170 results on '"McAllister, Liam"'
Search Results
152. On D3-brane potentials in compactifications with fluxes and wrapped D-branes
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Baumann, Daniel, primary, Dymarsky, Anatoly, additional, Klebanov, Igor R, additional, Maldacena, Juan, additional, McAllister, Liam, additional, and Murugan, Arvind, additional
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- 2006
- Full Text
- View/download PDF
153. Random matrices and the spectrum of N-flation
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Easther, Richard, primary and McAllister, Liam, additional
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- 2006
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154. An inflaton mass problem in string inflation from threshold corrections to volume stabilization
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McAllister, Liam, primary
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- 2006
- Full Text
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155. Relativistic D-brane Scattering is Extremely Inelastic
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McAllister, Liam, primary and Mitra, Indrajit, additional
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- 2005
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156. Beauty is Attractive: Moduli Trapping at Enhanced Symmetry Points
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Kofman, Lev, primary, Linde, Andrei, additional, Liu, Xiao, additional, Maloney, Alexander, additional, McAllister, Liam, additional, and Silverstein, Eva, additional
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- 2004
- Full Text
- View/download PDF
157. Heterotic moduli stabilization with fractional Chern-Simons invariants
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Gukov, Sergei, primary, Kachru, Shamit, additional, Liu, Xiao, additional, and McAllister, Liam, additional
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- 2004
- Full Text
- View/download PDF
158. Towards inflation in string theory
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Kachru, Shamit, primary, Kallosh, Renata, additional, Linde, Andrei, additional, Maldacena, Juan, additional, McAllister, Liam, additional, and Trivedi, Sandip P, additional
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- 2003
- Full Text
- View/download PDF
159. Bouncing brane cosmologies from warped string compactifications
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Kachru, Shamit, primary and McAllister, Liam, additional
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- 2003
- Full Text
- View/download PDF
160. CMBPol Mission Concept Study: Probing Inflation with CMB Polarization
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Baumann, Daniel, Jackson, Mark, Adshead, Peter, Amblard, Alexandre, Ashoorioon, Amjad, Bartolo, Nicola, Bean, Rachel, Beltran, Maria, de Bernardis, Francesco, Bird, Simeon, Chen, Xingang, Chung, Daniel, Colombo, Loris, Cooray, Asantha, Creminelli, Paolo, Dodelson, Scott, Dunkley, Joanna, Dvorkin, Cora, Easther, Richard, Finelli, Fabio, Flauger, Raphael, Hertzberg, Mark, Jones-Smith, Katherine, Kachru, Shamit, Kadota, Kenji, Khoury, Justin, Kinney, William, Komatsu, Eiichiro, Krauss, Lawrence, Lesgourgues, Julien, Liddle, Andrew, Liguori, Michele, Lim, Eugene, Linde, Andrei, Matarrese, Sabino, Mathur, Harsh, McAllister, Liam, Melchiorri, Alessandro, Nicolis, Alberto, Pagano, Luca, Peiris, Hiranya, Peloso, Marco, Pogosian, Levon, Pierpaoli, Elena, Riotto, Antonio, Seljak, Uros, Senatore, Leonardo, Shandera, Sarah, and Silverstein, Eva
- Abstract
