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Why a wiki? Initially, we had thought of writing a review paper to cover this topic, and thought of writing it in an online form initially to allow people to provide input as we wrote. Ultimately, we want these pages to provide both a concise introduction to the necessary background knowledge for getting these calculations to work, and a set of tutorials to help even beginners set them up. Our goal in setting up is to provide an accessible point of entry to free energy calculations. Recent literature seems to suggest that these calculations (when done well) are reaching the point where the results can be high quality, and that a main barrier to their more widespread use is the difficulty of setting them up and the amount of expertise required. This is the key to chemical change.Free energy calculations have historically been "experts-only" territory because they are difficult to set up, difficult to do well, and sometimes even difficult to analyze. To fill its outer shell an atom may get electrons from another atom, and, as a result, form what is called a "bond" with the other atom. For most atoms eight electrons will fill this outer shell, but this isn't true for most single atoms. For any atom is most stable if its outer electron shell is full. It is the arrangement of electrons around an atom that decides how and when the atom will take part in a chemical change. Atoms with only a few electrons will use only a small number of shells, and those with many electrons have a lot of shells. Electrons are arranged in different layers, called "shells." We can see these shells more clearly if we flatten them out. Every atom of uranium has ninety-two electrons. Every atom of hydrogen has only one electron.
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NARRATOR: If we could see an atom it might look something like this: the fuzziness represents the paths of very fast-moving particles called "electrons." Electrons orbit the central part of the atom, called the "nucleus." An atom may have only one electron, or it may have many, but every different kind of atom has a different number of electrons in orbit around its nucleus. SpaceNext50 Britannica presents SpaceNext50, From the race to the Moon to space stewardship, we explore a wide range of subjects that feed our curiosity about space!.Learn about the major environmental problems facing our planet and what can be done about them! Saving Earth Britannica Presents Earth’s To-Do List for the 21st Century.Britannica Beyond We’ve created a new place where questions are at the center of learning.100 Women Britannica celebrates the centennial of the Nineteenth Amendment, highlighting suffragists and history-making politicians.COVID-19 Portal While this global health crisis continues to evolve, it can be useful to look to past pandemics to better understand how to respond today.Student Portal Britannica is the ultimate student resource for key school subjects like history, government, literature, and more.From tech to household and wellness products. This Time in History In these videos, find out what happened this month (or any month!) in history.#WTFact Videos In #WTFact Britannica shares some of the most bizarre facts we can find.Demystified Videos In Demystified, Britannica has all the answers to your burning questions.
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