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Physical Review Letters 2008

Enero 2008


Effects of Inelastic Neutrino-Nucleus Scattering on Supernova
Dynamics and Radiated Neutrino Spectra
K. Langanke, G. Martínez-Pinedo, B. Müller, H.-Th. Janka, A. Marek,
W. R. Hix, A. Juodagalvis, and J. M. Sampaio
Published 3 January 2008
011101   Abstract    Full Text: [ PDF (173 kB)  GZipped PS   ]   
Order


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Abundant Stable Gauge Field Hair for Black Holes in Anti~Vde Sitter
Space
J. E. Baxter, Marc Helbling, and Elizabeth Winstanley
Published 8 January 2008
011301   Abstract    Full Text: [ PDF (448 kB)  GZipped PS   ]   
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Essay: Physical Review Letters; Sam Goudsmit's Vision
Published 18 January 2008
020001   Abstract    Full Text: [ PDF (161 kB)  GZipped PS   ]   


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Flavor Evolution of the Neutronization Neutrino Burst From an O-Ne-Mg
Core-Collapse Supernova
Huaiyu Duan, George M. Fuller, J. Carlson, and Yong-Zhong Qian
Published 18 January 2008
021101   Abstract    Full Text: [ PDF (228 kB)  GZipped PS   ]   
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Lorentz Violation for Photons and Ultrahigh-Energy Cosmic Rays
Matteo Galaverni and Günter Sigl
Published 18 January 2008
021102   Abstract    Full Text: [ PDF (171 kB)  GZipped PS   ]   
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Fitting Cosmic Microwave Background Data with Cosmic Strings and
Inflation
Neil Bevis, Mark Hindmarsh, Martin Kunz, and Jon Urrestilla
Published 14 January 2008
021301   Abstract    Full Text: [ PDF (273 kB)  GZipped PS   ]   
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Simultaneous Solution to Dark Matter and Flavor Problems of
Supersymmetry
Jonathan L. Feng, Bryan T. Smith, and Fumihiro Takayama
Published 15 January 2008
021302   Abstract    Full Text: [ PDF (299 kB)  GZipped PS   ]   
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First Results from the XENON10 Dark Matter Experiment at the Gran
Sasso National Laboratory
J. Angle et al. (XENON Collaboration)
Published 17 January 2008
021303   Abstract    Full Text: [ PDF (1331 kB)  GZipped PS   ]   
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Information Theory, Spectral Geometry, and Quantum Gravity
Achim Kempf and Robert Martin
Published 18 January 2008
021304   Abstract    Full Text: [ PDF (94 kB)  GZipped PS   ]   
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Atom-Interferometry Tests of the Isotropy of Post-Newtonian Gravity
Holger Müller, Sheng-wey Chiow, Sven Herrmann, Steven Chu, and
Keng-Yeow Chung
Published 22 January 2008
031101   Abstract    Full Text: [ PDF (741 kB)  GZipped PS   ]   
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Lower Limit to the Scale of an Effective Quantum Theory of
Gravitation
R. R. Caldwell and Daniel Grin
Published 22 January 2008
031301   Abstract    Full Text: [ PDF (138 kB)  GZipped PS   ]   
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Necessity of Dark Matter in Modified Newtonian Dynamics within
Galactic Scales
Ignacio Ferreras, Mairi Sakellariadou, and Muhammad Furqaan Yusaf
Published 25 January 2008
031302   Abstract    Full Text: [ PDF (240 kB)  GZipped PS   ]   
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Elementary Particles and Fields 
[ Previous / Next Subject | Issue Index | Top / Bottom of Page]

