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给研究生的四条金律

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    发表于 2009-5-18 19:39:05 | 显示全部楼层 |阅读模式
    论文文献
    标题: 给研究生的四条金律
    作者: Steven Weinberg
    所属专业方向: Education
    摘要: This essay is based on a commencement talk
    given by the author at the Science Convocation at
    McGill University in June 2003
    关键字:
    来源:

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    Steven Weinberg
    4 r: Z( |$ j" x9 C; W! J# i$ x$ F3 F
    Steven Weinberg is in the Department of Physics,
    ! E" R. i4 ]+ z# }the University of Texas at Austin, Texas 78712,
    + G& A* m: P: B& T$ n; K- LUSA. This essay is based on a commencement talk4 t+ ^0 F6 K* q2 y2 U# s
    given by the author at the Science Convocation at
    + T3 l# W5 z$ I7 {  @$ kMcGill University in June 2003.
    5 k* }% S' s& K5 U' P1 k* E1 `6 I7 y# `  ^/ F
    When I received my undergraduate degree — about a hundred years8 U& z9 A# y; E- f$ C0 |9 o
    ago — the physics literature seemed to me a vast, unexplored ocean,8 M' E9 L$ S% @! U
    every part of which I had to chart before beginning any research of my own. How* V( ?" @0 ^1 J% C' V
    could I do anything without knowing everything that had already been done?8 @0 p; d1 [* O; P
    Fortunately, in my first year of graduate school, I had the good luck to fall into the) r) I! \& a3 ?9 q5 W" o& @
    hands of senior physicists who insisted, over my anxious objections, that I must start
    ! R- w. }' Y) K$ v7 g2 n4 S1 ^doing research, and pick up what I needed to know as I went along. It was sink or
    / `2 m8 `; i* Hswim. To my surprise, I found that thisworks. I managed to get a quick PhD —+ D' ~2 r! {6 h# B, w8 e& b& T
    though when I got it I knew almost nothing about physics. But I did learn one big
    . u6 V0 z8 V0 c8 j$ Z) y! o6 {thing: that no one knows everything, and you don’t have to ./ r' |* s/ S1 _3 x& W
    3 u  y, x  ?' V" S) D8 T
    Another lesson to be learned, to continue
    ! q$ r- o7 N0 \9 E) S! t8 _using my oceanographic metaphor, is that/ F. o# {+ y) L6 S
    while you are swimming and not sinking you
    9 z) |2 v. |& P1 w. x6 g3 C2 i# mshould aim for rough water. When I was
    : h1 M  y( Y  s0 T) tteaching at the Massachusetts Institute of! i' ^- [: W: f: E
    Technology in the late 1960s, a student told
    9 d7 D1 Q, K# q) U' s4 Q7 X! lme that he wanted to go into general8 G# t0 g: K, x/ J2 V
    relativity rather than the area I was working
    ' g0 N6 P4 d, ?# C3 Gon, elementary particle physics, because
    9 ?* Y1 i+ X3 x  `the principles of the former were well; Q2 `2 ]) c( q- q3 t8 j! H
    known, while the latter seemed like a mess
    3 a# s# i$ B; {( J" n3 bto him. It struck me that he had just given
    % v6 n4 a1 z& C) ja perfectly good reason for doing the opposite.- r* f8 z9 S6 d' r
    Particle physics was an area where" ], G9 P  v4 k! L! V- Y
    creative work could still be done. It really was
    4 _  U5 @' h1 N( O) o& q# }6 fa mess in the 1960s, but since that time the# ~3 w( F$ P% I0 [1 h7 [& p
    work of many theoretical and experimental
    . P) r9 C* o4 Zphysicists has been able to sort it out, and! i7 N; ~& I3 R5 ]/ _+ {  V
    put everything (well, almost everything)3 y9 H- ~0 f! A
    together in a beautiful theory known as' k# |7 K0 I$ M/ Y1 {
    the standard model.My advice is to go for the
    4 O% V) `/ e& E9 m& \! j* }messes — that’s where the action is.# R: k: O3 G* i. E+ N. C0 g
    ' v! i  G: n5 h$ J" ^" F
    My third piece of advice is probably the0 L7 H8 p" \; G" K9 j
    hardest to take. It is to forgive yourself for/ v% ~9 Z' C4 y
    wasting time. Students are only asked to  \! s: f: `3 a( `3 k) x! m
    solve problems that their professors (unless
