Does the small CMB quadrupole moment suggest new physics

Motivated by WMAP's confirmation of an anomalously low value of the quadrupole moment of the CMB temperature fluctuations, we investigate the effects on the CMB of cutting off the primordial power spectrum P(k) at low wave numbers. This could arise, for example, from a break in the inflaton potential, a prior period of matter or radiation domination, or an oscillating scalar field which couples to the inflaton. We reanalyse the full WMAP parameter space supplemented by a low-k cutoff for P(k). The temperature correlations by themselves are better fit by a cutoff spectrum, but including the TE temperature-polarization spectrum reduces this preference to a 1.4σ effect. Inclusion of large scale structure data does not change the conclusion. If taken seriously, the low-k cutoff is correlated with optical depth so that reionization occurs even earlier than indicated by the WMAP analysis.

[1]  E. Gaztañaga,et al.  Two‐point anisotropies in WMAP and the cosmic quadrupole , 2003 .

[2]  Xinmin Zhang,et al.  Double inflation and the low CMB quadrupole , 2003, astro-ph/0305020.

[3]  D. Baumann,et al.  CMB-induced cluster polarization as a cosmological probe , 2003, astro-ph/0304416.

[4]  J.Wagg,et al.  2-point anisotropies in WMAP and the Cosmic Quadrupole , 2003, astro-ph/0304178.

[5]  C. Contaldi,et al.  Suppressing the lower multipoles in the CMB anisotropies , 2003, astro-ph/0303636.

[6]  J. Weeks,et al.  Cosmic microwave background constraints on lens spaces , 2003, astro-ph/0303580.

[7]  Andrei Linde Can we have inflation with Ω > 1?* , 2003, astro-ph/0303245.

[8]  A. Peet,et al.  SD-brane gravity fields and rolling tachyons , 2003, hep-th/0303035.

[9]  Max Tegmark,et al.  High resolution foreground cleaned CMB map from WMAP , 2003, astro-ph/0302496.

[10]  J. Weller,et al.  Reconstructing the primordial power spectrum , 2003, astro-ph/0302306.

[11]  Edward J. Wollack,et al.  First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters , 2003, astro-ph/0302209.

[12]  Edward J. Wollack,et al.  First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results , 2003, astro-ph/0302207.

[13]  Edward J. Wollack,et al.  First-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Parameter Estimation Methodology , 2003, astro-ph/0302218.

[14]  J. Weeks,et al.  Simulating cosmic microwave background maps in multiconnected spaces , 2002, astro-ph/0212223.

[15]  F. Lemieux,et al.  Are inflationary predictions sensitive to very high energy physics , 2002, hep-th/0210233.

[16]  R. Ellis,et al.  The 2dF Galaxy Redshift Survey: the power spectrum and the matter content of the Universe , 2001, astro-ph/0105252.

[17]  J. Yokoyama Chaotic new inflation and primordial spectrum of adiabatic fluctuations , 1999 .

[18]  A. Jaffe,et al.  Radical Compression of Cosmic Microwave Background Data , 1998, astro-ph/9808264.

[19]  J. Lesgourgues,et al.  CDM models with a BSI step-like primordial spectrum and a cosmological constant , 1998 .

[20]  J. Lesgourgues,et al.  CDM models with a BSI steplike primordial spectrum and a cosmological constant , 1997, astro-ph/9711139.

[21]  U. Seljak,et al.  A Line of sight integration approach to cosmic microwave background anisotropies , 1996, astro-ph/9603033.

[22]  A. Loeb,et al.  Faraday Rotation of Microwave Background Polarization by a Primordial Magnetic Field , 1996, astro-ph/9601055.

[23]  U. Seljak Gravitational Lensing Effect on Cosmic Microwave Background Anisotropies: A Power Spectrum Approach , 1995, astro-ph/9505109.

[24]  L. Knox,et al.  Determination of inflationary observables by cosmic microwave background anisotropy experiments. , 1995, Physical review. D, Particles and fields.

[25]  Y. Jing,et al.  An infrared cutoff revealed by the two years of COBE observations of cosmic temperature fluctuations. , 1994, Physical review letters.

[26]  Copeland,et al.  Reconstructing the inflaton potential: In principle and in practice. , 1993, Physical review. D, Particles and fields.

[27]  Hodges,et al.  Arbitrariness of inflationary fluctuation spectra. , 1990, Physical review. D, Particles and fields.

[28]  A. Vilenkin,et al.  Gravitational Effects upon Cosmological Phase Transitions , 1982 .

[29]  A. Starobinsky Spectrum of adiabatic perturbations in the universe when there are singularities in the inflation potential , 1992 .

[30]  Edward J. Wollack,et al.  Wilkinson Microwave Anisotropy Probe (WMAP) first year observations: TE polarization , 2003, astro-ph/0302213.