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Probing the Geometry of Warped String Compactifications at the Large
Hadron Collider
Gary Shiu, Bret Underwood, Kathryn M. Zurek, and Devin G. E. Walker
Published 22 January 2008
031601   Abstract    Full Text: [ PDF (242 kB)  GZipped PS   ]   
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Astrophysical Bounds on Photons Escaping into Extra Dimensions
A. Friedland and M. Giannotti
Published 23 January 2008
031602   Abstract    Full Text: [ PDF (111 kB)  GZipped PS   ]   
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Test of the Equivalence Principle Using a Rotating Torsion Balance
S. Schlamminger, K.-Y. Choi, T. A. Wagner, J. H. Gundlach, and E. G.
Adelberger
Published 28 January 2008
041101   Abstract    Full Text: [ PDF (381 kB)  GZipped PS   ]   
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Probing White Dwarf Interiors with LISA: Periastron Precession in
Eccentric Double White Dwarfs
B. Willems, A. Vecchio, and V. Kalogera
Published 29 January 2008
041102   Abstract    Full Text: [ PDF (125 kB)  GZipped PS   ]   
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Anthropic Arguments and the Cosmological Constant, with and without
the Assumption of Typicality
Irit Maor, Lawrence Krauss, and Glenn Starkman
Published 28 January 2008
041301   Abstract    Full Text: [ PDF (102 kB)  GZipped PS   ]   
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Lattice Calculation of Non-Gaussian Density Perturbations from the
Massless Preheating Inflationary Model
Alex Chambers and Arttu Rajantie
Published 28 January 2008
041302   Abstract    Full Text: [ PDF (134 kB)  GZipped PS   ]   
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Possibility of Observing Dark Matter via the Gyromagnetic Faraday
Effect
Susan Gardner
Published 29 January 2008
041303   Abstract    Full Text: [ PDF (109 kB)  GZipped PS   ]   
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How Cold Is Cold Dark Matter? Small-Scales Constraints from the Flux
Power Spectrum of the High-Redshift Lyman-[IMAGE] Forest
Matteo Viel, George D. Becker, James S. Bolton, Martin G. Haehnelt,
Michael Rauch, and Wallace L. W. Sargent
Published 29 January 2008
041304   Abstract    Full Text: [ PDF (131 kB)  GZipped PS   ]   
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Febrero 2008


Dark Matter and the First Stars: A New Phase of Stellar
Evolution Douglas Spolyar, Katherine Freese, and Paolo Gondolo
Published 4 February 2008
051101   Abstract    Full Text: [ PDF (209 kB)  GZipped PS   ]   
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Gamma-Ray Spectrum from Gravitino Dark Matter Decay
Alejandro Ibarra and David Tran
Published 13 February 2008
061301   Abstract    Full Text: [ PDF (129 kB)  GZipped PS   ]   
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Essay: The Tau Lepton and Thirty Years of Changes in Elementary
Particle Physics Research
Published 22 February 2008
070001   Abstract    Full Text: [ PDF (208 kB)  GZipped PS   ]   

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Nonlinear Evolution of Anisotropic Cosmological Power
Shin'ichiro Ando and Marc Kamionkowski
Published 21 February 2008
071301   Abstract    Full Text: [ PDF (140 kB)  GZipped PS   ]   
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Scaling Solution for Small Cosmic String Loops
Jorge V. Rocha
Published 21 February 2008
071601   Abstract    Full Text: [ PDF (95 kB)  GZipped PS   ]   
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Stability of Precessing Superfluid Neutron Stars
K. Glampedakis, N. Andersson, and D. I. Jones
Published 26 February 2008
081101   Abstract    Full Text: [ PDF (149 kB)  GZipped PS   ]   
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Deformations of the Constraint Algebra of Ashtekar's Hamiltonian
Formulation of General Relativity
Kirill Krasnov
Published 27 February 2008
081102   Abstract    Full Text: [ PDF (99 kB)  GZipped PS   ]   
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Nonlinear Growth of Firehose and Mirror Fluctuations in Astrophysical
Plasmas
A. A. Schekochihin, S. C. Cowley, R. M. Kulsrud, M. S. Rosin, and T.
Heinemann
Published 29 February 2008
081301   Abstract    Full Text: [ PDF (156 kB)  GZipped PS   ]   
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Marzo 2008


