Stars as Laboratories for Fundamental Physics - MPP Theory Group

More documents

Recommendations

Info

xii Table of Contents 13.7 Neutrino Opacity (514) 13.8 Right-Handed Neutrinos (516) 1. Dirac Mass (516) ⋄ 2. Right-Handed Currents (519) ⋄ 3. Magnetic Dipole Moments (521) ⋄ 4. Millicharges (522) ⋄ 5. Charge Radius (523) 14. Axions 14.1 The Strong CP-Problem (524) 14.2 The Peccei-Quinn Mechanism (521) 1. Generic Features (526) ⋄ 2. Axions as Nambu-Goldstone Bosons (528) ⋄ 3. Pseudoscalar vs. Derivative Interaction (531) ⋄ 4. The Onslaught of Quantum Gravity (532) 14.3 Fine Points of Axion Properties (534) 1. The Most Common Axion Models (534) ⋄ 2. Axion Mass and Coupling to Photons (535) ⋄ 3. Model-Dependent Axion-Fermion Coupling (536) 14.4 Astrophysical Axion Bounds (538) 14.5 Cosmological Limits (540) 15. Miscellaneous Exotica 15.1 Constancy of Fermi’s Constant (545) 15.2 Constancy of Newton’s Constant (546) 1. Present-Day Constraints from Celestial Mechanics (546) ⋄ 2. Big-Bang Nucleosynthesis (547) ⋄ 3. Properties of the Sun (549) ⋄ 4. White Dwarfs (551) ⋄ 5. Globular Clusters (551) 15.3 Test of the Equivalence Principle (554) 15.4 Photon Mass and Charge (555) 15.5 Free Quarks (556) 15.6 Supersymmetric Particles (557) 15.7 Majorons (558) 1. Particle-Physics and Cosmological Motivations (558) ⋄ 2. Majorons and Stars (562) 15.8 Millicharged Particles (564) 16. Neutrinos: The Bottom Line 16.1 Standard Neutrinos (568) 16.2 Minimally Extended Standard Model (570) 1. Cosmological Mass Limit for All Flavors (570) ⋄ 2. Oscillations of Solar Neutrinos (571) ⋄ 3. Oscillation of Supernova Neutrinos (572) ⋄ 4. Electromagnetic Properties (573)
Table of Contents xiii 16.3 New Interactions (574) 1. Majorana Masses (574) ⋄ 2. “Heavy” Neutrinos and Fast Decays (574) ⋄ 3. Electromagnetic Properties (576) ⋄ 4. Summary (579) Appendices A. Units and Dimensions (580) B. Neutrino Coupling Constants (583) C. Numerical Neutrino Energy-Loss Rates (585) 1. Plasma Process (585) ⋄ 2. Photoneutrino and Pair-Annihilation Process (586) ⋄ 3. Bremsstrahlung (588) ⋄ 4. Total Emission Rate (589) D. Characteristics of Stellar Plasmas (591) D.1 Normal Matter (591) 1. Temperatures and Densities (591) ⋄ 2. Relativistic Conditions for Electrons (593) ⋄ 3. Electron Degeneracy (593) ⋄ 4. Plasma Frequency (596) ⋄ 5. Screening Scale (596) ⋄ 6. Summary (598) D.2 Nuclear Matter (600) 1. The Ideal p n e ν e Gas (600) ⋄ 2. Kinetic and Chemical Equilibrium (600) ⋄ 3. Cold Nuclear Matter (601) ⋄ 4. Hot Nuclear Matter (602) References (606) Acronyms (642) Symbols (644) Subject Index (649)
Page 1 and 2: Georg G. Raffelt Stars as Laborator
Page 3 and 4: Table of Contents Preface (xiv) Ack
Page 5 and 6: Table of Contents vii 4.5 Neutrino
Page 7 and 8: Table of Contents ix 8. Neutrino Os
Page 9: Table of Contents xi 12. Radiative
Page 13 and 14: Preface xv Second, particles from d
Page 15 and 16: Preface xvii search for proton deca
Page 17 and 18: Preface xix cuts of higher-order gr
Page 19 and 20: Preface xxi quoted “astrophysical
Page 21 and 22: Chapter 1 The Energy-Loss Argument
Page 23 and 24: The Energy-Loss Argument 3 example
Page 25 and 26: The Energy-Loss Argument 5 trinos,
Page 27 and 28: The Energy-Loss Argument 7 As a sim
Page 29 and 30: The Energy-Loss Argument 9 The most
Page 31 and 32: The Energy-Loss Argument 11 against
Page 33 and 34: The Energy-Loss Argument 13 ing M;
