[1]
|
K. Freeman and G. McNamara, “In Search of Dark Matter,” Springer, Berlin, 2006.
|
[2]
|
F. Zwicky, “The Redshift of Extragalactic Nebulae,” Helvetica Physica Acta, Vol. 6, 1933, pp. 110-127.
|
[3]
|
J. P. Ostriker, et al., “The Size and Mass of Galaxies, and the Mass of the Universe,” Astrophysical Journal, Vol. 193, 1974, pp. L1-L4. doi:10.1086/181617
|
[4]
|
S. M. Faber and J. S. Gallagher, “Masses and Mass-to-Light Ratios of Galaxies,” Annual Review of Astronomy and Astrophysics, Vol. 17, No. 1, 1979, pp. 135-187.
|
[5]
|
M. Davis, et al., “On the Virgo Supercluster and the Mean Mass density of the Universe,” Astrophysical Journal, Vol. 238, 1980, pp. L113-L116. doi:10.1086/183269
|
[6]
|
V. Trimble, “Existence and Nature of Dark Matter in the Universe,” Annual Review of Astronomy and Astrophysics, Vol. 25, No. 1, 1987, pp. 425-472.
|
[7]
|
N. A. Bahcall et al., “Where is Dark Matter?” Astrophysical Journal, Vol. 447, 1995, pp. L81-L85.
|
[8]
|
C. Alcock, et al., “The MACHO Project: Microlensing Results from 5.7 Years of LMC Observations,” Astrophysical Journal, Vol. 542, No. 1, 2000, pp. 281-307.
doi:10.1086/309512
|
[9]
|
P. Tisserand, et al., “Limits on the MACHO Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds,” Astronomy & Astrophysics, Vol. 469, No. 2, 2007, pp. 387-404.
|
[10]
|
S. Sarkar, “Supersymmetric Inflation and Large-Scale Structure,” 1996.
|
[11]
|
D. N. Schramm and M. S. Turner, “Big-Bang Nucleosynthesis Enters the Precision Era,” Reviews of Modern Physics, Vol. 70, No. 1, 1998, pp. 303-318.
|
[12]
|
K. Jedamzik and M. Pospelov, “Big Bang Nucleosynthesis and Particle Dark Matter,” New Journal of Physics, Vol. 11, 2009, Article ID: 105028.
|
[13]
|
D. Clowe, et al., “A Direct Empirical Proof of the Existence of Dark Matter,” Astrophysical Journal, Vol. 648, No. 2, 2006, pp. L109-L113.doi:10.1086/508162
|
[14]
|
B. Nodland and J. P. Ralston, “Indication of Anistropy in Electromagnetic Propagation over Cosmological Distances,” Physical Review Letters, Vol. 78, No. 16, 1997, pp. 3043-3046.
|
[15]
|
L. S. Schulman, “Opposite Thermodynamic Arrows of Time,” Physical Review Letters, Vol. 83, No. 26, 1999, pp. 5419-5422.
|
[16]
|
F. Zwicky, “On the Masses of Nebulae and of Clusters of Nebulae,” Astrophysical Journal, Vol. 86, 1937, pp. 217- 246. doi:10.1086/143864
|
[17]
|
V. Rubin, N. Thonnard and W. K. Ford Jr., “Rotation Properties of 21 Sc Galaxies with a Large Range of Luminosities and Radii from NGC 4605 (R = 4 kpc) to UGC 2885 (R = 122 kpc),” Astrophysical Journal, Vol. 238, 1980, pp. 471-487. doi:10.1086/158003
|
[18]
|
S. M. Faber and R. E. Jackson, “Velocity Dispersions and Mass-to-Light Ratios for Elliptical Galaxies,” Astrophysical Journal, Vol. 204, 1976, pp. 668-683.
