標(biāo)題: Titlebook: Classical Mechanics; Matthew J. Benacquista,Joseph D. Romano Textbook 2018 Springer International Publishing AG 2018 Textbook Classical Me [打印本頁(yè)] 作者: NK871 時(shí)間: 2025-3-21 16:26
書(shū)目名稱(chēng)Classical Mechanics影響因子(影響力)
作者: Devastate 時(shí)間: 2025-3-21 23:10
Brooks A. Keel,Tammie K. SchalueIn this chapter, we extend our analysis of motion to rigid bodies—i.e., bodies having spatial extent, but which have a fixed shape, unchanged by any forces or torques that might act on them. We develop the kinematical framework needed for describing the complicated translational and rotational motion of a rigid body as it moves through space.作者: chlorosis 時(shí)間: 2025-3-22 00:44 作者: Flat-Feet 時(shí)間: 2025-3-22 06:33 作者: 不可知論 時(shí)間: 2025-3-22 09:35
Lisa Campo-Engelstein,Paul BurcherIn this chapter we introduce the basic concepts of special relativity—i.e., spacetime, 4-vectors, the relativistic form of Newton’s 2nd law, and the relativistic Lagrangian formulation, which could serve as the starting point for a course devoted to relativity or relativistic dynamics.作者: 我就不公正 時(shí)間: 2025-3-22 15:31 作者: 我就不公正 時(shí)間: 2025-3-22 18:33
Rigid Body Kinematics,In this chapter, we extend our analysis of motion to rigid bodies—i.e., bodies having spatial extent, but which have a fixed shape, unchanged by any forces or torques that might act on them. We develop the kinematical framework needed for describing the complicated translational and rotational motion of a rigid body as it moves through space.作者: enflame 時(shí)間: 2025-3-22 21:52
Small Oscillations,In this chapter, we will apply the Lagrangian formalism to the general case of coupled .-body systems perturbed from equilibrium. We will first look at the simple one-dimensional oscillator as a refresher, and then go on to develop the general formulation of the problem, applying it to solve a few simple example problems.作者: 憲法沒(méi)有 時(shí)間: 2025-3-23 01:34 作者: 作嘔 時(shí)間: 2025-3-23 08:47 作者: overhaul 時(shí)間: 2025-3-23 12:18
https://doi.org/10.1007/978-3-319-68780-3Textbook Classical Mechanics; Textbook Mechanics Physics; Analytical Mechanics textbook; Hamilton Prici作者: 青少年 時(shí)間: 2025-3-23 17:44
978-3-319-68779-7Springer International Publishing AG 2018作者: condemn 時(shí)間: 2025-3-23 21:15 作者: HEAVY 時(shí)間: 2025-3-24 00:31
Javier S. Castresana,Paula Lázcozn also be obtained by finding the stationary values of a functional, called the “action.” By doing so, we convert the problem of finding the equations of motion to a problem in the calculus of variations. We also introduce the Hamiltonian for a system of particles, which can be obtained from the Lag作者: opalescence 時(shí)間: 2025-3-24 04:18
Pedro J. Chedrese,Stella M. Celucheld outside the charge is nearly always a radial field if the particle can be considered to be a dimensionless point. Examples include the classical Newtonian law of gravitation, the electrostatic field, and the Yukawa model of the strong nuclear force. The common feature in these examples is a sphe作者: certitude 時(shí)間: 2025-3-24 09:31
Computer Assisted Analysis of Genesc energy that the total energy of the system is positive. In this chapter, we develop the tools needed to calculate the deflection angles of two particles as a function of the impact parameter and initial velocity of the incoming particle.作者: STEER 時(shí)間: 2025-3-24 11:27 作者: BACLE 時(shí)間: 2025-3-24 16:35 作者: 政府 時(shí)間: 2025-3-24 22:22
Matthew J. Benacquista,Joseph D. RomanoContains an early introduction of D’Alembert’s principle, variational principles and Lagrangian & Hamiltonian mechanics.Provides an ideal blend of general concepts and methods which are then applied t作者: 明確 時(shí)間: 2025-3-25 02:20 作者: 不開(kāi)心 時(shí)間: 2025-3-25 05:52
Scattering,c energy that the total energy of the system is positive. In this chapter, we develop the tools needed to calculate the deflection angles of two particles as a function of the impact parameter and initial velocity of the incoming particle.作者: 鳥(niǎo)籠 時(shí)間: 2025-3-25 09:59
Rigid Body Dynamics,ional motion of a rigid body as it moves through space. In particular, we derive Euler’s equations for rigid body motion, which extend the familiar first-year physics equations to general rotations in three dimensions around an axis that can change its orientation in response to external forces. We then apply Euler’s equations to several examples.作者: 酷熱 時(shí)間: 2025-3-25 14:15 作者: 簡(jiǎn)略 時(shí)間: 2025-3-25 17:45 作者: evasive 時(shí)間: 2025-3-25 20:00