Page 35 and 36: The Energy-Loss Argument 15 M ′ (
Page 37 and 38: The Energy-Loss Argument 17 Table 1
Page 39 and 40: The Energy-Loss Argument 19 ing to
Page 41 and 42: The Energy-Loss Argument 21 scalars
Page 43 and 44: Chapter 2 Anomalous Stellar Energy
Page 45 and 46: Anomalous Stellar Energy Losses Bou
Page 61 and 62:
Anomalous Stellar Energy Losses Bou
Page 63 and 64:
Page 65 and 66:
Page 67 and 68:
Page 69 and 70:
Page 71 and 72:
Page 73 and 74:
Page 75 and 76:
Page 77 and 78:
Page 79 and 80:
Page 81 and 82:
Page 83 and 84:
Page 85 and 86:
Page 87 and 88:
Page 89 and 90:
Page 91 and 92:
Page 93 and 94:
Page 95 and 96:
Page 97 and 98:
Page 99 and 100:
Page 101 and 102:
Page 103 and 104:
Page 105 and 106:
Page 107 and 108:
Page 109 and 110:
Chapter 3 Particles Interacting wit
Page 111 and 112:
Particles Interacting with Electron
Page 113 and 114:
Page 115 and 116:
Page 117 and 118:
Page 119 and 120:
Page 121 and 122:
Page 123 and 124:
Page 125 and 126:
Page 127 and 128:
Page 129 and 130:
Page 131 and 132:
Page 133 and 134:
Page 135 and 136:
Page 137 and 138:
Chapter 4 Processes in a Nuclear Me
Page 139 and 140:
Processes in a Nuclear Medium 119 t
Page 141 and 142:
Processes in a Nuclear Medium 121 f
Page 143 and 144:
Processes in a Nuclear Medium 123 F
Page 145 and 146:
Page 147 and 148:
Page 149 and 150:
Processes in a Nuclear Medium 129 v
Page 151 and 152:
Processes in a Nuclear Medium 131 4
Page 153 and 154:
Processes in a Nuclear Medium 133 i
Page 155 and 156:
Processes in a Nuclear Medium 135 H
Page 157 and 158:
Processes in a Nuclear Medium 137 I
Page 159 and 160:
Page 161 and 162:
Page 163 and 164:
Processes in a Nuclear Medium 143 i
Page 165 and 166:
Processes in a Nuclear Medium 145 s
Page 167 and 168:
Processes in a Nuclear Medium 147 E
Page 169 and 170:
Processes in a Nuclear Medium 149 a
Page 171 and 172:
Processes in a Nuclear Medium 151 T
Page 173 and 174:
Processes in a Nuclear Medium 153 r
Page 175 and 176:
Processes in a Nuclear Medium 155 4
Page 177 and 178:
Processes in a Nuclear Medium 157 I
Page 179 and 180:
Processes in a Nuclear Medium 159 t
Page 181 and 182:
Processes in a Nuclear Medium 161 A
Page 183 and 184:
Processes in a Nuclear Medium 163 R
Page 185 and 186:
Chapter 5 Two-Photon Coupling of Lo
Page 187 and 188:
Two-Photon Coupling of Low-Mass Bos
Page 189 and 190:
Page 191 and 192:
Page 193 and 194:
Page 195 and 196:
Page 197 and 198:
Page 199 and 200:
Page 201 and 202:
Page 203 and 204:
Page 205 and 206:
Page 207 and 208:
Page 209 and 210:
Page 211 and 212:
Page 213 and 214:
Chapter 6 Particle Dispersion and D
Page 215 and 216:
Particle Dispersion and Decays in M
Page 217 and 218:
Page 219 and 220:
Page 221 and 222:
Page 223 and 224:
Page 225 and 226:
Page 227 and 228:
Page 229 and 230:
Page 231 and 232:
Page 233 and 234:
Page 235 and 236:
Page 237 and 238:
Page 239 and 240:
Page 241 and 242:
Page 243 and 244:
Page 245 and 246:
Page 247 and 248:
Page 249 and 250:
Page 251 and 252:
Page 253 and 254:
Page 255 and 256:
Page 257 and 258:
Page 259 and 260:
Page 261 and 262:
Page 263 and 264:
Page 265 and 266:
Page 267 and 268:
Page 269 and 270:
Page 271 and 272:
Chapter 7 Nonstandard Neutrinos The
Page 273 and 274:
Nonstandard Neutrinos 253 (“spont
Page 275 and 276:
Nonstandard Neutrinos 255 kinematic
Page 277 and 278:
Nonstandard Neutrinos 257 95% CL ma
Page 279 and 280:
Nonstandard Neutrinos 259 Fig. 7.2.
