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Mecánica Clásica (Dourmashkin)

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    Históricamente, un conjunto de conceptos centrales —espacio, tiempo, masa, fuerza, impulso, torque y momento angular— se introdujeron en la mecánica clásica con el fin de resolver el problema físico más famoso, el movimiento de los planetas. Los principios de la mecánica describieron con éxito muchos otros fenómenos encontrados en el mundo. Las leyes de conservación que involucran energía, impulso e impulso angular proporcionaron un segundo enfoque paralelo para resolver muchos de los mismos problemas. En este curso, investigaremos ambos enfoques: Leyes de fuerza y de conservación. Nuestro objetivo es desarrollar una comprensión conceptual de los conceptos centrales, una familiaridad con la verificación experimental de nuestras leyes teóricas y una capacidad de aplicar el marco teórico para describir y predecir los movimientos de los cuerpos.

    This page titled Mecánica Clásica (Dourmashkin) is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by Peter Dourmashkin (MIT OpenCourseWare) via source content that was edited to the style and standards of the LibreTexts platform.