We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measurements to differentiate various inflationary mechanisms. In particular, a detection of primordial B-mode polarization would demonstrate that inflation occurred at a very high energy scale, and that the inflaton traversed a super-Planckian distance in field space. We explain how such a detection or constraint would illuminate aspects of physics at the Planck scale. Moreover, CMB measurements can constrain the scale-dependence and non-Gaussianity of the primordial fluctuations and limit the possibility of a significant isocurvature contribution. Each such limit provides crucial information on the underlying inflationary dynamics. Finally, we quantify these considerations by presenting forecasts for the sensitivities of a future satellite experiment to the inflationary parameters., Physics
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- 2009
161. The Origin of the Universe as Revealed Through the Polarization of the Cosmic Microwave Background
- Author
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Dodelson, Scott, Easther, Richard, Hanany, Shaul, Mcallister, Liam, Meyer, Stephan, Page, Lyman, Ade, Peter, Amblard, Alexandre, Ashoorioon, Amjad, Baccigalupi, Carlo, Balbi, Amedeo, Bartlett, James, Bartolo, Nicola, Baumann, Daniel, Beltran, Maria, Benford, Dominic, Birkinshaw, Mark, Bock, Jamie, Bond, Dick, Borrill, Julian, Bouchet, Francois, Bridges, Michael, Bunn, Emory, Calabrese, Erminia, Cantalupo, Christopher, Caramete, Ana, Carbone, Carmelita, Carroll, Sean, Chatterjee, Suchetana, Chen, Xingang, Church, Sarah, Chuss, David, Contaldi, Carlo R., Cooray, Asantha R., Creminelli, Paolo, Das, Sudeep, Bernardis, Francesco, Bernardis, Paolo, Delabrouille, Jacques, Desert, F. Xavier, Devlin, Mark J., Dickinson, Clive, Dicker, Simon, Dipirro, Michael, Dobbs, Matt A., Dore, Olivier, Dotson, Jessie, Dunkley, Joanna, Dvorkin, Cora, Eriksen, H. K., Falvella, Maria Cristina, Finley, Dave, Finkbeiner, Douglas P., Fixsen, Dale, Flauger, Raphael, Fosalba, Pablo, Fowler, Joseph W., Galli, Silvia, Gates, Evalyn I., Gear, Walter, Giraud-Heraud, Yannick, Gorski, Krzysztof, Greene, Brian, Gruppuso, Alessandro, Gundersen, Joshua, Halpern, Mark, Hamilton, Jean-Christophe, Hazumi, Masashi, Hernandez-Monteagudo, Carlos, Hertzberg, Mark, Hinshaw, Gary, Hirata, Christopher, Hivon, Eric, Holman, Richard, Holmes, Warren, Hu, Wayne, Hubmayr, Johannes, Huffenberger, Kevin, Hui, Howard, Hui, Lam, Irwin, Kent, Jackson, Mark, Jaffe, Andrew H., Johnson, Bradley, Johnson, Dean, Jones, William, Kachru, Shamit, Kadota, Kenji, Kaplan, Jean, Kaplinghat, Manoj, Keating, Brian G., Keskitalo, Reijo, Khoury, Justin, Kinney, William H., Kisner, Theodore, Knox, Lloyd, Kodama, Hideo, Kogut, Alan, Komatsu, Eiichiro, Kosowsky, Arthur, Kovac, John, Krauss, Lawrence M., Kurki-Suonio, Hannu, Lamarre, Jean-Michel, Landau, Susana Judith, Lawrence, Charles, Leach, Samuel M., Leblond, Louis, Lee, Adrian, Leitch, Erik, Leonardi, Rodrigo, Lesgourgues, Julien, Liddle, Andrew R., Lim, Eugene A., Limon, Michele, Loverde, Marilena, Lubin, Philip, Lunghi, Enrico, Lykken, Joseph D., Mactavish, Carolyn, Magalhaes, Antonio, Maino, Davide, Martin, Victoria, Sabino Matarrese, Mather, John C., Mathur, Harsh, Matsumura, Tomotake, Meerburg, Pieter, Melchiorri, Alessandro, Mersini-Houghton, Laura, Miller, Amber, Milligan, Michael, Moodley, Kavilan, Neimack, Michael, Nguyen, Hogan, Nicolis, Alberto, O Dwyer, Ian, Olinto, Angela, Pagano, Luca, Pajer, Enrico, Partridge, Bruce, Pearson, Timothy, Peiris, Hiranya V., Peloso, Marco, Piacentini, Francesco, Piat, Michel, Piccirillo, Lucio, Pierpaoli, Elena, Pietrobon, Davide, Pisano, Giampaolo, Pogosian, Levon, Pogosyan, Dmitri, Ponthieu, Nicolas, Popa, Lucia, Pryke, Clement, Raeth, Christoph, Ray, Subharthi, Reichardt, Christian, Ricciardi, Sara, Richards, Paul, Riotto, Antonio, Rocha, Graca, Ruhl, John, Rusholme, Benjamin, Scherrer, Robert, Scoccola, Claudia, Scott, Douglas, Sealfon, Carolyn, Sefusatti, Emiliano, Sehgal, Neelima, Seiffert, Michael, Senatore, Leonardo, Serra, Paolo, Shandera, Sarah