Page 281 and 282:
Nonstandard Neutrinos 261 In three-
Page 283 and 284:
Nonstandard Neutrinos 263 Flavor mi
Page 285 and 286:
Page 287 and 288:
Nonstandard Neutrinos 267 The quant
Page 289 and 290:
Nonstandard Neutrinos 269 dipole mo
Page 291 and 292:
Nonstandard Neutrinos 271 component
Page 293 and 294:
Page 295 and 296:
Nonstandard Neutrinos 275 moments.
Page 297 and 298:
Nonstandard Neutrinos 277 7.5.2 Spi
Page 299 and 300:
Nonstandard Neutrinos 279 where m
Page 301 and 302:
Neutrino Oscillations 281 and hence
Page 303 and 304:
Neutrino Oscillations 283 As usual
Page 305 and 306:
Neutrino Oscillations 285 two-flavo
Page 307 and 308:
Neutrino Oscillations 287 Fig. 8.2.
Page 309 and 310:
Neutrino Oscillations 289 8.2.4 Exp
Page 311 and 312:
Page 313 and 314:
Neutrino Oscillations 293 Apparentl
Page 315 and 316:
Page 317 and 318:
Neutrino Oscillations 297 when the
Page 319 and 320:
Neutrino Oscillations 299 If the ne
Page 321 and 322:
Neutrino Oscillations 301 8.3.5 The
Page 323 and 324:
Neutrino Oscillations 303 It is als
Page 325 and 326:
Neutrino Oscillations 305 system, h
Page 327 and 328:
Neutrino Oscillations 307 say, betw
Page 329 and 330:
Neutrino Oscillations 309 1991). Th
Page 331 and 332:
Oscillations of Trapped Neutrinos 3
Page 333 and 334:
Page 335 and 336:
Page 337 and 338:
Page 339 and 340:
Page 341 and 342:
Page 343 and 344:
Page 345 and 346:
Page 347 and 348:
Page 349 and 350:
Page 351 and 352:
Page 353 and 354:
Page 355 and 356:
Page 357 and 358:
Page 359 and 360:
Page 361 and 362:
Chapter 10 Solar Neutrinos The curr
Page 363 and 364:
Solar Neutrinos 343 Fig. 10.1. Sola
Page 365 and 366:
Solar Neutrinos 345 There exist vas
Page 367 and 368:
Solar Neutrinos 347 10.2 Calculated
Page 369 and 370:
Solar Neutrinos 349 Fig. 10.3. Norm
Page 371 and 372:
Solar Neutrinos 351 a certain range
Page 373 and 374:
Solar Neutrinos 353 While helium an
Page 375 and 376:
Solar Neutrinos 355 Bahcall and Pin
Page 377 and 378:
Solar Neutrinos 357 Xu et al. (1994
Page 379 and 380:
Solar Neutrinos 359 Table 10.4. Spe
Page 381 and 382:
Solar Neutrinos 361 Table 10.5. Pre
Page 383 and 384:
Solar Neutrinos 363 rates attribute
Page 385 and 386:
Solar Neutrinos 365 10.3.4 Water Ch
Page 387 and 388:
Solar Neutrinos 367 Fig. 10.10. Dif
Page 389 and 390:
Solar Neutrinos 369 Fig. 10.13. Mea
Page 391 and 392:
Solar Neutrinos 371 Table 10.9. Cur
Page 393 and 394:
Solar Neutrinos 373 of order the an
Page 395 and 396:
Solar Neutrinos 375 Fig. 10.16. 37
Page 397 and 398:
Solar Neutrinos 377 GALLEX, or Home
Page 399 and 400:
Solar Neutrinos 379 Table 10.10. Me
Page 401 and 402:
Solar Neutrinos 381 deficits in all
Page 403 and 404:
Solar Neutrinos 383 The ν e surviv
Page 405 and 406:
Solar Neutrinos 385 The allowed ran
Page 407 and 408:
Solar Neutrinos 387 10.7 Spin and S
Page 409 and 410:
Solar Neutrinos 389 10.8 Neutrino D
Page 411 and 412:
Solar Neutrinos 391 The small- and
Page 413 and 414:
Solar Neutrinos 393 flux above its
Page 415 and 416:
Chapter 11 Supernova Neutrinos The
Page 417 and 418:
Supernova Neutrinos 397 Fig. 11.1.