doi:10.1086/154215
|
[19]
|
X.-P. Wu, T. Chiueh, L.-Z. Fang, and Y.-J. Xue, “A Comparison of Different Cluster Mass Estimates: Consistency or Discrepancy?” Monthly Notices of the Royal Astronomical Society, Vol. 301, No. 3, 1998, pp. 861-871.doi:10.1046/j.1365-8711.1998.02055.x
|
[20]
|
N. W. Boggess, et al., “The COBE Mission: Its Design and Performance Two Years after the Launch,” Astrophysical Journal, Vol. 397, No. 2, 1992, pp. 420-429.
doi:10.1086/171797
|
[21]
|
A. Melchiorri, et al., “A Measurement of W from the North American Test Flight of Boomerang,” The Astrophysical Journal Letters, Vol. 536, No. 2, 2000, pp. L63-L66. doi:10.1086/312744
|
[22]
|
E. M. Leitch, et al., “Degree Angular Scale Interferometer 3 Year Cosmic Microwave Background Polarization Results,” Astrophysical Journal, Vol. 624, No. 2, 2005, pp. 10-20. doi:10.1086/428825
|
[23]
|
A. C. S. Readhead, et al., “Polarization Observations with the Cosmic Background Imager,” Science, Vol. 306 No. 5697, 2004, pp. 836-844.
|
[24]
|
G. Hinshaw, et al., “Five-Year Wilkinson Microwave Anisotropy Probe Observations: Data Processing, Sky Maps, and Basic Results,” Astrophysical Journal Supplement Series, Vol. 180, No. 2, 2009, pp. 225-245.
doi:10.1088/0067-0049/180/2/225
|
[25]
|
E. Komatsu, et al., “Five-Year Wilkinson Microwave Anisotropy Probe Observations: Cosmological Interpretation,” Astrophysical Journal Supplement Series, Vol. 180, No. 2, 2009, pp. 330-376.
doi:10.1088/0067-0049/180/2/330
|
[26]
|
V. Springle, et al., “Simulations of the Formation, Evolution and Clustering of Galaxies and Quasars,” Nature, Vol. 435, 2005, pp. 629-636.
|
[27]
|
J. R. Primack and D. Seckel, “Detection of Cosmic Dark Matter,” Annual Review of Astronomy and Astrophysics, Vol. 38, 1988, pp. 751-807.
|
[28]
|
R. D. Peccei and H. R. Quinn, “CP Conservation in the Presence of Pseudoparticles,” Physical Review Letters, Vol. 38, No. 25, 1977, pp. 1440-1443.
|
[29]
|
J. L. Feng, “Dark Matter Candidates from Particle Physics and Methods of Detection,” Annual Review of Astronomy and Astrophysics, Vol. 48, 2010, pp. 495-545.
|
[30]
|
G. G. Raffelt, “Astrophysical Axion Bounds,” Lecture Notes in Physics, Vol. 741, 2008, pp. 51-71.
|
[31]
|
P. Sikivie and Q.Yang, “Bose-Einstein Condensation of Dark Matter Axions,” Physical Review Letters, Vol. 103, No. 11, 2009, Article ID: 111301.
|
[32]
|
C. Robilliard, et al., “No Light Shining through a Wall: Results from a Photore Generation Experiment,” Physical Review Letters, Vol. 99, No. 19, 2007, p. 190403.
|
[33]
|
K. J. Mack and P. J. Steinhardt, “Cosmological Problems with Multiple Axion-Like Fields,” The Journal of Cosmology and Astroparticle Physics, Vol. 5, 2011, p. 1.
|
[34]
|
A. Renzini, “Effects of Cosmions in the Sun and in Globular Cluster Stars,” Astronomy & Astrophysics, Vol. 171, No. 1-2, 1987, pp. 121-122.
|
[35]
|
Y. Fukuda, et al., “Evidence for Oscillation of Atmospheric Neutrinos,” Physical Review Letters, Vol. 81, No. 8, 1998, pp. 1562-1567.
|
[36]
|
Q. R. Ahmad, et al., “Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory,” Physical Review Letters, Vol. 89, 2002, Article ID: 011301.