E., Shimon, Meir, Shirron, Peter, Sievers, Jonathan, Silk, Joseph I., Sigurdson, Kris, Silverberg, Robert F., Silverstein, Eva, Staggs, Suzanne, Starkman, Glenn D., Stebbins, Albert, Stivoli, Federico, Stompor, Radek, Sugiyama, Naoshi, Swetz, Daniel, Tartari, Andrea, Tegmark, Max, Timbie, Peter, Titov, Maxim P., Tristram, Matthieu, Trodden, Mark, Tucker, Gregory, Urrestilla, Jon, Veneziani, Marcella, Verde, Licia, Vieira, Joaquin, Walker, Terry, Wands, David, Watson, Scott, Weinberg, Steven, Weiss, Rainer, Wandelt, Benjamin, Winstein, Bruce D., Wollack, Edward, Wyman, Mark, Yadav, Amit, Yoon, Ki Won, Zahn, Olivier, Zaldarriaga, Matias, Zemcov, Michael, Zwart, Jonathan, APC - Cosmologie, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), APC - Gravitation (APC-Gravitation), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Max-Planck-Gesellschaft-Max-Planck-Gesellschaft, APC - Astrophysique des Hautes Energies (APC - AHE), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Bartlett, James, Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Physique Corpusculaire et Cosmologie - Collège de France (PCC), Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Collège de France (CdF)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut ) (AEI), PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, and Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO)
- Subjects
[SDU.ASTR.CO] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO] ,Astrophysics::Cosmology and Extragalactic Astrophysics - Abstract
Modern cosmology has sharpened questions posed for millennia about the origin of our cosmic habitat. The age-old questions have been transformed into two pressing issues primed for attack in the coming decade: How did the Universe begin? and What physical laws govern the Universe at the highest energies? The clearest window onto these questions is the pattern of polarization in the Cosmic Microwave Background (CMB), which is uniquely sensitive to primordial gravity waves. A detection of the special pattern produced by gravity waves would be not only an unprecedented discovery, but also a direct probe of physics at the earliest observable instants of our Universe. Experiments which map CMB polarization over the coming decade will lead us on our first steps towards answering these age-old questions.
162. Snowmass White Paper: Cosmology at the Theory Frontier
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Flauger, Raphael, Gorbenko, Victor, Austin Joyce, Mcallister, Liam, Shiu, Gary, and Silverstein, Eva
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High Energy Physics - Theory ,General Relativity and Quantum Cosmology ,High Energy Physics - Theory (hep-th) ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics - Abstract
The precision cosmological model describing the origin and expansion history of the universe, with observed structure seeded at the inflationary cosmic horizon, demands completion in the ultraviolet and in the infrared. The dynamics of the cosmic horizon also suggests an associated entropy, again requiring a microphysical theory. Recent years have seen enormous progress in understanding the structure of de Sitter space and inflation in string theory, and of cosmological observables captured by quantum field theory and solvable deformations thereof. The resulting models admit ongoing observational tests through measurements of the cosmic microwave background and large-scale structure, as well as through analyses of theoretical consistency by means of thought experiments. This paper, prepared for the TF01 and TF09 conveners of the Snowmass 2021 process, provides a synopsis of this important area, focusing on ongoing developments and opportunities., Comment: Contribution to Snowmass 2021
