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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. c( L0 x; q& F7 R& T4 d" e* J
    ( G( e" t2 X8 [/ M. Y
    Steven Weinberg is in the Department of Physics,
    3 m+ {# w2 b  F0 Y2 ithe University of Texas at Austin, Texas 78712,
    - D& q! Q* |4 `  w) m4 w/ @0 o3 p, KUSA. This essay is based on a commencement talk
    + X6 J2 z5 ~7 F; C! I- \given by the author at the Science Convocation at* t; M/ J' P0 p) v
    McGill University in June 2003.
    ; m; t# C2 O* L) E- O. x
      W! m, P2 S* ?* dWhen I received my undergraduate degree — about a hundred years
    4 U8 ~& k2 M+ V- ~ago — the physics literature seemed to me a vast, unexplored ocean,
    $ A7 \7 P( }5 _( U8 n: u- B7 E  Zevery part of which I had to chart before beginning any research of my own. How+ K4 G! W" D, U- E
    could I do anything without knowing everything that had already been done?* w& \7 M7 @4 w! }, A4 e% w
    Fortunately, in my first year of graduate school, I had the good luck to fall into the7 J% N0 |- w" M" O& g
    hands of senior physicists who insisted, over my anxious objections, that I must start
    5 C+ V, N6 o% l: g5 c& {& wdoing research, and pick up what I needed to know as I went along. It was sink or& z0 Z; o, `2 S# c" u
    swim. To my surprise, I found that thisworks. I managed to get a quick PhD —
    5 R6 H2 ^( h# n/ nthough when I got it I knew almost nothing about physics. But I did learn one big
    . T* q; u5 ?" w- M1 g% mthing: that no one knows everything, and you don’t have to .  o' [" `# n; _& S$ E' h
    5 d, j: [! k- I8 b
    Another lesson to be learned, to continue
    ' {4 T* U1 @' ?4 dusing my oceanographic metaphor, is that
    ; O& ~3 @6 A6 [while you are swimming and not sinking you7 R' ?( L' [# i7 O6 ]. s
    should aim for rough water. When I was
    $ }- V* w; P$ k( H  Y  ~teaching at the Massachusetts Institute of
    : v; D- e. e- U! Z* `" uTechnology in the late 1960s, a student told# w7 l! I  }( D; N3 w& i1 Y  \
    me that he wanted to go into general
    9 R5 S0 E- s5 b3 r" C& Brelativity rather than the area I was working% N( w. I1 d# h* ~/ y* e
    on, elementary particle physics, because/ B$ O5 }! z% l- R
    the principles of the former were well
    8 D+ ]) `; r) G. N& l7 o  Qknown, while the latter seemed like a mess( h1 l6 t, W7 X
    to him. It struck me that he had just given! V' y% D% s# w: P! p# [
    a perfectly good reason for doing the opposite.9 ^/ `) E1 S5 W8 w/ @  T& G. q
    Particle physics was an area where% v7 a3 K  h: V, D1 V
    creative work could still be done. It really was
    ) `, B7 X0 I6 Z* g) l- g4 `a mess in the 1960s, but since that time the
    9 e' B5 f. B$ L- W* V4 y  e( `work of many theoretical and experimental5 R6 c/ b; P+ Z$ n/ H$ Y) v  {! }
    physicists has been able to sort it out, and
    " r* I$ |2 f5 a4 h$ ?* yput everything (well, almost everything)/ \  T) I* s  A* q- I+ S
    together in a beautiful theory known as
    & r0 a5 R: f0 L$ \the standard model.My advice is to go for the
    . V* y7 @+ l5 ~2 lmesses — that’s where the action is.
    & z) M7 v% Z6 _/ L3 f% q
    6 Y4 ^$ {7 a) U0 s9 }+ DMy third piece of advice is probably the. \& s2 k5 ?; I) D) E% l
    hardest to take. It is to forgive yourself for% x% v% S$ r" l6 E9 f5 D! N
    wasting time. Students are only asked to3 c* Z% N6 p: Y+ z& z6 S; X
    solve problems that their professors (unless) K+ e5 @8 C( P9 P
    unusually cruel) know to be solvable. In2 H; L" E$ B% Y5 z6 u
    addition,it doesn’t matter if the problems are
    # X* s5 J2 l) K' E9 @2 Zscientifically important — they have to be
    % n2 ]# N: f  g1 ~solved to pass the course. But in the real
    ) f* o& ~  I! Hworld, it’s very hard to know which problems
    & y# e1 t. v. ~) _6 [2 K# Dare important, and you never know whether
    ' M+ L' {3 c: ^+ V/ ~6 sat a given moment in history a problem is
    0 w- q0 E% Z4 O8 V9 h% O! ?7 R+ A8 Z4 |solvable. At the beginning of the twentieth8 q/ i' N& C/ ?" Z* ^* s5 X5 g
    century, several leading physicists, including* d& o5 p% h$ L5 m: [
    Lorentz and Abraham, were trying to work; c3 b9 B$ F- A4 l) b
    out a theory of the electron. This was partly1 d7 c0 z7 }; e
    in order to understand why all attempts to$ ]8 x0 U8 ]; L, b! G9 n" V
    detect effects of Earth’s motion through the
      `4 Z6 O* t4 U) y7 r" ^ether had failed. We now know that8 f$ ^, z4 N' z* `
    they were working on the wrong problem.: u8 Q: L. \* @1 G! I+ Q& B0 r
    At that time, no one could have developed a
    # ~+ P7 E3 @8 ?$ W  {4 ]successful theory of the electron, because) Y# b& O# W8 U( ]0 j
    quantum mechanics had not yet been# k6 H& T: `+ ^
    discovered. It took the genius of Albert
    3 `, U) y7 _5 n  n6 ZEinstein in 1905 to realize that the right
    , b* c' x3 Z& Z) i. [problem on which to work was the effect
    1 \- t$ Y% f( U7 V! x5 V( Vof motion on measurements of space and) Y7 U% {: J5 I$ r% `
    time. This led him to the special theory of  `( |( C9 u9 X. N9 O
    relativity. As you will never be sure which0 u  v: b# P( k7 J
    are the right problems to work on, most
    2 M7 H& m% o" J5 O4 o  \of the time that you spend in the laboratory; c: q& y- }, n3 M4 p( X
    or at your desk will be wasted. If you want5 R$ x5 W3 q3 y- B. {9 R' V
    to be creative, then you will have to get used
    ) a' ^: A& l' h* @& M3 w# cto spending most of your time not being- ?) w  ?: ~/ c3 W. X
    creative, to being becalmed on the ocean of
    8 f" h. ~' P2 u( d, \- Cscientific knowledge.
