复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 20 The special theory of relativity

Chapter 20 The special theory of relativity Albert Einstein(1879-1955)
Chapter 20 The special theory of relativity Albert Einstein ( 1879 ~ 1955 )

20-1 Troubles with classical physics The kinematics developed by galileo and the mechanics developed by Newton, which form the basis of what we call"classical physics, had many triumphs. However, a number of experimental phenomena can not be understood with these otherwise successful classical theories 1. Troubles with our ideas about time The pions( or z created at rest are observed
20-1 Troubles with classical physics The kinematics developed by Galileo and the mechanics developed by Newton, which form the basis of what we call “classical physics”, had many triumphs. However, a number of experimental phenomena can not be understood with these otherwise successful classical theories. 1. Troubles with our ideas about time The pions ( or ) created at rest are observed + −

to decay( to other particles)with an average lifetime of only 26.0ns In one particular experiment, pions were created in motion at a speed ofv=0.913c. In this case they were observed to travel in the laboratory an average distance of D=17.4m before decaying, from which we conclude that they decay in a time given by D/=637ns, much larger than the lifetime measured for pions at rest This effect. called time dilation", which cannot be explained by Newtonian physics. In Newtonian physics time is a universal coordinate having identical values for all observers
to decay ( to other particles ) with an average lifetime of only . In one particular experiment, pions were created in motion at a speed of . In this case they were observed to travel in the laboratory an average distance of before decaying, from which we conclude that they decay in a time given by , much larger than the lifetime measured for pions at rest. This effect, called “time dilation”, which cannot be explained by Newtonian physics. In Newtonian physics time is a universal coordinate having identical values for all observers. 26.0ns v = 0.913c ns v D = 63.7 D =17.4m

2. Trouble with our ideas about length Suppose an observer in the above laboratory placed one marker at the location of the pion's formation and another at the location of its decay The distance between the markers is measured to be 17.4m. Now consider the observer who is traveling along with the pion at a speed of u=0.913c This observer, to whom the pion appear to be at rest, measures its lifetime to be 260ns, and the distance between the markers is (0913c)(260×103)=71m Thus two observers measure different value for the same length interval 3. Troubles with our ideas about light
2. Trouble with our ideas about length Suppose an observer in the above laboratory placed one marker at the location of the pion’s formation and another at the location of its decay. The distance between the markers is measured to be 17.4m. Now consider the observer who is traveling along with the pion at a speed of u=0.913c. This observer, to whom the pion appear to be at rest, measures its lifetime to be 26.0ns, and the distance between the markers is Thus two observers measure different value for the same length interval. (0.913c)(26.0 10 ) 7.1m 9 = − 3. Troubles with our ideas about light

20-2 The postulates of special relativity 1. Einstein offered two postulates that form the basis of his special theory of relativity o The principle of relativity: The laws of phys are the same in all inertial reference frames. sics (D The principle of the constancy of the speed of light The speed of light in free space has the same value c in all inertial reference frames 2. The first postulate declares that the laws of physics are absolute, universal, and same for all inertial observers
20-2 The postulates of special relativity 1. Einstein offered two postulates that form the basis of his special theory of relativity. (I) The principle of relativity: “The laws of physics are the same in all inertial reference frames.” (II) The principle of the constancy of the speed of light : “ The speed of light in free space has the same value c in all inertial reference frames.” 2. The first postulate declares that the laws of physics are absolute, universal, and same for all inertial observers

The Second postulate is much more difficult to accept, because it violates ourcommon sense which is firmly grounded in the Galilean kinematics that we have learned from everyday experiences It implies that it is impossible to accelerate a particle to a speed greater than c
The Second postulate is much more difficult to accept, because it violates our “ common sense”, which is firmly grounded in the Galilean kinematics that we have learned from everyday experiences. It implies that “it is impossible to accelerate a particle to a speed greater than c

