CMBPol Mission Concept Study Probing Ination with CMB Polarization

By D. Baumann, M. Jackson, Peter Adshead, A. Amblard, A. Ashoorioon, N. Bartolo, R. Bean, M. Beltrán, F. Bernardis, Simeon Bird and 49 more. 2008

277 citations recorded by the source corpus.

We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of ination. We focus on the prospects for using CMB measurements

Subfields: Astronomy and Astrophysics, Finance, Oceanography

View Paper: https://www.semanticscholar.org/paper/90da4b29d364f1f6a70c59b6af5f5bb29d3514e8

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. D. Baumann
2. L. Senatore
3. E. Pajer
4. M. Zaldarriaga
5. Liam McAllister
6. Marco Peloso
7. Xingang Chen
8. D. Green

In Finance

1. D. Baumann
2. J. Fergusson
3. L. Senatore
4. M. Liguori
5. Andrei Linde
6. V. Vennin
7. V. Poulin
8. A. Starobinsky

In Oceanography

1. E. Pajer
2. L. Senatore
3. D. Baumann
4. D. Green
5. M. Liguori
6. M. Zaldarriaga
7. D. Roest
8. J. Fergusson

Citations in the corpus

• Inflationary Cosmology after Planck 2013 (2014, background): “18 Appendix: Alternatives to inflation?”
• Cosmological non-linearities as an effective fluid (2010, background): “Many models of inflation indeed produce initial conditions where vector modes are zero and tensor modes are negligibly small [53, 54].”
• On soft limits of inflationary correlation functions (2012, methodology): “Looking ahead, LSS-experiments like EUCLID [63] and LSST [64], as well as CMB-experiments like PIXIE [65] and CMBPol [66] all have the potential to teach us a great deal about the soft limits of inflationary correlations.”
• Equilateral Non-Gaussianity and New Physics on the Horizon (2011, unknown): “NL ) ∼ 10 (CMBPol [35], COrE [36]).”
• COrE (Cosmic Origins Explorer) A White Paper (2011, background): “[67] and foreground subtraction residuals are also included [68] with the aim of propagating their effect into parameter uncertainties.”
• D3-brane potentials from fluxes in AdS/CFT (2010, background): “In a rather economical way, inflation explains both the large-scale homogeneity of the universe and the small-scale inhomogeneities required for the formation of galaxies [6, 7].”
• Observable non-gaussianity from gauge field production in slow roll inflation, and a challenging connection with magnetogenesis (2012, background): “which gives the amplitude of the power spectrum from the usual vacuum fluctuations [56].”
• Exploring cosmic origins with CORE: Inflation (2016, background): “The CMB-Pol mission concept study produced a number of detailed white papers, one of which deals with inflation [17] and thus has much overlap with this work, and also specialized white papers on foregrounds [18, 19] and gravitational lensing [20], as well as a general overview paper [21].”
• Searching for slow-roll moduli inflation in massive type IIA supergravity with metric fluxes (2008, background): “According to the most naive estimates, the scale of inflation may only be few orders of magnitude below the Planck scale, implying that cosmology might even provide an experimental test for string theory [1], [2], quite likely the only one in the foreseeable future.”