Kerr Black Holes Are Not Unique to General Relativity
Dimitrios Psaltis, Delphine Perrodin, Keith R. Dienes, and Irina
Mocioiu
Published 3 March 2008
091101   Abstract    Full Text: [ PDF (94 kB)  GZipped PS   ]   
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Anomalous Orbital-Energy Changes Observed during Spacecraft Flybys of
Earth
John D. Anderson, James K. Campbell, John E. Ekelund, Jordan Ellis,
and James F. Jordan
Published 3 March 2008
091102   Abstract    Full Text: [ PDF (236 kB)  GZipped PS   ]   
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Tabletop Creation of Entangled Multi-keV Photon Pairs and the Unruh
Effect
Ralf Schützhold, Gernot Schaller, and Dietrich Habs
Published 3 March 2008
091301   Abstract    Full Text: [ PDF (149 kB)  GZipped PS   ]   
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Cosmic (Super)String Constraints from 21 cm Radiation
Rishi Khatri and Benjamin D. Wandelt
Published 4 March 2008
091302   Abstract    Full Text: [ PDF (246 kB)  GZipped PS   ]   
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Baryon Acoustic Oscillation Intensity Mapping of Dark Energy
Tzu-Ching Chang, Ue-Li Pen, Jeffrey B. Peterson, and Patrick McDonald
Published 5 March 2008
091303   Abstract    Full Text: [ PDF (224 kB)  GZipped PS   ]   
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Planckian Birth of a Quantum de Sitter Universe
J. Ambjørn, A. Görlich, J. Jurkiewicz, and R. Loll
Published 7 March 2008
091304   Abstract    Full Text: [ PDF (154 kB)  GZipped PS   ]   
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[IMAGE]First Observation of the Greisen-Zatsepin-Kuzmin Suppression
R. U. Abbasi et al. (High Resolution Fly's Eye Collaboration)
Published 10 March 2008
101101   Abstract    Full Text: [ PDF (192 kB)  GZipped PS   ]   
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Fractal Threshold Behavior in Vacuum Gravitational Collapse
Sebastian J. Szybka and Tadeusz Chmaj
Published 12 March 2008
101102   Abstract    Full Text: [ PDF (333 kB)  GZipped PS   ]   
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Does the Planck Mass Run on the Cosmological-Horizon Scale?
Georg Robbers, Niayesh Afshordi, and Michael Doran
Published 18 March 2008
111101   Abstract    Full Text: [ PDF (126 kB)  GZipped PS   ]   
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Constraints on Torsion from Bounds on Lorentz Violation
V. Alan Kostelecký, Neil Russell, and Jay D. Tasson
Published 20 March 2008
111102   Abstract    Full Text: [ PDF (92 kB)  GZipped PS   ]   
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Weak Cosmic Censorship: As Strong as Ever
Shahar Hod
Published 26 March 2008
121101   Abstract    Full Text: [ PDF (101 kB)  GZipped PS   ]   
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General Nonextremal Rotating Charged Gödel Black Holes in Minimal
Five-Dimensional Gauged Supergravity
Shuang-Qing Wu
Published 24 March 2008
121301   Abstract    Full Text: [ PDF (103 kB)  GZipped PS   ]   
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Relativistic Photon Mediated Shocks
Amir Levinson and Omer Bromberg
Published 31 March 2008
131101   Abstract    Full Text: [ PDF (215 kB)  GZipped PS   ]   
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Abril 2008


Signatures of Gravitational Fixed Points at the Large Hadron Collider
Daniel F. Litim and Tilman Plehn
Published 1 April 2008
131301   Abstract    Full Text: [ PDF (262 kB)  GZipped PS   ]   
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Nearly Scale Invariant Spectrum of Gravitational Radiation from
Global Phase Transitions
Katherine Jones-Smith, Lawrence M. Krauss, and Harsh Mathur
Published 2 April 2008
131302   Abstract    Full Text: [ PDF (139 kB)  GZipped PS   ]   
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[IMAGE]Physical Interpretation of the Spectrum of Black Hole
Quasinormal Modes Michele Maggiore
Published 8 April 2008
141301   Abstract    Full Text: [ PDF (138 kB)  GZipped PS   ]   
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Binary~VBlack-Hole Merger: Symmetry and the Spin Expansion
Latham Boyle, Michael Kesden, and Samaya Nissanke
Published 17 April 2008
151101   Abstract    Full Text: [ PDF (259 kB)  GZipped PS   ]   
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Universal Charge-Radius Relation for Subatomic and Astrophysical
Compact Objects
Jes Madsen
Published 17 April 2008
151102   Abstract    Full Text: [ PDF (115 kB)  GZipped PS   ]   