    - |( A; M0 Q* b) \
    3 B; M( f- d8 u) v: E" e! FFinally, learn something about the history
    / @' J1 b' p' v6 u8 Cof science,or at a minimum the history of your9 w# _; \1 t) h: n# R# H7 w8 ^
    own branch of science. The least important* S2 ?* E) v. O( h
    reason for this is that the history may actually# V% x6 m. k7 W
    be of some use to you in your own scientific
    $ T& d  l$ b) o; \work. For instance, now and then scientists: f: e* p. F  A3 z0 [6 t- s( h
    are hampered by believing one of the oversimplified! B9 l# r+ }& T/ }! w. j% S' f: w. @
    models of science that have0 V2 G0 c1 {; H* A5 O
    been proposed by philosophers from Francis
    7 q) O' W( ]# C( O  v4 kBacon to Thomas Kuhn and Karl Popper.9 e6 f0 ]  R0 k( A! _) h/ z' I
    The best antidote to the philosophy of science9 w( ?" S+ d2 M3 E2 b0 M
    is a knowledge of the history of science.! t5 z: e5 k+ Y
    More importantly, the history of science
    2 {# t4 T3 y% b# U, i3 Gcan make your work seem more worthwhile! R  w+ y" ^; A3 X% l
    to you. As a scientist, you’re probably not
    9 ?8 X2 q& I1 i) {% @3 m1 L, U! f3 xgoing to get rich. Your friends and relatives5 P" @9 C6 M3 n; ^, Z9 t1 K
    probably won’t understand what you’re2 a' z  y0 S: p0 ]3 r
    doing.And if you work in a field like elementary  ~+ h. Q4 e( S  h' k  b* I
    particle physics, you won’t even have the* ~" ]9 X( e7 P+ b8 T/ F; ?: q
    satisfaction of doing something that is
    9 j* D  v6 I8 Y4 {/ G+ G& Uimmediately useful. But you can get great
    5 }- p# G9 u: d: `, Y+ c7 |7 ~  f% Ksatisfaction by recognizing that your work in
    2 o  M8 r) Y! O; }science is a part of history.
    . b) E* L: i4 n* C' Y  ?- a/ A! x) t+ H5 ?
    Look back 100 years, to 1903. How0 b; }4 e% H+ ]3 l! T1 J, b
    important is it now who was Prime Minister1 `  o& L3 w! ^! o8 P+ p5 [6 f
    of Great Britain in 1903, or President of the
    2 u( f0 L3 L0 c+ V; xUnited States? What stands out as really
    2 Z+ h: e7 S9 A7 m1 r/ K0 _7 Simportant is that at McGill University,
    - P% K5 J! |. k  e& s, YErnest Rutherford and Frederick Soddy were! Q# ]& @' X* q  ^8 r1 n% w
    working out the nature of radioactivity.
    7 |1 m+ h, H6 N0 QThis work (of course!) had practical applications,2 ]( r4 L' ~" ^
    but much more important were its8 S2 o- a6 x8 [; ]7 r, K
    cultural implications. The understanding of
    : Y) {5 Z6 \+ D: @% g- l# X4 Eradioactivity allowed physicists to explain
    " p* f. m& r" s5 U/ y) nhow the Sun and Earth’s cores could still be
    * Z- U# E$ s' ]8 fhot after millions of years. In this way, it" B- Z' S: |" `
    removed the last scientific objection to what
    5 g9 A& ?; x, e1 m  J/ P# i" {many geologists and paleontologists
    1 l3 _; L# b2 ?- r3 Vthought was the great age of the Earth and
    . i( Q7 B  U- T( u- Ithe Sun.After this,Christians and Jews either
    5 J2 H! r- m8 ?( t7 Dhad to give up belief in the literal truth of
    # _- A7 L/ d3 Q5 Hthe Bible or resign themselves to intellectual$ }, q5 H8 V3 w! r1 Y1 w
    irrelevance. This was just one step in a& w1 p& p9 l! d; G% J/ P
    sequence of steps from Galileo through# r/ a: I% |, [2 {
    Newton and Darwin to the present that,time0 J4 D8 _  T6 V/ H
    after time,has weakened the hold of religious) K  A, |6 v" H
    dogmatism. Reading any newspaper nowadays
    7 ~. t+ N: Q" z9 R" Bis enough to show you that this work, m! P1 h- N$ [* m: p, n, o
    is not yet complete. But it is civilizing work,
    . X/ |. o" q1 r/ ^; [of 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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    2018-2-2 08:17
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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
    . ^/ ^0 k# W! _1.没有人可以无所不知,你也不必无所不知;
    2 A& B3 _4 S; e9 D; {# E2.选择混乱,那是活力所在;
    , E+ p9 r0 N& _1 @1 U3.“浪费时间”是必要的;$ s! l: H$ y: ?' K
    4.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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