The Cosmic Microwave Background and Fundamental Physics

[1]  Raphael Flauger,et al.  Oscillations in the CMB from axion monodromy inflation , 2009, 0907.2916.

[2]  P. A. R. Ade,et al.  MEASUREMENT OF COSMIC MICROWAVE BACKGROUND POLARIZATION POWER SPECTRA FROM TWO YEARS OF BICEP DATA , 2009, 0906.1181.

[3]  A. Challinor,et al.  Lecture notes on the physics of cosmic microwave background anisotropies , 2009, 0903.5158.

[4]  P. Lilje,et al.  INCREASING EVIDENCE FOR HEMISPHERICAL POWER ASYMMETRY IN THE FIVE-YEAR WMAP DATA , 2009, 0903.1229.

[5]  Steven Gratton,et al.  B-mode Detection with an Extended Planck Mission , 2009, 0903.0345.

[6]  A. Pontzen.  Rogues' gallery: the full freedom of the Bianchi CMB anomalies , 2009, 0901.2122.

[7]  M. Hobson,et al.  Anisotropic, nonsingular early universe model leading to a realistic cosmology , 2008, 0809.4335.

[8]  P. Ferreira,et al.  Constraining Lorentz violation with cosmology. , 2008, Physical review letters.

[9]  B. Wandelt,et al.  Evidence of primordial non-Gaussianity (fNL) in the Wilkinson microwave anisotropy probe 3-year data at 2.8sigma. , 2008, Physical review letters.

[10]  P. Steinhardt,et al.  Intuitive understanding of non-gaussianity in ekpyrotic and cyclic models , 2008, 0804.1293.

[11]  Edward J. Wollack,et al.  FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION , 2008, 0803.0547.

[12]  J. Uzan,et al.  Predictions from an anisotropic inflationary era , 2008, 0801.3596.

[13]  J. Bond,et al.  HIGH-RESOLUTION CMB POWER SPECTRUM FROM THE COMPLETE ACBAR DATA SET , 2008, 0801.1491.

[14]  A. Lasenby,et al.  Bianchi VIIh models and the cold spot texture , 2007, 0712.1789.

[15]  M. Hobson,et al.  A Cosmic Microwave Background Feature Consistent with a Cosmic Texture , 2007, Science.

[16]  C. Contaldi,et al.  Inflationary perturbations in anisotropic backgrounds and their imprint on the cosmic microwave background , 2007, 0707.4179.

[17]  P. Stefanescu,et al.  Constraints on time variation of fine structure constant from WMAP-3yr data , 2007, 0707.0190.

[18]  A. Pontzen,et al.  Bianchi model CMB polarization and its implications for CMB anomalies , 2007, 0706.2075.

[19]  Andrei Linde,et al.  Testing string theory with cosmic microwave background , 2007 .

[20]  L. McAllister,et al.  A Microscopic Limit on Gravitational Waves from D-brane Inflation , 2006, hep-th/0610285.

[21]  D. Boyanovsky,et al.  CMB quadrupole suppression: II. The early fast roll stage , 2006, astro-ph/0607487.

[22]  A. Lasenby,et al.  Markov chain Monte Carlo analysis of Bianchi VIIh models , 2006, astro-ph/0605325.

[23]  Edward J. Wollack,et al.  Three Year Wilkinson Microwave Anistropy Probe (WMAP) Observations: Polarization Analysis , 2006, astro-ph/0603450.

[24]  K. Gorski,et al.  On the Viability of Bianchi Type VIIh Models with Dark Energy , 2005, astro-ph/0512433.

[25]  A. Slosar,et al.  Test of modified newtonian dynamics with recent boomerang data , 2005 .

[26]  Yen-Ting Lin,et al.  Wilkinson Microwave Anisotropy Probe Constraints on the Intracluster Medium , 2005 .

[27]  K. Gorski,et al.  Evidence of Vorticity and Shear at Large Angular Scales in the WMAP Data: A Violation of Cosmological Isotropy? , 2005, astro-ph/0503213.

[28]  J. Bekenstein.  Relativistic gravitation theory for the modified newtonian dynamics paradigm , 2004 .

[29]  E.Martinez-Gonzalez,et al.  Detection of a non‐Gaussian spot in WMAP , 2004, astro-ph/0405341.

[30]  E. Silverstein,et al.  DBI in the sky , 2004, hep-th/0404084.

[31]  P. Lilje,et al.  Asymmetries in the Cosmic Microwave Background Anisotropy Field , 2004 .

[32]  J. Bekenstein.  Relativistic gravitation theory for the MOND paradigm , 2004, astro-ph/0403694.

[33]  R. B. Barreiro,et al.  Detection of Non-Gaussianity in the Wilkinson Microwave Anisotropy Probe First-Year Data Using Spherical Wavelets , 2003, astro-ph/0310273.

[34]  A. Melchiorri,et al.  New constraints on varying α , 2003, astro-ph/0309205.

[35]  C. Doran,et al.  Closed universes, de Sitter space, and inflation , 2003, astro-ph/0307311.

[36]  Matias Zaldarriaga,et al.  Significance of the largest scale CMB fluctuations in WMAP , 2003, astro-ph/0307282.

[37]  G. Efstathiou,et al.  Is the low cosmic microwave background quadrupole a signature of spatial curvature , 2003, astro-ph/0303127.

[38]  M. Kaplinghat,et al.  Constraining variations in the fine structure constant with the cosmic microwave background , 1998, astro-ph/9810133.

[39]  S. Carroll.  QUINTESSENCE AND THE REST OF THE WORLD : SUPPRESSING LONG-RANGE INTERACTIONS , 1998, astro-ph/9806099.

[40]  D. Lyth.  What Would We Learn by Detecting a Gravitational Wave Signal in the Cosmic Microwave Background Anisotropy , 1996, hep-ph/9606387.

[41]  S. Fulling,et al.  Book-Review - Aspects of Quantum Field Theory in Curved Spacetime , 1989 .

[42]  J. Barrow,et al.  Universal rotation - How large can it be? , 1985 .

[43]  M. Milgrom.  A modification of the newtonian dynamics as a possible alternative to the hidden mass hypothesis , 1983 .

[44]  S. Hawking,et al.  The Rotation and Distortion of the Universe , 1973 .

[45]  S. Hawking.  On the Rotation of the Universe , 1969 .

[46]  R. Sachs,et al.  Perturbations of a Cosmological Model and Angular Variations of the Microwave Background , 1967 .

[47]  ournal of C osmology and A stroparticle hysics J Theory of cosmological perturbations in an anisotropic universe , 2022 .