Why the universe is just so

被引:143
作者
Hogan, CJ [1 ]
机构
[1] Univ Washington, Dept Astron, Seattle, WA 98195 USA
[2] Univ Washington, Dept Phys, Seattle, WA 98195 USA
关键词
D O I
10.1103/RevModPhys.72.1149
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Some properties of the world are fixed by physics derived from mathematical symmetries, while others are selected from an ensemble of possibilities. Several successes and failures of "anthropic" reasoning in this context are reviewed in light of recent developments in astrobiology, cosmology, and unification physics. Specific issues raised include our space-time location (including the reason for the present age of the universe), the time scale of biological evolution, the tuning of global cosmological parameters, and the origin of the Large Numbers of astrophysics and the parameters of the standard model. Out of the 20 parameters of the standard model, the basic behavior and structures of the world (nucleons, nuclei, atoms, molecules, planets, stars, galaxies) depend mainly on five of them: m(e), m(u), m(d), alpha, and alpha (G) (where m(proton) and alpha (QCD) are taken as defined quantities). Three of these appear to be independent in the context of Grand Unified Theories (that is, not fixed by any known symmetry) and at the same time have values within a very narrow window which provides for stable nucleons and nuclei and abundant carbon. The conjecture is made that the two light quark masses and one coupling constant are ultimately determined even in the "final theory" by a choice from a large or continuous ensemble, and the prediction is offered that the correct unification scheme will not allow calculation of (m(d)-m(u))/m(proton) from first principles alone.
引用
收藏
页码:1149 / 1161
页数:13
相关论文
共 75 条
[1]   Global distribution of crustal magnetization discovered by the Mars Global Surveyor MAG/ER experiment [J].
Acuña, MH ;
Connerney, JEP ;
Ness, NF ;
Lin, RP ;
Mitchell, D ;
Carlson, CW ;
McFadden, J ;
Anderson, KA ;
Rème, H ;
Mazelle, C ;
Vignes, D ;
Wasilewski, P ;
Cloutier, P .
SCIENCE, 1999, 284 (5415) :790-793
[2]   Viable range of the mass scale of the standard model [J].
Agrawal, V ;
Barr, SM ;
Donoghue, JF ;
Seckel, D .
PHYSICAL REVIEW D, 1998, 57 (09) :5480-5492
[3]   Anthropic considerations in multiple-domain theories and the scale of electroweak symmetry breaking [J].
Agrawal, V ;
Barr, SM ;
Donoghue, JF ;
Seckel, D .
PHYSICAL REVIEW LETTERS, 1998, 80 (09) :1822-1825
[4]   The hierarchy problem and new dimensions at a millimeter [J].
Arkani-Hamed, N ;
Dimopoulos, S ;
Dvali, G .
PHYSICS LETTERS B, 1998, 429 (3-4) :263-272
[5]  
Barrow J.D., 1986, ANTHROPIC COSMOLOGIC
[6]  
BEREZHIANI Z, 1996, HEPPH9602325
[7]   The eighteen arbitrary parameters of the standard model in your everyday life [J].
Cahn, RN .
REVIEWS OF MODERN PHYSICS, 1996, 68 (03) :951-959
[8]  
CARR JB, 1979, NATURE, V278, P611
[9]   THE ANTHROPIC PRINCIPLE AND ITS IMPLICATIONS FOR BIOLOGICAL EVOLUTION [J].
CARTER, B .
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 1983, 310 (1512) :347-363
[10]  
CARTER B, 1974, IAU S, V63