    ' y  n7 J& E$ a2 @$ h) U5 Munusually cruel) know to be solvable. In$ U  K* z; L* x# D; k8 ^' s
    addition,it doesn’t matter if the problems are5 l/ d/ D! o2 G
    scientifically important — they have to be) R6 z/ A( v* U3 L/ y
    solved to pass the course. But in the real9 y+ |: q. y# T8 r+ {
    world, it’s very hard to know which problems
    8 H4 `, L6 ~& ~8 P1 N4 v8 Hare important, and you never know whether
      I0 {2 C3 C/ F! _" Lat a given moment in history a problem is6 A% l9 Z/ }4 H. R/ V
    solvable. At the beginning of the twentieth
    ! d1 i5 w6 z+ v7 Acentury, several leading physicists, including
    - f) R- I- F$ O0 m  ?" y0 }Lorentz and Abraham, were trying to work
    ( B4 B4 _- @- H% e7 mout a theory of the electron. This was partly6 p7 W' u; o3 _& t# b' l) o
    in order to understand why all attempts to1 T* {/ K1 R# m, P
    detect effects of Earth’s motion through the
    : I! k  ~& w$ d  G. _! Yether had failed. We now know that& e* e" h! h$ i9 Y* p1 Z7 p9 c3 y
    they were working on the wrong problem.
    . A3 Z( K: H+ d0 a) ^+ r6 gAt that time, no one could have developed a& _3 E& g9 f0 c7 P: H
    successful theory of the electron, because+ C1 x9 g, |( Z5 R6 W3 c* z
    quantum mechanics had not yet been
    9 [3 v. b& V2 j. u$ gdiscovered. It took the genius of Albert
    1 @/ t0 C2 z2 I  p0 j( `Einstein in 1905 to realize that the right' _. J/ `4 y/ o' S2 Q5 ^
    problem on which to work was the effect# n* _( [6 o# X8 }
    of motion on measurements of space and9 V5 U& u8 u1 k8 o
    time. This led him to the special theory of
    1 h# R6 Y% X) ~+ O) x) Orelativity. As you will never be sure which
    # q$ f+ }/ C8 Z% J7 v. G& aare the right problems to work on, most# t! ^& ~5 L8 G- ?5 V$ F/ a
    of the time that you spend in the laboratory
    6 ~. v7 a: Y$ [, d) \  j1 bor at your desk will be wasted. If you want$ F$ n. c4 a' g7 E. z4 g/ ]
    to be creative, then you will have to get used
    + |( p( @6 j& R, G, {2 u1 x- Jto spending most of your time not being
    4 j5 @) l5 w: V  d9 z/ Ecreative, to being becalmed on the ocean of+ l" m+ _: A; v/ X
    scientific knowledge.
    . E" R/ y* ^9 _. `" T8 v9 t7 h7 M
    Finally, learn something about the history
    $ f1 C2 |, j8 s' ]/ Tof science,or at a minimum the history of your
    5 t. H8 h. _) V9 }own branch of science. The least important, U3 n7 F8 R3 D. C5 N
    reason for this is that the history may actually) [1 x- J  S9 y: }
    be of some use to you in your own scientific
    9 M6 Z6 S4 L  \/ Z1 t. `work. For instance, now and then scientists" i8 R* k- M0 d$ G4 Y% {
    are hampered by believing one of the oversimplified
    5 N- l: C& N, ^/ |$ o) pmodels of science that have
    - Y: [$ H; c* S; ~* R1 k: Nbeen proposed by philosophers from Francis
    . X8 y" r0 @, J% NBacon to Thomas Kuhn and Karl Popper.+ Q& {) p9 F& m& f
    The best antidote to the philosophy of science& v$ G: H( ?: Z  |4 W% b" O2 _
    is a knowledge of the history of science.
    % R( i# V' C- V7 F2 v: PMore importantly, the history of science4 i; n" ?; G, z5 Z4 C& E* h7 W: p& y, g
    can make your work seem more worthwhile
    ! m* R% F: U) J, _% ato you. As a scientist, you’re probably not
    & c( ]5 S/ e, ^' }9 m6 egoing to get rich. Your friends and relatives
    " x8 }% h  D6 k; s# Kprobably won’t understand what you’re$ H) O7 x9 ?) L2 R$ U
    doing.And if you work in a field like elementary
    7 f8 P  N& w+ p( gparticle physics, you won’t even have the% O$ ^# J" m5 M% ~" `
    satisfaction of doing something that is
    / u8 d6 J  [6 t. d; r! H8 }immediately useful. But you can get great
    ! t4 [- T) L7 h6 asatisfaction by recognizing that your work in2 {: O% G9 z; b& k
    science is a part of history.( D1 m$ ]5 b: \8 K9 ?