|
[37]
|
P. C. McGuire and P. Steinhardt, “Cracking Open the Window for Strongly Interacting Massive Particles as the Halo Dark Matter,” 2001, arXiV:astro-ph/0105567v1.
|
[38]
|
H. Pagels and J. P. Primack, “Supersymmetry, Cosmology, and New Physics at TeraElectronvolt Energies,” Physical Review Letters, Vol. 48, No. 4, 1982, pp. 223- 226.
|
[39]
|
G. Blumenthal, et al., “Galaxy Formation by Dissipationless Particles Heavier than the Neutrino,” Nature, Vol. 299, 1982, pp. 37-38.
|
[40]
|
T. Moroi, et al., “Cosmological Constraints on the Light Stable Gravitino,” Physics Letters B, Vol. 303, 1993, pp. 289-294.
|
[41]
|
N. Okada and O. Seto, “A Brane World Cosmological Solution to the Gravitino Problem,” Physical Review D, Vol. 71, 2005, Article ID: 023517.
|
[42]
|
A. de Gouvea, et al., “Cosmology of Supersymmetric Models with Low-Energy Gauge Mediation,” Physical Review D, Vol. 56, 1997, pp. 1281-1299.
|
[43]
|
F. Takayama and M. Yamaguchi, “Gravitino Dark Matter without R-Parity,” Physics Letters B, Vol. 485, No. 4, 2000, pp. 388-392. doi:10.1016/S0370-2693(00)00726-7
|
[44]
|
T. Falk, et al., “Heavy Sneutrinos as Dark Matter,” Physics Letters B, Vol. 339, No. 3, 1994, pp. 248-251.
doi:10.1016/0370-2693
|
[45]
|
C. Arina and N. Fornengo, “Sneutrino Cold Dark Matter, a New Analysis: Relic Abundance and Detection Rates,” Journal of High Energy Physics, Vol. 11, 2007, p. 29.
|
[46]
|
D. G. Cerde?o, et al., “Very Light Right-Handed Sneutrino Dark Matter in the NMSSM,” Journal of Astronomy and Astroparticle Physics, Vol. 11, 2011, p. 27.
|
[47]
|
B. Dumont, et al., “Mixed Sneutrino Dark Matter in Light of the 2011 XENON and LHC Results,” 2012.
arXiv:1206.1521.
|
[48]
|
H. Goldberg, “Constraint on the Photino Mass from Cosmology,” Physical Review Letters, Vol. 50, No. 19, 1983, pp. 1419-1422.
|
[49]
|
J. Ellis, et al., “Towards a Supersymmetric Cosmology,” Physics Letters B, Vol. 147, No. 1-3, 1984, pp. 27-33.
doi:10.1016/0370-2693
|
[50]
|
S. Dodelson and L. M. Widrow, “Sterile Neutrinos as Dark Matter,” Physical Review Letters, Vol. 72, 1994, pp. 17-20. doi:10.1103/PhysRevLett.72.17
|
[51]
|
L. M. Krauss, “New Constraints on ‘INO’ Masses from Cosmology (I). Supersymmetric INOS,” Nuclear Physics B, Vol. 227, No. 3, 1983, pp. 556-569.
doi:10.1016/0550-3213
|
[52]
|
D. V. Nanopoulos, et al., “After Primordial Inflation,” Physics Letters B, Vol. 127, No. 1-2, 1983, pp. 30-34.
doi:10.1016/0370-2693
|
[53]
|
R. Juszkiewicz, et al., “Constraints on Cosmologically Regenerated Gravitinos,” Physics Letters B, Vol. 158, No. 6, 1985, pp. 463-467.doi:10.1016/0370-2693
|
[54]
|
M. Bolz, et al., “Thermal Production of Gravitinos,” Nuclear Physics B, Vol. 606, No. 1-2, 2001, pp. 518-544.
doi:10.1016/S0550-3213
|
[55]
|
J. L. Feng, et al., “Graviton Cosmology in Universal Extra Dimensions,” Physical Review D, Vol. 68, No. 8, 2003, Article ID: 085018.