163. Snowmass Theory Frontier: Astrophysics and Cosmology
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Green, Daniel, Ruderman, Joshua T., Safdi, Benjamin R., Shelton, Jessie, Achucarro, Ana, Adshead, Peter, Akrami, Yashar, Baryakhtar, Masha, Baumann, Daniel, Berlin, Asher, Blinov, Nikita, Boddy, Kimberly K., Buschmann, Malte, Cabass, Giovanni, Caldwell, Robert, Castorina, Emanuele, Chen, Thomas Y., Chen, Xingang, Coulton, William, Croon, Djuna, Yanou Cui, Curtin, David, Cyr-Racine, Francis-Yan, Dessert, Christopher, Dienes, Keith R., Draper, Patrick, Du, Peizhi, Ellis, Sebastian A. R., Essig, Rouven, Flauger, Raphael, Fong, Chee Sheng, Foster, Joshua W., Fumagalli, Jacopo, Harigaya, Keisuke, Horiuchi, Shunsaku, Ivanov, Mikhail M., Kahn, Yonatan, Knapen, Simon, Leane, Rebecca K., Lee, Hayden, Lentz, Erik W., Lewandowski, Matthew, Lisanti, Mariangela, Long, Andrew J., Loverde, Marilena, Maleknejad, Azadeh, Mcallister, Liam, Mcdermott, Samuel D., Mcgehee, Robert, Meerburg, P. Daniel, Meyers, Joel, Dizgah, Azadeh Moradinezhad, Münchmeyer, Moritz, Outmezguine, Nadav Joseph, Pajer, Enrico, Palma, Gonzalo A., Parikh, Aditya, Park, Jong-Chul, Peter, Annika H. G., Pimentel, Guilherme L., Renaux-Petel, Sébastien, Rodd, Nicholas L., Shakya, Bibhushan, Shiu, Gary, Silverstein, Eva, Simonovic, Marko, Singh, Rajeev, Sleight, Charlotte, Takhistov, Volodymyr, Tanedo, Philip, Taronna, Massimo, Thomas, Brooks, Toro, Natalia, Tsai, Yu-Dai, Vitagliano, Edoardo, Vogelsberger, Mark, Wallisch, Benjamin, Wandelt, Benjamin D., Wechsler, Risa H., Weniger, Christoph, Wu, W. L. Kimmy, Xu, Weishuang Linda, Yamada, Masaki, Yu, Hai-Bo, Zhang, Zhengkang, Zhong, Yi-Ming, and Zurek, Kathryn
- Subjects
High Energy Physics - Theory ,High Energy Physics - Phenomenology ,Astrophysics and Astronomy ,High Energy Physics - Phenomenology (hep-ph) ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,High Energy Physics - Theory (hep-th) ,hep-th ,astro-ph.CO ,FOS: Physical sciences ,hep-ph ,Particle Physics - Theory ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Particle Physics - Phenomenology - Abstract
We summarize progress made in theoretical astrophysics and cosmology over the past decade and areas of interest for the coming decade. This Report is prepared as the TF09 "Astrophysics and Cosmology" topical group summary for the Theory Frontier as part of the Snowmass 2021 process., Comment: 57 pages
164. Stabilizing Antibrane Pseudomoduli
- Author
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Gandhi, Sohang, McAllister, Liam, Sjörs, Stefan, Gandhi, Sohang, McAllister, Liam, and Sjörs, Stefan
- Abstract
In a KKLT compactification, an anti-D3-brane at the tip of a warped deformed conifold region plays the crucial role of contributing positive vacuum energy. This antibrane also gives rise to light moduli, corresponding to angular motion around the tip. Following the work of Aharony, Antebi, and Berkooz, we characterize the leading effects due to compactification that lift these potentially dangerous pseudomoduli.We show that the dominant contribution to the anti-D3-brane potential arises from nonperturbative effects stabilizing the K\"ahler moduli. In ten-dimensional supergravity, this contribution is mediated by perturbations of three-form flux. Incorporating these flux perturbations, we compute the leading contribution to the potential for angular motion of the anti-D3-brane. We show that the resulting mass is parametrically larger than that obtained in prior work. However, we give a conclusive demonstration that bulk effects cannot stabilize the antibrane moduli above the IR scale without severe fine tuning.