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Far-from-Constant Mean Curvature Solutions of Einstein's Constraint
Equations with Positive Yamabe Metrics
M. Holst, G. Nagy, and G. Tsogtgerel
Published 23 April 2008
161101   Abstract    Full Text: [ PDF (118 kB)  GZipped PS   ]   
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Possibility of Precise Measurement of the Cosmological Power Spectrum
with a Dedicated Survey of 21 cm Emission after Reionization
Abraham Loeb and J. Stuart B. Wyithe
Published 22 April 2008
161301   Abstract    Full Text: [ PDF (204 kB)  GZipped PS   ]   
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Quantum Bounce and Cosmic Recall
Alejandro Corichi and Parampreet Singh
Published 23 April 2008
161302   Abstract    Full Text: [ PDF (102 kB)  GZipped PS   ]   
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Analysis of Rotation Curves in the Framework of the Gravitational
Suppression Model
Christiane Frigerio Martins and Paolo Salucci
Published 12 April 2007
151301   Abstract    Full Text: [ PDF (666 kB)  GZipped PS   ]   
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Mayo 2008


Complete Analytic Solution of the Geodesic Equation in
Schwarzschild~V(Anti-)de Sitter Spacetimes
Eva Hackmann and Claus Lämmerzahl
Published 2 May 2008
171101   Abstract    Full Text: [ PDF (201 kB)  GZipped PS   ]   
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Late Time Behavior of False Vacuum Decay: Possible Implications for
Cosmology and Metastable Inflating States
Lawrence M. Krauss and James Dent
Published 30 April 2008
171301   Abstract    Full Text: [ PDF (88 kB)  GZipped PS   ]   
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Non-Gaussianities in New Ekpyrotic Cosmology
Evgeny I. Buchbinder, Justin Khoury, and Burt A. Ovrut
Published 2 May 2008
171302   Abstract    Full Text: [ PDF (107 kB)  GZipped PS   ]   
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Evidence of Primordial Non-Gaussianity (fNL) in the Wilkinson
Microwave Anisotropy Probe 3-Year Data at 2.8[IMAGE]
Amit P. S. Yadav and Benjamin D. Wandelt
Published 7 May 2008
181301   Abstract    Full Text: [ PDF (170 kB)  GZipped PS   ]   
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No-Boundary Measure of the Universe
James B. Hartle, S. W. Hawking, and Thomas Hertog
Published 23 May 2008
201301   Abstract    Full Text: [ PDF (140 kB)  GZipped PS   ]    Order

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June 2008

How Quantum is the Big Bang?
Martin Bojowald
Published 3 June 2008
221301   Abstract    Full Text: [ PDF (102 kB)  GZipped PS   ]    Order

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Magnetic Field Production during Preheating at the Electroweak Scale
Andrés Díaz-Gil, Juan García-Bellido, Margarita García Pérez, and Antonio
González-Arroyo
Published 16 June 2008
241301   Abstract    Full Text: [ PDF (428 kB)  GZipped PS   ]    Order


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Beyond Two Dark Energy Parameters
Devdeep Sarkar, Scott Sullivan, Shahab Joudaki, Alexandre Amblard, Daniel
E. Holz, and Asantha Cooray
Published 19 June 2008
241302   Abstract    Full Text: [ PDF (121 kB)  GZipped PS   ]    Order

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Relativistic Closed-Form Hamiltonian for Many-Body Gravitating
Systems in the Post-Minkowskian Approximation
Tomáš Ledvinka, Gerhard Schäfer, and JiÅ~Yí BiÄ~Mák
Published 23 June 2008
251101   Abstract    Full Text: [ PDF (111 kB)  GZipped PS   ]
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Hierarchies from D-brane Instantons in Globally Defined Calabi-Yau
Orientifolds
Mirjam CvetiÄ~M and Timo Weigand
Published 24 June 2008
251601   Abstract    Full Text: [ PDF (110 kB)  GZipped PS   ]
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Wrapped Branes as Qubits
L. Borsten, D. Dahanayake, M. J. Duff, H. Ebrahim, and W. Rubens
Published 25 June 2008
251602   Abstract    Full Text: [ PDF (88 kB)  GZipped PS   ]
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Cascading Gravity: Extending the Dvali-Gabadadze-Porrati Model to
Higher Dimension
Claudia de Rham, Gia Dvali, Stefan Hofmann, Justin Khoury, Oriol
Pujolàs, Michele Redi, and Andrew J. Tolley
Published 27 June 2008
251603   Abstract    Full Text: [ PDF (106 kB)  GZipped PS   ]
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Search for Large Extra Dimensions via Single Photon plus Missing
Energy Final States at [IMAGE]=1.96 TeV
V. M. Abazov et al. (D0 Collaboration)
Published 30 June 2008
011601   Abstract    Full Text: [ PDF (224 kB)  GZipped PS   ]   
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July 2008