20-3 Consequences of Einstein' s postulates 1.The relativity of time We consider two observers: S is at rest on the ground, and S is in a train moving on a long straight track at constant speed u relative to s The observers carry identical timing devices, illustrated in Fig 20-4, consisting of a flashing light bulb F attached to a detector d and separated by a distance Lo from a mirror m The bulb emits a flash of light that travels to the mirror when the reflected light returns to d, the clock ticks and another flash is triggered
20-3 Consequences of Einstein’s postulates 1.The relativity of time We consider two observers: S is at rest on the ground, and S’ is in a train moving on a long straight track at constant speed u relative to S. The observers carry identical timing devices, illustrated in Fig 20-4, consisting of a flashing light bulb F attached to a detector D and separated by a distance from a mirror M. The bulb emits a flash of light that travels to the mirror, when the reflected light returns to D, the clock ticks and another flash is triggered. L0

The time interval At between ticks is 2L (20-1) The interval At is observed by either s or s when the FD clock is at rest respect to that observer Fig 20-4
The time interval between ticks is: (20-1) The interval is observed by either S or S’ when the clock is at rest respect to that observer. M F D Fig 20-4 L0 0 t c L t 0 0 2 = 0 t

We now consider the situation when one observer looks at a clock carried by the other. Fig 20-5 shows that s observes on the clock carried by s on the moving train B L Fig 20-5 FIDI S FID uAt s
We now consider the situation when one observer looks at a clock carried by the other. Fig 20-5 shows that S observes on the clock carried by S’ on the moving train. F D S A B C L L ' S ' S ' S ut Fig 20-5 F D F D

According to s, the flash is emitted at A, reflected at b. and detected at c This interva△tis 1s2l2/n2 +(l 2 △ (2020) Substituting for Lo from Eg(20-1)and solving Eq(20-2)for At gives △ △t (/)2 (203)
According to S, the flash is emitted at A, reflected at B, and detected at C. This interval is (20-20) Substituting for from Eq(20-1) and solving Eq(20-2) for gives (20-3) c t L u c L t 2 2 0 ) 2 2 ( 2 + = = 2 0 1 ( ) c u t t − = t t L0
按次数下载不扣除下载券;
注册用户24小时内重复下载只扣除一次;
顺序:VIP每日次数-->可用次数-->下载券;
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 24 Entropy and the second law of thermodynamics.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 18 Wave Motion.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 14 Gravitation.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)7.4 热力学第二定律.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)7.3 循环过程 卡诺循环.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)7.2.2 理想气体的等温过程和绝热过程.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)7.2.1 理想气体的等容过程和等压过程.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)7.1.2 热力学第一定律.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)7.1.1 准静态过程 功 热量.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)6.3 麦克斯韦气体分子速率分布定律.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)6.2 理想气体的压强公式.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)6.1 状态、过程与理想气体.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)3.3 完全弹性碰撞 完全非弹性碰撞.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)3.1-3.2 功与功率、几种常见力的功.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)2.6.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)2.5 角动量定理角动量守恒定律.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)2.4 转动惯量和力矩.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)2.3 动量守恒定律.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)2.2.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件)2.1 牛顿定律的应用举例.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 10 Angular momentum.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 6 Momentum.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 5 Applications of Newton’s Law.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 3 Force and Newton’s laws.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 21 Temperature.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 0 Preface.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 2 Motion in one dimension.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 1 Measurement.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Ch.11 Energy I:Work and kinetic energy.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Ch.12 Energy II:Potential energy.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 23 The first law of thermodynamics.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 9 Rotational dynamics.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 17 Oscillations.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 22 Molecular properties of gases.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 19 Sound waves.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 8 Rotational kinematics.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 7 Systems of particles.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Chapter 4 Motion in two and three dimensions.ppt
- 复旦大学:《大学物理》课程教学资源(PPT课件,英文)Ch.13 Energy III:Conservation of energy.ppt
- 复旦大学:《高分子物理》课程电子讲义_第一章 导论、第二章 高分子的大小和形状.pdf