Page 419 and 420:
Supernova Neutrinos 399 beyond the
Page 421 and 422:
Supernova Neutrinos 401 ate neutrin
Page 423 and 424:
Supernova Neutrinos 403 Convection
Page 425 and 426:
Supernova Neutrinos 405 Hayes, and
Page 427 and 428:
Supernova Neutrinos 407 11.2 Predic
Page 429 and 430:
Supernova Neutrinos 409 must then b
Page 431 and 432:
Supernova Neutrinos 411 Figure 11.6
Page 433 and 434:
Supernova Neutrinos 413 signal (Sec
Page 435 and 436:
Supernova Neutrinos 415 time) on 23
Page 437 and 438:
Supernova Neutrinos 417 All of the
Page 439 and 440:
Supernova Neutrinos 419 to multiple
Page 441 and 442:
Supernova Neutrinos 421 the final-s
Page 443 and 444:
Supernova Neutrinos 423 ter of 53 e
Page 445 and 446:
Supernova Neutrinos 425 Given these
Page 447 and 448:
Supernova Neutrinos 427 thorough st
Page 449 and 450:
Supernova Neutrinos 429 The forward
Page 451 and 452:
Supernova Neutrinos 431 Another int
Page 453 and 454:
Supernova Neutrinos 433 ber of ν e
Page 455 and 456:
Supernova Neutrinos 435 A “normal
Page 457 and 458:
Supernova Neutrinos 437 Fig. 11.19.
Page 459 and 460:
Supernova Neutrinos 439 The approxi
Page 461 and 462:
Supernova Neutrinos 441 be taken to
Page 463 and 464:
Supernova Neutrinos 443 sense that
Page 465 and 466:
Supernova Neutrinos 445 presence of
Page 467 and 468:
Supernova Neutrinos 447 An even mor
Page 469 and 470:
Chapter 12 Radiative Particle Decay
Page 471 and 472:
Radiative Particle Decays 451 one c
Page 473 and 474:
Radiative Particle Decays 453 corre
Page 475 and 476:
Radiative Particle Decays 455 is no
Page 477 and 478:
Radiative Particle Decays 457 Fig.
Page 479 and 480:
Page 481 and 482:
Radiative Particle Decays 461 12.3.
Page 483 and 484:
Radiative Particle Decays 463 emiss
Page 485 and 486:
Radiative Particle Decays 465 range
Page 487 and 488:
Page 489 and 490:
Radiative Particle Decays 469 weak
Page 491 and 492:
Radiative Particle Decays 471 value
Page 493 and 494:
Radiative Particle Decays 473 ignor
Page 495 and 496:
Page 497 and 498:
Page 499 and 500:
Radiative Particle Decays 479 Table
Page 501 and 502:
Radiative Particle Decays 481 In or
Page 503 and 504:
Page 505 and 506:
Radiative Particle Decays 485 while
Page 507 and 508:
Radiative Particle Decays 487 h 100
Page 509 and 510:
Page 511 and 512:
Radiative Particle Decays 491 still
Page 513 and 514:
Chapter 13 What Have We Learned fro
Page 515 and 516:
What Have We Learned from SN 1987A
Page 517 and 518:
Page 519 and 520:
Page 521 and 522:
Page 523 and 524:
Page 525 and 526:
Page 527 and 528:
Page 529 and 530:
Page 531 and 532:
Page 533 and 534:
Page 535 and 536:
Page 537 and 538:
Page 539 and 540:
Page 541 and 542:
Page 543 and 544:
Page 545 and 546:
Axions 525 Table 14.1. Particle mag
Page 547 and 548:
Axions 527 or axion decay constant.
Page 549 and 550:
Axions 529 The Yukawa coupling h is
Page 551 and 552:
Axions 531 14.2.3 Pseudoscalar vs.