165. The origin of the universe as revealed through the polarization of the cosmic microwave background
- Author
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Dodelson, Scott, Easther, Richard, Hanany, Shaul, McAllister, Liam, Meyer, Stephan, Page, Lyman, Ade, Peter A. R., Amblard, Alexander, Ashoorioon, Amjad, Baccigalupi, Carlo, Balbi, Amedeo, Bartlett, James, Bartolo, Nicola, Baumann, Daniel, Beltran, Maria, Benford, Dominic, Birkinshaw, Mark, Bock, Jamie, Bond, Dick, Borrill, Julian, Bouchet, Francois, Bridges, Michael, Bunn, Emory, Calabrese, Erminia, Cantalupo, Christopher, Caramete, Ana, Carbone, Carmelita, Carroll, Sean, Chatterjee, Suchetana, Chen, Xingang, Church, Sarah, Chuss, David, Contaldi, Carlo, Cooray, Asantha, Creminelli, Paolo, Das, Sudeep, de Bernardis, Francesco, de Bernardis, Paolo, Delabrouille, Jacques, Dsert, F. Xavier, Devlin, Mark, Dickinson, Clive, Dicker, Simon, DiPirro, Michael, Dobbs, Matt, Dore, Olivier, Dotson, Jessie, Dunkley, Joanna, Dvorklin, Cora, Eriksen, Hans Kristian, Falvella, Maria Christiana, Finley, Dave, Finkbeiner, Douglas, Fixen, Dale, Flauger, Raphael, Fosalba, Pablo, Fowler, Joseph, Galli, Silvia, Gates, Evalyn, Gear, Walter Kieran, Giraud-Heraud, Yannick, Gorski, Krzysztof, Greene, Brian, Gruppuso, Alessandro, Gundersen, Josh, Halpern, Mark, Hirata, Christopher, Hivon, Eric, Holman, Richard, Holmes, Warren, Hu, Wayne, Hubmayr, Johannes, Huffenberger, Kevin, Hui, Howard, Hui, Lam, Irwin, Kent, Jackson, Mark, Jaffe, Andrew, Johnson, Bradley, Johnson, Dean, Jones, William, Kachru, Shamit, Kadota, Kenji, Kaplan, Jean, Kaplinghat, Manoj, Keating, Brian, Keskitalo, Reijo, Khoury, Justin, Kinney, Will, Kisner, Theodore, Knox, Lloyd, Kodama, Hideo, Kogut, Alan, Komatsu, Eiichiro, Kosowsky, Reijo, Kurki-Suonio, Hannu, Lamarre, Jean-Michel, Landau, Susana, Leach, Samuel, Leblond, Louis, Lee, Adrian, Leitch, Erik, Leonardi, Rodrigo, Lesgourgues, Julien, Liddle, Andrew, Lim, Eugene, Limon, Michele, Loverde, Marilena, Lubin, Philip, Lunghi, Enrico, Lykken, Joseph, MacTavish, Carolyn, Magalhaes, Antonio, Maino, Davide, Martin, Victoria, Matarrese, Sabino, Mather, John, Mathur, Harsh, Matsumura, Tomotake, Meerburg, Pieter, Melchiorri, Alessandro, Mersini-Houghton, Laura, Miller, Amber, Milligan, Michael, Moodley, Kavilan, Neimack, Michael, Nguyen, Hogan, Nicolis, Alberto, O'Dwyer, Ian, Olinto, Angela, Pagano, Luca, Pajer, Enrico, Partridge, Bruce, Pearson, Timothy, Peiris, Hiranya, Peloso, Marco, Piacentini, Francesco, Piat, Michel, Piccirillo, Lucio, Pierpaoli, Elena, Pietrobon, Davide, Pisano, Giampaolo, Pogosian, Levon, Pogosyan, Dmitri, Ponthieu, Nicolas, Popa, Lucia, Pryke, Clement, Raeth, Christoph, Ray, Subharthi, Reichardt, Christian, Ricciardi, Sara, Richards, Paul, Riotto, Antonio, Rocha, Graca, Ruhl, John, Rusholme, Benjamin, Scherrer, Robert, Scoccola, Claudia, Scott, Douglas, Sealfon, Carolyn, Sefusatti, Emiliano, Sehgal, Neelima, Seiffert, Michael, Serra, Paolo, Shandera, Sarah, Shimon, Meir, Shirron, Peter, Sievers, Jonathan, Silk, Joe, Sigurdson, Kris, Silverberg, Robert, Silverstein, Eva, Staggs, Suzanne, Starkman, Glenn, Stebbins, Albert, Stivoli, Frederico, Stompor, Radek, Sugiyama, Naoshi, Swetz, Daniel, Tartari, Andrea, Tegmark, Max, Timbie, Peter, Titov, Maxim, Tristram, Matthieu, Trodden, Mark, Tucker, Gregory, Urrestilla, Jon, Veneziani, Marcella, Verde, Licia, Vieira, Joaquin, Walker, Terry, Wands, David, Watson, Scott, Weinberg, Steven, Weiss, Rainer, Wandelt, Benjamin, Winstein, Bruce, Wollack, Edward, Wyman, Mark, Yadav, Amit, Won