1. The total linear moment um is(a) conserved(b) non-conserved (c) impose(d) non-impose2. The generalized moment um isƏL(а) р; —(b) р; — тӑ,(c) Pj = mq;ƏL(d) р; —3. For hyperbolic orbit the values of energy E and eccentricity ɛ are(a) E = 0 and ɛ > 1(b) E > 0 and ɛ > 1(c) E > 0 and ɛ = 1(d) E > 0 and e = 04. The latitude of a place where the plane of vibration of a pendulum rotat es once aday is(а) 90°(b) 60°(c) 45°(d) 30°5. The Lagrange's equations of motion for a sy stem is equivalent to.of motion..equat ions(a) Newt on's(b) Laplace(c) Poisson(d) Maxwell's6. In a cycloe the wind whirls in thesense in the nort hern hemisphere(a) upwards(b) downwards(c) clockwise(d) anticlockwise7. The n-dimensional space is calledspace(a) solar(b) configuration(с) real(d) zeroMathematicsAn alytical Mechanics (Math-363)Page 2 of 28. Generalized coordinates(a) Depends on each other(b) Independent on each ot her(c) necessarily spherical coordinat es(d) May be Cart esian coordinat e9. particle is constrained to move along the inner surface of a hemisphere number ofdegrees of freedom of the particle(a) 1(b) 2(c) 3(d) 410. Constraints that can be expressed as equations of coordinates and time, i.e., by anexpression of the formf (r1, r2, r3, · · · , t) = 0,are said to be(a) holonomic(b) nonholonomic(c) scleronomous(d) Hieronymus

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1. The total linear moment um is (a) conserved (b) non-conserved (c) impose (d) non-impose

Classical Dynamics of Particles and Systems

5th Edition

ISBN:9780534408961

Author:Stephen T. Thornton, Jerry B. Marion

Publisher:Stephen T. Thornton, Jerry B. Marion

Chapter8: Central-force Motion

Section: Chapter Questions

Problem 8.4P

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