11讲:功动能势能保守势力的机械能守恒定律牛顿万有引力定律Lecture 11: Work - Kinetic Energy - Potential Energy - Conservative Forces - Conservation of Mechanical Energy - Newton's Law of Universal Gravitation |
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课程网址: | http://videolectures.net/mit801f99_lewin_lec11/ |
主讲教师: | Walter H. G. Lewin |
开课单位: | 麻省理工学院 |
开课时间: | 2008-10-10 |
课程语种: | 英语 |
中文简介: | ** 1。 1D工作和动能:**引入工作方程及其单位。推导出工作能量定理,表明动能的变化等于通过所有力的总和(因此净力)对粒子进行的工作。重力对向上抛出的物体进行负面工作,直到达到其轨迹的最大高度。 ** 2。以3维计算的工作:**显示3D工作分解为每个1D组件的总和。 ** 3。重力是一种保守力:**通过重力完成的工作,而粒子向上移动一个垂直距离h是-mgh,无论采用何种路径。当力量完成的工作与路径无关时,该力量称为保守力量。 ** 4。当重力是唯一的力量时:**通过重新排列工作能量定理引入重力势能方程。势能和动能可以来回转换,但如果仅涉及保守力,它们的总和即机械能是守恒的。摩擦不是一种保守的力量。当摩擦受到威胁时,可以应用工作能量定理,但不保留机械能。 ** 5。重要的是势能的差异:**重力势能可以是正的,负的或零,这取决于你选择的原点。选择原点在哪里都没关系。 ** 6。过山车,倒置:**机械能守恒用于分析过山车上物体的速度。当过山车颠倒时,向心加速度必须大于g;因此,机械能必须超过阈值。 ** 7。牛顿万有引力定律:引入了牛顿万有引力定律。重力在距离平方上下降。如果涉及大的距离,则由于质量M的物体引起的重力势在无穷远处被认为是零。引力势与M成正比,与M的距离成反比。这种形式与地球表面附近使用的小距离近似是一致的。 ** 8。保护机械能和破坏球:**破坏球将重力势能转换为动能和来回。如果以零速度释放,则破坏球在释放时不应高于其高度。 Lewin教授通过展示这一点来说明他的生活。 |
课程简介: | **1. 1D Work and Kinetic Energy:** The equation for work, and its units are introduced. The work-energy theorem is derived showing that the change in kinetic energy equals the work done on a particle by the sum of all forces (thus the net force). Gravity does negative work on an object thrown upwards until it reaches its maximum height of its trajectory. **2. Work Calculated in 3-Dimensions:** Work in 3D is shown to decompose into the sum of each 1D component. **3. Gravity is a Conservative Force:** Work done by gravity while a particle moves upwards a vertical distance h is -mgh, regardless of the path taken. When the work done by a force is independent of the path, that force is called a conservative force. **4. When Gravity is the only Force:** The equation for gravitational potential energy is introduced by rearranging the work-energy theorem. Potential energy and kinetic energy can be converted back and forth but their sum, the mechanical energy, is conserved if only conservative forces are involved. Friction is not a conservative force. When friction is at stake, the work-energy theorem can be applied, but mechanical energy is not conserved. **5. What Matters is the Difference in Potential Energy:** Gravitational potential energy can be positive, negative or zero depending on your choice of origin. It really doesn't matter where you choose the origin. **6. A Roller Coaster, Upside-down:** The conservation of mechanical energy is used to analyze the velocity of an object on a roller coaster. The centripetal acceleration, when the roller coaster is upside down, must be greater than g; the mechanical energy must therefore exceed a threshold value. **7. Newton's Law of Universal Gravitation:** Newton's law of universal gravitation is introduced. The gravitational force falls off as one over the distance squared. If large distances are involved, the gravitational potential due to an object of mass M is taken to be zero at infinity. The gravitational potential is proportional to M and inversely proportional to the distance from M. This formalism is consistent with the small distance approximation used near the Earth's surface. **8. Conservation of Mechanical Energy and a Wrecking Ball:** A wrecking ball is converting gravitational potential energy into kinetic energy and back and forth. If released with zero speed, the wrecking ball should NOT swing higher than its height when it was released. Professor Lewin puts his life on the line by demonstrating this. |
关 键 词: | 牛顿万有引力定律; 机械能; 保守力 |
课程来源: | 视频讲座网 |
最后编审: | 2020-06-29:zyk |
阅读次数: | 130 |