Yoon, Ki, Zahn, Olivier, Zaldarriage, Mattias, Zemcov, Michael, Zwart, Jonathan, Dodelson, Scott, Easther, Richard, Hanany, Shaul, McAllister, Liam, Meyer, Stephan, Page, Lyman, Ade, Peter A. R., Amblard, Alexander, Ashoorioon, Amjad, Baccigalupi, Carlo, Balbi, Amedeo, Bartlett, James, Bartolo, Nicola, Baumann, Daniel, Beltran, Maria, Benford, Dominic, Birkinshaw, Mark, Bock, Jamie, Bond, Dick, Borrill, Julian, Bouchet, Francois, Bridges, Michael, Bunn, Emory, Calabrese, Erminia, Cantalupo, Christopher, Caramete, Ana, Carbone, Carmelita, Carroll, Sean, Chatterjee, Suchetana, Chen, Xingang, Church, Sarah, Chuss, David, Contaldi, Carlo, Cooray, Asantha, Creminelli, Paolo, Das, Sudeep, de Bernardis, Francesco, de Bernardis, Paolo, Delabrouille, Jacques, Dsert, F. Xavier, Devlin, Mark, Dickinson, Clive, Dicker, Simon, DiPirro, Michael, Dobbs, Matt, Dore, Olivier, Dotson, Jessie, Dunkley, Joanna, Dvorklin, Cora, Eriksen, Hans Kristian, Falvella, Maria Christiana, Finley, Dave, Finkbeiner, Douglas, Fixen, Dale, Flauger, Raphael, Fosalba, Pablo, Fowler, Joseph, Galli, Silvia, Gates, Evalyn, Gear, Walter Kieran, Giraud-Heraud, Yannick, Gorski, Krzysztof, Greene, Brian, Gruppuso, Alessandro, Gundersen, Josh, Halpern, Mark, Hirata, Christopher, Hivon, Eric, Holman, Richard, Holmes, Warren, Hu, Wayne, Hubmayr, Johannes, Huffenberger, Kevin, Hui, Howard, Hui, Lam, Irwin, Kent, Jackson, Mark, Jaffe, Andrew, Johnson, Bradley, Johnson, Dean, Jones, William, Kachru, Shamit, Kadota, Kenji, Kaplan, Jean, Kaplinghat, Manoj, Keating, Brian, Keskitalo, Reijo, Khoury, Justin, Kinney, Will, Kisner, Theodore, Knox, Lloyd, Kodama, Hideo, Kogut, Alan, Komatsu, Eiichiro, Kosowsky, Reijo, Kurki-Suonio, Hannu, Lamarre, Jean-Michel, Landau, Susana, Leach, Samuel, Leblond, Louis, Lee, Adrian, Leitch, Erik, Leonardi, Rodrigo, Lesgourgues, Julien, Liddle, Andrew, Lim, Eugene, Limon, Michele, Loverde, Marilena, Lubin, Philip, Lunghi, Enrico, Lykken, Joseph, MacTavish, Carolyn, Magalhaes, Antonio, Maino, Davide, Martin, Victoria, Matarrese, Sabino, Mather, John, Mathur, Harsh, Matsumura, Tomotake, Meerburg, Pieter, Melchiorri, Alessandro, Mersini-Houghton, Laura, Miller, Amber, Milligan, Michael, Moodley, Kavilan, Neimack, Michael, Nguyen, Hogan, Nicolis, Alberto, O'Dwyer, Ian, Olinto, Angela, Pagano, Luca, Pajer, Enrico, Partridge, Bruce, Pearson, Timothy, Peiris, Hiranya, Peloso, Marco, Piacentini, Francesco, Piat, Michel, Piccirillo, Lucio, Pierpaoli, Elena, Pietrobon, Davide, Pisano, Giampaolo, Pogosian, Levon, Pogosyan, Dmitri, Ponthieu, Nicolas, Popa, Lucia, Pryke, Clement, Raeth, Christoph, Ray, Subharthi, Reichardt, Christian, Ricciardi, Sara, Richards, Paul, Riotto, Antonio, Rocha, Graca, Ruhl, John, Rusholme, Benjamin, Scherrer, Robert, Scoccola, Claudia, Scott, Douglas, Sealfon, Carolyn, Sefusatti, Emiliano, Sehgal, Neelima, Seiffert, Michael, Serra, Paolo, Shandera, Sarah, Shimon, Meir, Shirron, Peter, Sievers, Jonathan, Silk, Joe, Sigurdson, Kris, Silverberg, Robert, Silverstein, Eva, Staggs, Suzanne, Starkman, Glenn, Stebbins, Albert, Stivoli, Frederico, Stompor, Radek, Sugiyama, Naoshi, Swetz, Daniel, Tartari, Andrea, Tegmark, Max, Timbie, Peter, Titov, Maxim, Tristram, Matthieu, Trodden, Mark, Tucker, Gregory, Urrestilla, Jon, Veneziani, Marcella, Verde, Licia, Vieira, Joaquin, Walker, Terry, Wands, David, Watson, Scott, Weinberg, Steven, Weiss, Rainer, Wandelt, Benjamin, Winstein, Bruce, Wollack, Edward, Wyman, Mark, Yadav, Amit, Won Yoon, Ki, Zahn, Olivier, Zaldarriage, Mattias, Zemcov, Michael, and Zwart, Jonathan
