computational Cosmology.

Newsletter: The ICC's May 2015 newsletter is available for download.

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RECENT PUBLICATIONS
SUB-DAMPED LYMAN α SYSTEMS IN THE XQ-100 SURVEY - II. CHEMICAL EVOLUTION AT 2.4 ≤ Z ≤ 4.3
Berg T. A. M., Fumagalli M., D'Odorico V., Ellison S. L., López S., Becker G. D., Christensen L., Cupani G., Denney K. D., Sánchez-Ramírez R., Worseck G.
CHARACTERIZING THE TARGET SELECTION PIPELINE FOR THE DARK ENERGY SPECTROSCOPIC INSTRUMENT BRIGHT GALAXY SURVEY
Ruiz-Macias O., Zarrouk P., Cole S., Baugh C. M., Norberg P., Lucey J., Dey A., Eisenstein D. J., Doel P., Gaztañaga E., Hahn C., Kehoe R., Kitanidis E., Landriau M., Lang D., Moustakas J., Myers A. D., Prada F., Schubnell M., Weinberg D. H., Wilson M. J.
MODELLING THE QUENCHING OF STAR FORMATION ACTIVITY FROM THE EVOLUTION OF THE COLOUR-MAGNITUDE RELATION IN VIPERS
Manzoni G., Scodeggio M., Baugh C. M., Norberg P., De Lucia G., Fritz A., Haines C. P., Zamorani G., Gargiulo A., Guzzo L., Iovino A., Małek K., Pollo A., Siudek M., Vergani D.
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Kelly A. J., Jenkins A., Frenk C. S.

Contact Details

Institute for Computational Cosmology,
Ogden Centre for Fundamental Physics - West,
Department of Physics,
Durham University,
South Road,
Durham DH1 3LE
 
Tel: 44 (0)191 3343635