|
[56]
|
J. R. Ellis, et al., “Prospects for Sparticle Discovery in Variants of the MSSM,” Physics Letters B, Vol. 603, No. 1, 2004, pp. 51-62.
|
[57]
|
K. Rajagopal, et al., “Cosmological Implications of Axinos,” Nuclear Physics B, Vol. 358, No. 2, 1991, pp. 447-470. doi:10.1016/0550-3213
|
[58]
|
L. Covi, et al., “Axinos as Dark Matter,” Journal of High Energy Physics, Vol. 5, No. 8, 2001, p. 33.
|
[59]
|
H. Baer and A. D. Box, “Fine-Tuning Favors Mixed Axion/Axino Cold Dark Matter over Neutralinos in the Minimal Supergravity Model,” European Physical Journal C, Vol. 68, No. 3, 2010, pp. 523-537.
|
[60]
|
J. Cembranos, et al., “Resolving Cosmic Gamma Ray Anomalies with Dark Matter Decaying Now,” Physical Review Letters, Vol. 99, No. 9, 2007,Article ID: 191301.
|
[61]
|
H. C. Cheng, et al., “Kaluza-Klein Dark Matter,” Physical Review Letters, Vol. 89, 2002, Article ID: 211301.
|
[62]
|
G. Servant and T. M. T. Tait, “Is the Lightest Kaluza-Klein Particle a Viable Dark Matter Candidate?” Nuclear Physics B, Vol. 650, No. 1-2, 2003, pp. 391-419.
doi:10.1016/S0550-3213(02)01012-X
|
[63]
|
S. W. Hawking, “Gravitationally Collapsed Objects of Very Low Mass,” Monthly Notices of the Royal Astronomical Society, Vol. 152, 1971, p. 75.
|
[64]
|
S. W. Hawking, “Particle Creation by Black Holes,” Communications in Mathematical Physics, Vol. 43, No. 3, 1971, pp. 199-220.
|
[65]
|
S. W. Hawking, “Black Hole Explosions?” Nature, Vol. 248, No. 5443, 1974, pp. 30-31.
|
[66]
|
D. N. Page, “Particle Emission Rates from a Black Hole: Massless Particles from an Uncharged, Nonrotating Hole,” Physical Review D, Vol. 13, 1976, pp. 198-206.
|
[67]
|
R. Hadgedron, “Statistical Thermodynamics of Strong Interactions at High Energies,” Nuovo Cimento, Vol. 3, 1965, pp. 147-186.
|
[68]
|
D. B. Cline and D. A. Sanders, “Further Evidence for Some Gamma-Ray Bursts Consistent with Primordial Black Hole Evaporation,” Astrophysical Journal, Vol. 486, No. 1, 1997, pp. 169-178. doi:10.1086/304480
|
[69]
|
S. Al Dallal, “Primordial Black Holes and Holeums as Progenitors of Galactic Diffuse Gamma-Ray Background,” Advances in Space Research, Vol. 46, No. 4, 2010, pp. 468-471. doi:10.1016/j.asr.2010.05.005
|
[70]
|
D. B. Cline, “A Gamma-Ray Halo ‘Glow’ from Primordial Black Hole Evaporation,” Astrophysical Journal, Vol. 501, No. 1, 1998, pp. L1-L3. doi:10.1086/311433
|
[71]
|
J. L. Osborne, et al., “The Diffuse Flux of Energetic Extragalactic Gamma Rays,” Journal of Physics G, Vol. 20, No. 7, 1994, pp. 1089-1101.
|
[72]
|
D. D. Dixon, et al., “Evidence for a Galactic Gamma-Ray Halo,” New Astronomy, Vol. 3, No. 7, 1998, pp. 539-561.
doi:10.1016/S1384-1076
|
[73]
|
L. K. Chavda and A. L. Chavda, “Dark Matter and Stable Bound States of Primordial Black Holes,” Classical and Quantum Gravity, Vol. 19, No. 11, 2002, pp. 2927-2938.
