Fundamentals of Physics Extended (10th Edition) by David Halliday and Robert Resnick 2013 COLOR 30.7MB

Fundamentals of Physics Extended (10th Edition) by David Halliday and Robert Resnick 2013 COLOR 30.7MB
Item# 15121677tbo
Retail price: US$220.00
Sale price: US$15.00

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Fundamentals of Physics Extended (10th Edition) COLOR 30.7MB 2013

The 10th edition of Hallidays Fundamentals of Physics building upon previous issues by offering several new features and additions. The new edition offers most accurate, extensive and varied set of assessment questions of any course management program in addition to all questions including some form of question assistance including answer specific feedback to facilitate success. The text also offers multimedia presentations (videos and animations) of much of the material that provide an alternative pathway through the material for those who struggle with reading scientific exposition. Furthermore, the book includes math review content in both a self-study module for more in-depth review and also in just-in-time math videos for a quick refresher on a specific topic. The Halliday content is widely accepted as clear, correct, and complete. The end-of-chapters problems are without peer. The new design, which was introduced in 9e continues with 10e, making this new edition of Halliday the most accessible and reader-friendly book on the market.

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The front cover shows a simulation of the collisions of the lead-ion beams at CERN, as recorded by the detector ALICE. The collisions produce a plasma of quarks and gluons in a sizable volume, with a density greater than that in a neutron star and with a temperature 100 000 times that in the Sun's core. These conditions match those a few microseconds after the big bang beginning of the universe. In our normal low-energy world, quarks and gluons are always locked up inside the confines of particles such as protons and neutrons. However, in the high-energy collisions within ALICE, they undergo deconfinement to produce the plasma, which is a unique state of matter that acts like an ideal fluid with no viscosity. Such was the state of the universe just after the big bang.