CMB polarization by the asymmetric template of scalar perturbations
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[1] V. Sreenath,et al. Large scale anomalies in the CMB and non-Gaussianity in bouncing cosmologies , 2020, Classical and Quantum Gravity.
[2] A. Marcos-Caballero,et al. Scale-dependent dipolar modulation and the quadrupole-octopole alignment in the CMB temperature , 2019, Journal of Cosmology and Astroparticle Physics.
[3] M. Sadegh,et al. B-mode power spectrum of CMB via polarized Compton scattering , 2019, Journal of Cosmology and Astroparticle Physics.
[4] Lucy Rosenbloom. arXiv , 2019, The Charleston Advisor.
[5] R. B. Barreiro,et al. Planck 2018 results. IX. Constraints on primordial non-Gaussianity , 2019, 1905.05697.
[6] J. Aumont,et al. Planck2018 results , 2018, Astronomy & Astrophysics.
[7] Shamik Ghosh,et al. A pixel space method for testing dipole modulation in the CMB polarization , 2018, 1807.02359.
[8] M. Haghighat,et al. Dipolar dark matter and CMB B-mode polarization , 2018, The European Physical Journal C.
[9] P. K. Rath,et al. Testing statistical isotropy in cosmic microwave background polarization maps , 2017, 1707.04076.
[10] C. A. Oxborrow,et al. Planck2015 results , 2015, Astronomy & Astrophysics.
[11] S. Tizchang,et al. Cosmic microwave background polarization in non-commutative space-time , 2016, The European Physical Journal C.
[12] D. Wands,et al. Expected dipole asymmetry in CMB polarization , 2014, 1411.5312.
[13] D. Wands,et al. CMB hemispherical asymmetry from non-linear isocurvature perturbations , 2014, 1410.8036.
[14] K. Koyama,et al. The intrinsic B-mode polarisation of the Cosmic Microwave Background , 2014, 1401.3296.
[15] P. K. Rath,et al. Testing the dipole modulation model in CMBR , 2013, 1308.0924.
[16] A. Mazumdar,et al. CMB dipole asymmetry from a fast roll phase , 2013, 1306.5736.
[17] C. A. Oxborrow,et al. Planck 2015 results: XXIII. The thermal Sunyaev-Zeldovich effect-cosmic infrared background correlation , 2015, 1509.06555.
[18] P. K. Rath,et al. Direction dependence of the power spectrum and its effect on the cosmic microwave background radiation , 2013, 1302.2706.
[19] Edward J. Wollack,et al. NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS , 2012, 1212.5226.
[20] Edward J. Wollack,et al. NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP) OBSERVATIONS: FINAL MAPS AND RESULTS , 2012, 1212.5225.
[21] P. Cochat,et al. Et al , 2008, Archives de pediatrie : organe officiel de la Societe francaise de pediatrie.
[22] Karim A. Malik,et al. Cosmological perturbations , 2008, Series on the Foundations of Natural Science and Technology.
[23] F. Vernizzi,et al. Non-linear isocurvature perturbations and non-Gaussianities , 2008, 0809.4646.
[24] C. Gordon. Broken Isotropy from a Linear Modulation of the Primordial Perturbations , 2006, astro-ph/0607423.
[25] U. Chicago,et al. On the large-angle anomalies of the microwave sky , 2005, astro-ph/0508047.
[26] P. Lilje,et al. The N-Point Correlation Functions of the First-Year Wilkinson Microwave Anisotropy Probe Sky Maps , 2004, astro-ph/0407271.
[27] J. García-Bellido,et al. Modern Cosmology , 2004, hep-ph/0407111.
[28] M. Giannotti,et al. Faraday Rotation of the Cosmic Microwave Background Polarization and Primordial Magnetic Field Properties , 2004, astro-ph/0405420.
[29] P. Lilje,et al. Asymmetries in the Cosmic Microwave Background Anisotropy Field , 2004 .
[30] 조남욱. 전자/제조업의 Collaboration 전략 , 2003 .
[31] T. Souradeep,et al. Measuring the Statistical Isotropy of the Cosmic Microwave Background Anisotropy , 2003 .
[32] A. Kosowsky. Cosmic microwave background polarization , 1995, astro-ph/9501045.
[33] J. R. Bond,et al. Cosmic background radiation anisotropies in universes dominated by nonbaryonic dark matter , 1984 .
[34] W. Hager,et al. and s , 2019, Shallow Water Hydraulics.
[35] J. Lesgourgues,et al. NEUTRINO IN COSMOLOGY , 2010 .
[36] J. Hearnshaw,et al. Monthly Notices of the Royal Astronomical Society , 1999 .
[37] V. Sreenath,et al. Anomalies in the CMB from a cosmic bounce , 2020, General Relativity and Gravitation.