PA
Pavan Kumar Aluri
Also known as: Pavan K. Aluri
Indian Institute of Technology (BHU), Korea Institute for Advanced Study, Indian Institute of Technology Kanpur, University of Hyderabad, University of Cape Town, Acharya Nagarjuna University
About
My primary area of research is in cosmology, specifically Cosmic Microwave Background (CMB) studies - theory and data analysis, Modified theories of gravity, and tests of statistical isotropy. I would like to expand my understanding of using other probes of Cosmology to gain a better insight into the origin and evolution of our universe.
Employment
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Indian Institute of Technology (BHU) Assistant Professor2018 - Present
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Korea Institute for Advanced Study KIAS-KASI Joint Post-doctoral fellow2017 - 2018
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University of Cape Town Claude Leon Post-doctoral fellow2016 - 2017
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Inter-University Centre for Astronomy and Astrophysics Post-doctoral fellow2013 - 2016
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Indian Institute of Science Education and Research Bhopal Post-doctoral fellow2012 - 2013
Education
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Indian Institute of Technology Kanpur Ph.D.2005 - 2013
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University of Hyderabad M.Sc.2002 - 2004
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Acharya Nagarjuna University B.Sc.1999 - 2002
Projects & Funding
Projects & funding information is unavailable.
Publications (20)
- Parity in Planck full-mission CMB temperature maps Save
- Corrigendum to ``Parity in Planck full-mission CMB temperature maps'' [Astroparticle Physics, Vol. 125 (2021), 102493] Save
- Large Angular-scale Multipoles at Redshift \ensuremath∼ 0.8 Save
- Testing statistical isotropy in cosmic microwave background polarization maps Save
- Alignments of parity even/odd-only multipoles in CMB Save
- Improved Diffuse Foreground Subtraction with the ILC Method: CMB Map and Angular Power Spectrum Using Planck and WMAP Observations Save
- A Perturbative Analysis of Synchrotron Spectral Index Variation over the Microwave Sky Save
- Planck 2015 results. XVI. Isotropy and statistics of the CMB Save
- Cross-correlation analysis of CMB with foregrounds for residuals Save
- Direction dependence of cosmological parameters due to cosmic hemispherical asymmetry Save