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A General Test of the Copernican Principle
Chris Clarkson, Bruce Bassett, and Teresa Hui-Ching Lu
Published 2 July 2008
011301   Abstract    Full Text: [ PDF (93 kB)  GZipped PS   ]   
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Elementary Particles and Fields 
[ Previous / Next Subject | Issue Index | Top / Bottom of Page]


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Analytical Characterization of Oscillon Energy and Lifetime
Marcelo Gleiser and David Sicilia
Published 3 July 2008
011602   Abstract    Full Text: [ PDF (214 kB)  GZipped PS   ]   
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Strong CP Problem with 1032 Standard Model Copies
Gia Dvali and Glennys R. Farrar
Published 1 July 2008
011801   Abstract    Full Text: [ PDF (97 kB)  GZipped PS   ]   
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Volume 101, Issue 3,

Bjorken Flow from an Anti~Vde Sitter Space Schwarzschild Black Hole
James Alsup and George Siopsis
Published 18 July 2008
031602   Abstract    Full Text: [ PDF (112 kB)  GZipped PS   ]   
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Volume 101, Issue 4 

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Brightening of an Accretion Disk due to Viscous Dissipation of
Gravitational Waves during the Coalescence of Supermassive Black
Holes
Bence Kocsis and Abraham Loeb
Published 25 July 2008
041101   Abstract    Full Text: [ PDF (209 kB)  GZipped PS   ]   
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Eötvös Bounds on Couplings of Fundamental Parameters to Gravity
Thomas Dent
Published 25 July 2008
041102   Abstract    Full Text: [ PDF (118 kB)  GZipped PS   ] Order
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Membranes on an Orbifold
Neil Lambert and David Tong
Published 25 July 2008
041602   Abstract    Full Text: [ PDF (102 kB)  GZipped PS   ]   
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Observation of the Suppression of the Flux of Cosmic Rays above
4×1019 eV
J. Abraham et al. (Pierre Auger Collaboration)
Published 4 August 2008
061101   Abstract    Full Text: [ PDF (246 kB)  GZipped PS   ]   
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See accompanying Viewpoint Physics 1, 9 (2008)

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Binary-Black-Hole Encounters, Gravitational Bursts, and Maximum Final
Spin
Matthew C. Washik, James Healy, Frank Herrmann, Ian Hinder, Deirdre
M. Shoemaker, Pablo Laguna, and Richard A. Matzner
Published 5 August 2008
061102   Abstract    Full Text: [ PDF (323 kB)  GZipped PS   ]   
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Singularity Problem with f(R) Models for Dark Energy
Andrei V. Frolov
Published 7 August 2008
061103   Abstract    Full Text: [ PDF (161 kB)  GZipped PS   ]   
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Primordial Fluctuations and Non-Gaussianities in Multifield
Dirac-Born-Infeld Inflation
David Langlois, Sébastien Renaux-Petel, Danièle A. Steer, and
Takahiro Tanaka
Published 7 August 2008
061301   Abstract    Full Text: [ PDF (110 kB)  GZipped PS   ]   

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Gravity Duals for Nonrelativistic Conformal Field Theories
Koushik Balasubramanian and John McGreevy
Published 4 August 2008
061601   Abstract    Full Text: [ PDF (103 kB)  GZipped PS   ]   
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See accompanying Viewpoint Physics 1, 10 (2008)

 

http://xxx.lanl.gov/abs/0712.0486

Halos of Unified Dark Matter Scalar Field

Authors: Daniele Bertacca, Nicola Bartolo, Sabino Matarrese (Physics Dept. and INFN, Padova, ITALY)
(Submitted on 4 Dec 2007)
Abstract: We investigate the static and spherically symmetric solutions of Einstein's equations for a scalar field with non-canonical kinetic term, assumed to provide both the dark matter and dark energy components of the Universe. In particular, we give a prescription to obtain solutions (dark halos) whose rotation curve v_c(r) is in good agreement with observational data. We show that there exist suitable scalar field Lagrangians that allow to describe the cosmological background evolution and the static solutions with a single dark fluid.
Comments: 19 pages LaTeX file
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:0712.0486v1 [astro-ph]