Classical Mechanics978-3-319-68780-3Series ISSN 2192-4791 Series E-ISSN 2192-4805 作者: 縫紉 時(shí)間: 2025-3-26 02:54
Computer Assisted Analysis of Genesc energy that the total energy of the system is positive. In this chapter, we develop the tools needed to calculate the deflection angles of two particles as a function of the impact parameter and initial velocity of the incoming particle.作者: outrage 時(shí)間: 2025-3-26 06:50
Jessie Dorais,C. Matthew Petersonional motion of a rigid body as it moves through space. In particular, we derive Euler’s equations for rigid body motion, which extend the familiar first-year physics equations to general rotations in three dimensions around an axis that can change its orientation in response to external forces. We then apply Euler’s equations to several examples.作者: NAV 時(shí)間: 2025-3-26 09:19
Allan J. Jacobs,Kavita Shah Aroracribe the oscillatory motion of strings, membranes, and solid objects. We discuss both the eigenfunction and normal form solutions of the wave equation, paying particular attention to various boundary conditions and initial conditions.作者: orthodox 時(shí)間: 2025-3-26 15:17 作者: 內(nèi)部 時(shí)間: 2025-3-26 19:29
,Hamilton’s Principle and Action Integrals,n also be obtained by finding the stationary values of a functional, called the “action.” By doing so, we convert the problem of finding the equations of motion to a problem in the calculus of variations. We also introduce the Hamiltonian for a system of particles, which can be obtained from the Lag作者: 虛度 時(shí)間: 2025-3-26 23:08
Central Force Problems,eld outside the charge is nearly always a radial field if the particle can be considered to be a dimensionless point. Examples include the classical Newtonian law of gravitation, the electrostatic field, and the Yukawa model of the strong nuclear force. The common feature in these examples is a sphe作者: resilience 時(shí)間: 2025-3-27 03:11
Scattering,c energy that the total energy of the system is positive. In this chapter, we develop the tools needed to calculate the deflection angles of two particles as a function of the impact parameter and initial velocity of the incoming particle.作者: FIR 時(shí)間: 2025-3-27 06:45
Rigid Body Dynamics,ional motion of a rigid body as it moves through space. In particular, we derive Euler’s equations for rigid body motion, which extend the familiar first-year physics equations to general rotations in three dimensions around an axis that can change its orientation in response to external forces. We 作者: 過(guò)度 時(shí)間: 2025-3-27 10:49 作者: conference 時(shí)間: 2025-3-27 13:53
Textbook 2018This text describes the background and tools for use in the fields of modern physics, such as quantum mechanics, astrophysics, particle physics, and relativity. Students who have had basic undergraduate classical mechanics or who have a good understanding of the mathematical methods of physics will 作者: 地牢 時(shí)間: 2025-3-27 19:09
2192-4791 as quantum mechanics, astrophysics, particle physics, and relativity. Students who have had basic undergraduate classical mechanics or who have a good understanding of the mathematical methods of physics will benefit from this book..978-3-319-68779-7978-3-319-68780-3Series ISSN 2192-4791 Series E-ISSN 2192-4805 作者: cluster 時(shí)間: 2025-3-28 00:02 作者: enchant 時(shí)間: 2025-3-28 05:38
Holly A. LaVoie,Pedro J. Chedrese Lagrange’s equations of the 1st and 2nd kind. We shall see that the Lagrangian formulation of mechanics allows us to analyze problems that are much harder to solve when approached with a direct application of Newton’s laws.作者: 擋泥板 時(shí)間: 2025-3-28 09:15
Pedro J. Chedrese,Stella M. Celuchewtonian law of gravitation, the electrostatic field, and the Yukawa model of the strong nuclear force. The common feature in these examples is a spherically-symmetric potential that depends only on the radial separation from the point-particle source of the field. In this chapter, we will focus on mostly on gravitationally-bound systems.作者: 褪色 時(shí)間: 2025-3-28 11:23 作者: FID 時(shí)間: 2025-3-28 18:00 作者: finite 時(shí)間: 2025-3-28 22:18 作者: 僵硬 時(shí)間: 2025-3-28 23:53
,Hamilton’s Principle and Action Integrals,the generalized coordinates and momenta. The Hamiltonian formulation is particularly well-suited for illustrating the intimate connection between continuous symmetries of the system and conserved quantities.作者: 很是迷惑 時(shí)間: 2025-3-29 03:05
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