Hael Collins
Department of Physics
Carnegie Mellon University
Pittsburgh, PA 15213, United States

Overview

Research

Articles

Seminars

Courses

Lectures

Seminars and conference talks

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The influence of inhomogeneities on the large-scale expansion of the universe,
University of Sussex, Cosmology Seminar, October 8, 2010.

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A few unanswered questions about the inflationary picture,
ESQG 2010, NORDITA, Stockholm, July 12–16, 2010, Invited Talk.

Enhancing non-Gaussianities by breaking local Lorentz invariance,
Lancaster University, Cosmology and High Energy Physics Seminar, November 27, 2009.

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Enhancing non-Gaussianities by breaking local Lorentz invariance,
PASCOS 2009, DESY, Hamburg, July 6–10, 2009, Parallel Session Talk.

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Enhancing non-Gaussianities by breaking local Lorentz invariance,
The Invisible Universe International Conference, Palais de l’UNESCO, June 29–July 3, 2009, Parallel Session Talk.

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Testing the inflationary picture,
Particle Physics and Cosmology: From the Smallest Scales to the Largest, Nordic Researcher Networks Meeting, Niels Bohr International Academy, April 1–3, 2009, Parallel Session Talk.

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Trans-Planckian relics in the scalar to tensor ratio,
The Second UniverseNet Meeting, Seeking Links between Fundamental Physics and Cosmology
, University of Oxford, September 22–26, 2008, Parallel Session Talk.

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Unparticles and inflation,
Lund University, High Energy Physics Seminar, May 15, 2008.

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Unparticles and inflation,
The Niels Bohr Institute, The NBIA workshop on Field Theory and Cosmology, March 27, 2008.

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Effective theory approaches to the trans-Planckian problem,
The Niels Bohr Institute, Theoretical Particle Physics and Cosmology Seminar, February 5, 2008.

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Cosmic signals from the breaking of local Lorenz invariance,
University of Massachusetts, High Energy and Nuclear Seminar, May 11, 2007.

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Ripples in the cosmos,
Columbia University, Graduate Student Seminar, March 23, 2007.

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The light from beyond the stars,
Columbia University, Undergraduate Seminar, March 22, 2007.

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Seeking finer structures in the CMB: An effective theory for an initial state of inflation,
Los Alamos National Laboratory, T-8 Theory Seminar, February 26, 2007.

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Seeking finer structures in the CMB: An effective theory for an initial state of inflation,
University of South Carolina, Physics Colloquium, February 6, 2007.

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Ripples in the cosmos,
University of Buffalo, Physics Colloquium, January 30, 2007.

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An effective theory of initial conditions in inflation,
PASCOS 2006, Ohio State University, September 10–15, 2006, Parallel Session Talk.

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The effective theory of an initial state,
Perimeter Institute Workshop, Natural Ultraviolet Cutoffs in Expanding Space-times, September 5–8, 2006.

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Energy-momentum divergences and the renormalization of gravity,
University of Massachusetts, High Energy Lunch Talk, April 4, 2006.

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An effective theory of initial conditions in inflation,
University of North Carolina, Chapel Hill, Cosmology Seminar, February 24, 2006.

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Beyond the big bang,
University of North Carolina, Chapel Hill, Colloquium, February 23, 2006.

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An effective theory of initial conditions in inflation,
New Views of the Universe, University of Chicago, December 12, 2005, Parallel Session Talk.

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An effective theory of initial conditions in inflation,
University of Toronto, High Energy Physics Seminar, November 14, 2005 and
Perimeter Institute, Cosmology Seminar, November 15, 2005.

An effective theory of initial conditions in inflation,
University of Massachusetts, High Energy Lunch Talk, November 8, 2005.

Renormalization of initial conditions and the trans-Planckian problem of inflation,
Frontiers in Contemporary Physics III, Vanderbilt University, May 23–28, 2005, Parallel Session Talk.

Initial conditions and renormalization,
Virginia Tech, Particle Physics and Astrophysics Seminar, November 1, 2004.

Initial conditions and propagation
COSMO-04, University of Toronto, September 17–21, 2004, Parallel Session Talk.

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The taming of the α-vacuum,
PASCOS 2004, Northeastern University, August 16–22, 2004, Parallel Session Talk.

Taming the α-vacuum,
University of Massachusetts, High Energy/Nuclear Seminar, May 14, 2004.

The fate of the α-vacuum,
Fermilab, Theory Seminar, March 25, 2004 and
Purdue University, High Energy Theory Seminar, March 23, 2004.

The fate of the α-vacuum,
Yale University, Particle Theory Seminar, February 5, 2004 and
Cornell University, Particle Theory Seminar, February 4, 2004.

The fate of the α-vacuum,
University of Madison, String Theory Seminar, November 18, 2003.

The fate of the α-vacuum,
Fermilab Workshop, de Sitter Days, November 13–15, 2003.

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The fate of the α-vacuum,
International Symposium on Quantum Theory and Symmetries, University of Cincinnati, September 10–14, 2003, Parallel Session Talk.

The fate of the α-vacuum,
PHENO 2003 Symposium, University of Madison, May 5–7, 2003, Parallel Session Talk.

Radion-induced brane preheating,
COSMO-02, Chicago, September 18–21, 2002, Parallel Session Talk.

The Randall-Sundrum cosmology as brane dynamics in an AdS-S bulk,
Theory Institute 2002, Argonne National Laboratory, September 9–13, 2002.

Radion-induced brane preheating,
Extra Dimensions and Beyond, Santa Fe 2002 Summer Workshop, August 4–10, 2002.

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The Randall-Sundrum scenario with an extra warped dimension,
MRST 2001, University of Western Ontario, May 15–18, 2001.

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The Randall-Sundrum scenario with an extra warped dimension,
PASCOS 2001, University of North Carolina Chapel Hill, April 9–14, 2001, Parallel Session Talk.

Hiding a cosmological constant in a warped extra dimension,
Carnegie Mellon University, High Energy Theory Seminar, January 29, 2001.

Hiding a cosmological constant in a warped extra dimension,
Argonne National Laboratory, Theory Seminar, January 22, 2001.

The cosmological constant and warped extra dimensions,
University of Toronto, High Energy Physics Seminar, December 12, 2000.

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Brane cosmologies without orbifolds,
MRST 2000, University of Rochester, May 8–9, 2000.

Brane cosmologies without orbifolds,
University of Toronto, High Energy Physics Seminar, April 20, 2000.

Many of the older talks were created with a version of Powerpoint designed for Macintosh computers running OS 9; so some of the fonts, especially in the equations, will not appear correctly on other operating systems.