Submission history
From: Sabino Matarrese [view email]


Astrophysics, abstract
astro-ph/0608681
From: Dragan Huterer [view email]
Date (v1): Thu, 31 Aug 2006 18:05:22 GMT (97kb)
Date (revised v2): Wed, 31 Jan 2007 20:50:52 GMT (97kb)

Separating Dark Physics from Physical Darkness: Minimalist Modified Gravity vs. Dark Energy


Authors: Dragan Huterer (KICP Chicago), Eric V. Linder (Lawrence Berkeley Lab)

Comments: 9 pages, 4 figures, matches the PRD published version
Journal-ref: Phys.Rev. D75 (2007) 023519

The acceleration of the cosmic expansion may be due to a new component of physical energy density or a modification of physics itself. Mapping the expansion of cosmic scales and the growth of large scale structure in tandem can provide insights to distinguish between the two origins. Using Minimal Modified Gravity (MMG) - a single parameter gravitational growth index formalism to parameterize modified gravity theories - we examine the constraints that cosmological data can place on the nature of the new physics. For next generation measurements combining weak lensing, supernovae distances, and the cosmic microwave background we can extend the reach of physics to allow for fitting gravity simultaneously with the expansion equation of state, diluting the equation of state estimation by less than 25% relative to when general relativity is assumed, and determining the growth index to 8%. For weak lensing we examine the level of understanding needed of quasi- and nonlinear structure formation in modified gravity theories, and the trade off between stronger precision but greater susceptibility to bias as progressively more nonlinear information is used.

 

Astrophysics, abstract
astro-ph/0702015
From: Zong-Kuan Guo [view email]
Date (v1): Thu, 1 Feb 2007 03:17:17 GMT (136kb)
Date (revised v2): Tue, 6 Feb 2007 13:24:20 GMT (136kb)

Probing the Coupling between Dark Components of the Universe

Authors: Zong-Kuan Guo, Nobuyoshi Ohta, Shinji Tsujikawa

Comments: 8 pages, 7 figures, RevTeX, references added
Report-no: KU-TP 012

We place observational constraints on a coupling between dark energy and dark matter by using 71 Type Ia supernovae (SNe Ia) from the first year of the five-year Supernova Legacy Survey (SNLS), the cosmic microwave background (CMB) shift parameter from the three-year Wilkinson Microwave Anisotropy Probe (WMAP), and the baryon acoustic oscillation (BAO) peak found in the Sloan Digital Sky Survey (SDSS). The interactions we study are (i) constant coupling delta and (ii) varying coupling delta(z) that depends on a redshift z, both of which have simple parametrizations of the Hubble parameter to confront with observational data. We find that the combination of the three databases marginalized over a present dark energy density gives stringent constraints on the coupling, -0.08 < delta < 0.03 (95% CL) in the constant coupling model and -0.4 < delta_0 < 0.1 (95% CL) in the varying coupling model, where delta_0 is a present value. The uncoupled LambdaCDM model (w_X = -1 and delta = 0) still remains a good fit to the data, but the negative coupling (delta < 0) with a phantom equation of state of dark energy (w_X < -1) is slightly favoured over the LambdaCDM model.


High Energy Physics - Theory, abstract

hep-th/0702001
From: Robert Brandenberger [view email]
Date: Wed, 31 Jan 2007 21:42:14 GMT (53kb)

String Gas Cosmology and Structure Formation - A Brief Review

Authors: Robert Brandenberger

Comments: Invited talk at CosPA 2006, Nov. 15 - 17, 2006, National Taiwan University, Taipei, to be publ. in the proceedings, 11 pages, 3 figures

For suitable cosmological backgrounds, thermal fluctuations of a gas of strings can generate a scale-invariant spectrum of cosmological fluctuations without requiring a phase of inflationary expansion. We highlight the key points of this mechanism, and discuss cosmological backgrounds in which this scenario can be realized. The spectrum of cosmological perturbations has a small red tilt (like in scalar field-driven inflation) but (unlike in inflation) there is a small blue tilt of the spectrum of gravitational waves.