Page 553 and 554:
Axions 533 Notably, the Higgs field
Page 555 and 556:
Axions 535 otic heavy quarks: only
Page 557 and 558:
Axions 537 Various axion models dif
Page 559 and 560:
Axions 539 Bounds on the Yukawa cou
Page 561 and 562:
Axions 541 Fig. 14.5. Astrophysical
Page 563 and 564:
Axions 543 decay into axions. This
Page 565 and 566:
Chapter 15 Miscellaneous Exotica St
Page 567 and 568:
Miscellaneous Exotica 547 Table 15.
Page 569 and 570:
Miscellaneous Exotica 549 15.2.3 Pr
Page 571 and 572:
Miscellaneous Exotica 551 Most rece
Page 573 and 574:
Miscellaneous Exotica 553 Fig. 15.1
Page 575 and 576:
Miscellaneous Exotica 555 A violati
Page 577 and 578:
Miscellaneous Exotica 557 nuclei it
Page 579 and 580:
Miscellaneous Exotica 559 mass, and
Page 581 and 582:
Miscellaneous Exotica 561 backgroun
Page 583 and 584:
Miscellaneous Exotica 563 SN 1987A
Page 585 and 586:
Miscellaneous Exotica 565 which led
Page 587 and 588:
Miscellaneous Exotica 567 For a nar
Page 589 and 590:
Neutrinos: The Bottom Line 569 the
Page 591 and 592:
Neutrinos: The Bottom Line 571 Neut
Page 593 and 594:
Neutrinos: The Bottom Line 573 Apar
Page 595 and 596:
Neutrinos: The Bottom Line 575 is d
Page 597 and 598:
Neutrinos: The Bottom Line 577 of t
Page 599 and 600:
Neutrinos: The Bottom Line 579 siti
Page 601 and 602:
Units and Dimensions 581 In the ast
Page 603 and 604:
Appendix B Neutrino Coupling Consta
Page 605 and 606:
Appendix C Numerical Neutrino Energ
Page 607 and 608:
Numerical Neutrino Energy-Loss Rate
Page 609 and 610:
Numerical Neutrino Energy-Loss Rate
Page 611 and 612:
Appendix D Characteristics of Stell
Page 613 and 614:
Characteristics of Stellar Plasmas
Page 615 and 616:
Page 617 and 618:
Page 619 and 620:
Page 621 and 622:
Page 623 and 624:
Page 625 and 626:
Page 627 and 628:
References 607 Akhmedov, E. Kh., an
Page 629 and 630:
References 609 Bahcall, J. N., Kras
Page 631 and 632:
References 611 Bilenky, S. M., and
Page 633 and 634:
References 613 Cannon, R. D. 1970,
Page 635 and 636:
References 615 Cooper-Sarkar, A. M.
Page 637 and 638:
References 617 Dodelson, S., Friema
Page 639 and 640:
References 619 Fukuda, Y., et al. 1
Page 641 and 642:
References 621 Goyal, A., Dutta, S.
Page 643 and 644:
References 623 Hoogeveen, F., and S
Page 645 and 646:
References 625 Kawakami, H., et al.
Page 647 and 648:
References 627 Landau, L. D., and P
Page 649 and 650:
References 629 Mayle, R. W., and Wi
Page 651 and 652:
References 631 Nieves, J. F., and P
Page 653 and 654:
References 633 Pochoda, P., and Sch
Page 655 and 656:
References 635 Ross, J. E., and All
Page 657 and 658:
References 637 Shlyakhter, A. I. 19
Page 659 and 660:
References 639 Totsuka, Y. 1993, Ne
Page 661 and 662:
References 641 Wiezorek, C., et al.
Page 663 and 664:
Acronyms 643 L l.h. l.h.s. ly LMC L
Page 665 and 666:
Symbols 645 dp differential in phas
Page 667 and 668:
Symbols 647 X j Peccei-Quinn charge
Page 669 and 670:
Subject Index A α-Ori 189 A665, A1
Page 671 and 672:
Subject Index 651 Coulomb gauge 204
Page 673 and 674:
Subject Index 653 H Hayashi line 32
Page 675 and 676:
Subject Index 655 multiple scatteri
Page 677 and 678:
Subject Index 657 neutrino radiativ
Page 679 and 680:
Subject Index 659 Primakoff process
Page 681 and 682:
Subject Index 661 SN 1987A bounds (
Page 683 and 684:
Subject Index 663 supernova core bi
show all

Stars as Laboratories for Fundamental Physics - MPP Theory Group

Create successful ePaper yourself

Delete template?

Save as template?