In General > s.a. experiments; history; teaching; theory.
* In terms of paradigms:
Classical mechanics, quantum mechanics, (quantum) field theory.
* Parts: Experimental
domain (object), mathematical model, conventional interpretation.
* Objects/systems: Elementary
particles, fields and interactions, nuclear physics, atomic physics, solid
state, astronomy and astrophysics.
* Formalisms: Few-particle
and many-body dynamics, continuous media and fields, statistical mechanics.
* Methods: Hamiltonian and Lagrangian formulations.
Specific Topics > s.a. QCD
phenomenology.
@ I: Rothman 91; Dyson 93; Silverman 93; Ehrlich 94; Morrison 94; Barrow
99; Azaroff 00; Siegfrid 00; Jargodzki & Potter
01 [puzzles]; Aslamazov & Varlamov 04 [condensed matter emphasis].
@ III: Peierls 79; Van der Merwe ed-83; Lahti & Mittelstaedt ed-85;
Kheyfets & Miller JMP(91);
Zhang ht/02-in
[solid state and fundamental physics].
@ Reference book: Anderson ed-89; Cohen ed-95.
Main Open Problems, Present State
* According to Ginzburg PT(90)may:
- Macrophysics: (1)
Controlled nuclear synthesis; (2) High-temperature (room Tc?)
superconductivity; Superdiamagnetism; (3) New substances (metallic H and others);
(4) Solid state physics (metal/dielectric transition, charge/spin-density waves,
disordered semiconductors, spin glasses, quantum Hall effect, mesoscopics);
(5) Second-order phase transitions and critical phenomena; (6) Surface physics;
(7) Liquid crystals; very large molecules; (8) Behavior of matter in very strong
magnetic fields; (9) Rasers, grasers, ultrahigh power lasers; (10) Strongly
non-linear phenomena (non-linear physics); (11) Supertransuranic elements,
exotic nuclei.
- Microphysics: (12)
Particle mass spectrum; Quarks and gluons (QCD, number of parameters, generations);
(13) Unified electroweak theory (W +/–,
Z0, leptons); (14) Grand unification
(proton decay, n mass, magnetic monopoles,
supersymmetry, strings); (15) Quantum gravity and fundamental length, high
and superhigh-energy interactions; (16) CP invariance and non-conservation;
phase
transitions
in
vacuum.
- Astrophysics: (17)
Experimental verification of general relativity; (18) Detection of gravitational
waves; (19) Connection between cosmology and hep, the cosmological constant
problem;
(20)
Neutron stars and pulsars; (21) Black holes; (22) Quasars and galactic nuclei,
formation of galaxies,
dark matter; (23) Origin of cosmic rays; cosmic X-rays and
-rays
(including superhigh energy); (24) Neutrino astronomy (solar neutrino problem
etc).
* Extra problems: Large
dimensionless numbers; The Pioneer anomalous acceleration.
* 2006 hot topics: In
decreasing order, carbon nanotubes, nanowires, quantum dots, fullerenes, giant
magnetoresistance, M-theory,
quantum computation.
@ General references: Ginzburg 85, PT(90)may;
Leggett 88; Kundt ap/98-in
[disagreements]; survey pw(99)dec;
Mermin PT(01)feb;
Lämmerzahl et al gq/06-in
[solar system anomalies].
@ Status, trends: Ellis MPLA(93);
roundtable
PT(94)mar;
Langenberg PT(94)dec
[future];
Fitch et al ed-97; issue RMP(99)71#2;
Freund ht/04-in
[spacetime + matter]; Banks phy/06 + pw(06)may
[hot
topic index]; Winterberg a0805 ["clouds
of physics"]; > s.a. cosmology, particle
physics.
Applications
* Examples: Quantum mechanics
– theory of light – lasers – CD's; General relativity – gravitational
redshift – GPS [@ Berry pw(04)dec].
@ Fundamental vs applied: Rech(92)dec,
p1410.
@ Examples: news PT(04)jul
[particle physics and restoring old recordings].
@ Econophysics: Amaral et al PRL(98), Lee et al PRL(98)-pn(98)oct;
Piotrowski & Sladkowski APPB(01)qp [and
quantum mechanics]; Daniel & Sornette a0802 [rev, historical].
@ Research Fields in Physics 9th ed, AIP 94 [r CP(95)#4].
Main page – Abbreviations – Journals – Comments – Other
sites – Acknowledgements
Send feedback and suggestions to bombelli at olemiss.edu – Modified
27 jun 2008