doi:10.1088/0264-9381/19/11/311
|
[74]
|
B. Paczynski, “Gravitational Microlensing by the Galactic Halo,” Astrophysical Journal, Vol. 304, 1986, pp. 1-5.
doi:10.1086/164140
|
[75]
|
D. S. Graff and K. Frees, “Analysis of a Hubble Space Telescope Search for Red Dwarfs: Limits on Baryonic Matter in the Galactic Halo,” The Astrophysical Journal Letters, Vol. 456, No. 1, 1996, p. L49.
doi:10.1086/309850
|
[76]
|
J. R. Najita, et al., “From Stars to Superplanets: The Low-Mass Initial Mass Function in the Young Cluster IC 348,” Astrophysical Journal, Vol. 541, No. 2, 2000, pp. 977-1003. doi:10.1086/309477
|
[77]
|
I. A. Bond, et al., “OGLE 2003-BLG-235/MOA 2003-BLG-53: A Planetary Microlensing Event,” The Astrophysical Journal Letters, Vol. 606, No. 2, 2004, pp. L155-L158. doi:10.1086/420928
|
[78]
|
A. Udalski, et al., “A Jovian-Mass Planet in Microlensing Event OGLE-2005-BLG-071,” The Astrophysical Journal Letters, Vol. 628, No. 2, 2005, pp. L109-L112.
doi:10.1086/432795
|
[79]
|
A. Gould, et al., “Microlens OGLE-2005-BLG-169 Implies That Cool Neptune-like Planets Are Common,” The Astrophysical Journal Letters, Vol. 644, No. 1, 2006, pp. L37-L40. doi:10.1086/505421
|
[80]
|
B. S. Gaudi, et al., “Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing,” Science, Vol. 319, No. 5865, 2008, pp. 927-930.
|
[81]
|
M. Milgrom, “A Modification of the Newtonian Dynamics as a Possible Alternative to the Hidden Mass Hypothesis,” Astrophysical Journal, Vol. 270, 1983, pp. 365-370. doi:10.1086/161130
|
[82]
|
M. Milgrom, “A Modification of the Newtonian Dynamics-Implications for Galaxies,” Astrophysical Journal, Vol. 270, 1983, pp. 371-389. doi:10.1086/161131
|
[83]
|
R. H. Sanders, “Modified Newtonian Dynamics and its Implications,” Proceedings of the Space Telescope Science Institute Symposium, Baltimore, 2-5 May 2001, p. 62.
|
[84]
|
L. Smolin, “The Trouble with Physics: The Rise of String Theory, the Fall of a Science, and What Comes Next,” Houghton Mifflin Co., New York, 2006.
|
[85]
|
R. Wojtak, et al., “Gravitational Redshift of Galaxies in Clusters as Predicted by General Relativity,” Nature, Vol. 477, No. 7366, 2011, pp. 567-569.
|
[86]
|
J. D. Bekenstein, “The Modified Newtonian Dynamics-MOND-and Its Implications for New Physics,” Contemporary Physics, Vol. 47, No. 6, 2006, p. 387.
doi:10.1080/00107510701244055
|
[87]
|
J. Moffat, “Gravitational Theory, Galaxy Rotation Curves and Cosmology without Dark Matter,” Journal of Cosmology and Astroparticle Physics, Vol. 5, 2005, p. 3.
|
[88]
|
P. D. Mannheim, “Alternatives to Dark Matter and Dark Energy,” Progress in Particle and Nuclear Physics, Vol. 56, 2006, pp. 340-445.
|
[89]
|
D. J. Gross, et al., “Heterotic String Theory: (II). The Interacting Heterotic String,” Nuclear Physics B, Vol. 267, No. 1, 1986, pp. 75-124.
doi:10.1016/0550-3213(86)90146-X
|
[90]
|
L. van Wawebeck, et al., “Detection of Correlated Galaxy Ellipticities on CFHT Data: First Evidence for Gravitational Lensing by Large Scale Structures,” Astronomy & Astrophysics, Vol. 358, No. 1, 2000, pp. 30-44.
|