    : P. B. }; E5 E/ u+ [Look back 100 years, to 1903. How
    5 M7 X% E' M7 m9 }7 f% e1 Y( himportant is it now who was Prime Minister
    ( C/ N. Z2 k: k; O3 Y: T# U. mof Great Britain in 1903, or President of the
    $ d$ d( A) G1 _& n; h& QUnited States? What stands out as really
    4 D$ `7 s$ L  \% f! f1 e1 h" Fimportant is that at McGill University,5 o2 L1 L5 X8 p: Z  L$ i9 x, `- _
    Ernest Rutherford and Frederick Soddy were. \. i1 _0 X. H
    working out the nature of radioactivity.
    " J- {$ k: F# H; c: E% QThis work (of course!) had practical applications,' K8 m* l4 u/ m5 F; d; N( P" x7 k1 S
    but much more important were its
    / R/ E; G' u4 d6 F: Zcultural implications. The understanding of7 H% ]$ x0 ?5 b. q
    radioactivity allowed physicists to explain
    5 C; Q* u- k$ F+ C. o5 Ihow the Sun and Earth’s cores could still be1 R+ D0 n$ Y. q
    hot after millions of years. In this way, it9 @2 M# v- b( P. }1 X" |
    removed the last scientific objection to what4 _) a* N' K5 o% f- K( Q+ i
    many geologists and paleontologists+ P1 t% e/ P% Y3 P  F0 a
    thought was the great age of the Earth and
    ) ?# O& O$ ]) s: a9 j" B; othe Sun.After this,Christians and Jews either
    * l4 x4 b" W# c0 n# \- ~3 ~( Xhad to give up belief in the literal truth of/ ^- _9 L" ]  }, \/ c6 Y0 T2 F" G
    the Bible or resign themselves to intellectual
    ; W9 U% {( W1 P) G* _1 k6 dirrelevance. This was just one step in a5 l* r2 c# e6 a  D* {1 o  D1 F+ v
    sequence of steps from Galileo through
    ( ]  ?8 _' @% ?8 CNewton and Darwin to the present that,time
    0 Q6 T3 H9 I% B# L$ g1 _/ Nafter time,has weakened the hold of religious8 H2 ^7 N" k, \3 m& I' V  ]: @
    dogmatism. Reading any newspaper nowadays4 L/ m. t0 f2 _" u
    is enough to show you that this work
    8 Z7 _/ I$ y/ F: `) T* Sis not yet complete. But it is civilizing work,
    % Y) g0 M# p+ _9 yof which scientists are able to feel proud.
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    发表于 2009-5-18 19:43:50 | 显示全部楼层
    顶一下哈哈哈哈
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    [LV.1]初来乍到

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    发表于 2009-5-18 20:30:59 | 显示全部楼层
    支持一下!!!!!!!!!!!!
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    [LV.1]初来乍到

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    发表于 2009-5-18 21:35:45 | 显示全部楼层
    英文的啊,有些意思不知道理解的准确不
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    发表于 2009-9-8 15:51:40 | 显示全部楼层
    自己的理解的啊
    1 c$ M$ l% U5 ~" |+ L: c" b% g: N1.没有人可以无所不知,你也不必无所不知;0 \; O5 _! O1 I, C
    2.选择混乱,那是活力所在;
    ) s. E) V, X. E0 g: q: A9 C3.“浪费时间”是必要的;
    2 V: a: U, |) e3 S6 Y1 @8 A+ ?& U4.学点科学史。
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    发表于 2009-9-8 16:38:43 | 显示全部楼层
    乎,英文的啊,哎,估计理解不准了。
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    [LV.6]常住居民II

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    发表于 2009-9-14 23:30:27 | 显示全部楼层
    楼主翻译一下嘛!要不发到英语区也行
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    [LV.2]偶尔看看I

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    发表于 2009-9-15 09:41:00 | 显示全部楼层
    四条定律 ???
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    发表于 2009-9-15 09:53:59 | 显示全部楼层
    you han yu pin yin ban de ma ...
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    发表于 2009-9-15 13:41:10 | 显示全部楼层
    英文的哟~~~~~~~~~~~~~
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