- Abstract
Modern cosmology has sharpened questions posed for millennia about the origin of our cosmic habitat. The age-old questions have been transformed into two pressing issues primed for attack in the coming decade: • How did the Universe begin? The current cosmological paradigm successfully explains how the majestic structure observed in the Universe today grew out of small ripples in the density of matter. What is the physical origin of the primordial seeds which are ultimately responsible for the existence of galaxies, stars, planets, and people in the Universe? It is natural to expect (and many theories predict) that whatever produced the density ripples also produced gravity waves – undulations in the fabric of space-time which travel at the speed of light. Does the Universe contain a spectrum of primordial gravity waves produced by the same mechanism which produced the ripples in the density? • What physical laws govern the Universe at the highest energies? All explanations for the seeds of structure rely on physics at energies far beyond those probed by, e.g., CERN’s Large Hadron Collider. Experiments probing these seeds therefore may provide information about new particles, forces, or perhaps even extra dimensions of space that are visible only at the highest energies. The clearest window onto these questions is the pattern of polarization in the Cosmic Microwave Background (CMB), which is uniquely sensitive to primordial gravity waves. A detection of the special pattern produced by gravity waves would be not only an unprecedented discovery, but also a direct probe of physics at the earliest observable instants of our Universe. Experiments which map CMB polarization over the coming decade will lead us on our first steps towards answering these age-old questions.
166. Planck-suppressed operators
- Author
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McAllister, Liam [Department of Physics, Cornell University, Ithaca, NY 14853 (United States)]
- Published
- 2014
- Full Text
- View/download PDF
167. Effects of Compactification in D-brane Inflation
- Author
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McAllister, Liam [Department of Physics, Cornell University, Ithaca, New York 14853 (United States)]
- Published
- 2010
- Full Text
- View/download PDF
168. Towards an explicit model of D-brane inflation
- Author
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McAllister, Liam [Department of Physics, Princeton University, Princeton, NJ 08544 (United States)]
- Published
- 2008
- Full Text
- View/download PDF
169. A microscopic limit on gravitational waves from D-brane inflation
- Author
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McAllister, Liam [Department of Physics, Princeton University, Princeton, New Jersey 08544 (United States)]
- Published
- 2007
- Full Text
- View/download PDF
170. CERN Winter School on Supergravity, Strings, and Gauge Theory 2010
- Author
-
McAllister, Liam
- Published
- 2010
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