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Synopsis • This brief guidebook assists you in mastering the difficult concept of pushing electrons that is vital to your success in Organic Chemistry. With an investment of only 12 to 16 hours of self-study you can have a better understanding of how to write resonance structures and will become comfortable with bond-making and bond-breaking steps in organic mechanisms. A paper-on-pencil approach uses active involvement and repetition to teach you to properly push electrons to generate resonance structures and write organic mechanisms with a minimum of memorization.
Compatible with any organic chemistry textbook. SpartanModel replaces the plastic models used by past generations of organic chemistry students. This set of easy-to-use digital builders allows you to construct and manipulate 3-D molecules of any size or complexity.
Each copy includes software on CD-ROM, an extensive molecular database, 3-D glasses, and a Tutorial and User's Guide with 50 pages of activities for organic chemistry.
• • • The energy released from a detonated in the can be divided into four basic categories: • —40–50% of total energy • —30–50% of total energy • —5% of total energy (more in a ) • —5–10% of total energy with the mass of the explosion Depending on the design of the weapon and the environment in which it is detonated the energy distributed to these categories can be increased or decreased. The blast effect is created by the coupling of immense amounts of energy, spanning the, with the surroundings. Locations such as submarine,,, or exo-atmospheric determine how much energy is produced as blast and how much as radiation. In general, denser media around the bomb, like water, absorb more energy, and create more powerful while at the same time limiting the area of its effect. When an air burst occurs, lethal blast and thermal effects proportionally scale much more rapidly than lethal radiation effects, as higher and higher yield nuclear weapons are used. The physical-damage mechanisms of a nuclear weapon (blast and thermal radiation) are identical to those of conventional explosives, but the energy produced by a nuclear explosive is millions of times more powerful per gram and the temperatures reached are briefly in the tens of millions of degrees.
Energy from a nuclear explosive is initially released in several forms of penetrating radiation. When there is a surrounding material such as air, rock, or water, this radiation interacts with and rapidly heats it to an equilibrium temperature (i.e. So that the matter is at the same temperature as the atomic bomb's matter). This causes of surrounding material resulting in its rapid expansion. Created by this expansion contributes to the formation of a shockwave.
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When a nuclear detonation occurs in air near sea level, much of the released energy interacts with the atmosphere and creates a shockwave which expands spherically from the center. Intense thermal radiation at the hypocenter forms a and if the burst is low enough, it is often associated with a. In a burst at high altitude, where the air density is low, more energy is released as ionizing gamma radiation and x-rays than an atmosphere-displacing shockwave.
In 1942 there was some initial speculation among the scientists developing the first nuclear weapons that there might be a possibility of igniting the Earth's atmosphere with a large enough. This would concern a nuclear reaction of two nitrogen atoms forming a carbon and an oxygen atom, with release of energy. This energy would heat up the remaining nitrogen enough to keep the reaction going until all nitrogen atoms were consumed. Was assigned the task of studying whether there was a possibility in the very early days, and concluded there was no possibility due to inverse cooling of the fireball., a mathematician, was asked to make a similar calculation just before, with the same result. Nevertheless, the notion has persisted as a rumor for many years, and was the source of at the Trinity test.