Astrophysics, abstract
astro-ph/0511628
From: R. G. Vishwakarma [view email]
Date (v1): Mon, 21 Nov 2005 20:03:33 GMT (10kb)
Date (revised v2): Thu, 1 Dec 2005 01:01:12 GMT (12kb)
Date (revised v3): Thu, 1 Feb 2007 21:32:31 GMT (13kb)

Recent Supernovae Ia observations tend to rule out all the cosmologies?

Authors: R. G. Vishwakarma (Zacatecas University)

Comments: Replaced with accepted version

Dark energy and the accelerated expansion of the universe have been the direct predictions of the distant supernovae Ia observations which are also supported, indirectly, by the observations of the CMB anisotropies, gravitational lensing and the studies of galaxy clusters. Today these results are accommodated in what has become the `concordance cosmology': a universe with flat spatial sections t=constant with about 70% of its energy in the form of Einstein's cosmological constant \Lambda.
However, we find that as more and more supernovae Ia are observed, more accurately and towards higher redshift, the probability that the data are well explained by the cosmological models decreases alarmingly, finally ruling out the concordance model at more than 95% confidence level. This raises doubts against the `standard candle'-hypothesis of the supernovae Ia and their use to constrain the cosmological models. We need a better understanding of the entire SN Ia phenomenon in order to have cosmological consequences from them.

 

Astrophysics, abstract
astro-ph/0511763
From: William Komp [view email]
Date (v1): Mon, 28 Nov 2005 15:38:36 GMT (178kb)
Date (revised v2): Thu, 1 Feb 2007 22:02:33 GMT (800kb)

Do Type-Ia Supernovae Constrain the Total Equation of State?

Authors: William Komp

Comments: version 2, 21 pages, 7 figures, 3 tables, submitted to Prd

In this paper, we consider a couple of alternative dark energy models using the total equation of state of the cosmological fluid, $\wt$. These models are fit to the recent type-Ia supernovae data and are compared to previously considered models. The first model is based on the hyperbolic tangent and provides a good estimate of the rate of the transition to dark energy domination. The second model is a cubic spline model. This model demonstrates and quantifies the non-monotonicity in the total equation of state coming from the supernovae observations. At present, the supernovae observations indicate significance to non-monotonically decreasing dark energy. We derive constraints on the spline paramters and compare and constrast the results to the Cosmological Constant dark energy model. Both the hyperbolic and splines models indicate that a precise physical notion of dark enegy is a potentially ever more mysterious quantity?



Astrophysics, abstract
astro-ph/0701692
From: Lawrence M. Krauss [view email]
Date: Wed, 24 Jan 2007 15:22:39 GMT (58kb)

Dark Energy, A Cosmological Constant, and Type Ia Supernovae

Authors: Lawrence M. Krauss, Katherine Jones-Smith (CERCA, Case Western Reserve University), Dragan Huterer (KICP, University of Chicago)

Comments: 8 pages, submitted to New Journal of Physics

We focus on uncertainties in supernova measurements, in particular of individual magnitudes and redshifts, to review to what extent supernovae measurements of the expansion history of the universe are likely to allow us to constrain a possibly redshift-dependent equation of state of dark energy, $w(z)$. focus in particular on the central question of how well one might rule out the possibility of a cosmological constant $w=-1$. We argue that it is unlikely that we will be able to significantly reduce the uncertainty in the determination of $w$ beyond its present bounds, without significant improvements in our ability to measure the cosmic distance scale as a function of redshift. Thus, unless the dark energy significantly deviates from $w(z)=-1$ at some redshift, very stringent control of the statistical and systematic errors will be necessary to have a realistic hope of empirically distinguishing exotic dark energy from a cosmological constant.

 

Astrophysics, abstract
astro-ph/0702002
From: Niayesh Afshordi [view email]
Date: Thu, 1 Feb 2007 19:50:04 GMT (74kb)

Cuscuton Cosmology: Dark Energy meets Modified Gravity

Authors: Niayesh Afshordi (ITC, Harvard), Daniel J.H. Chung (UW-Madison), Michael Doran (Heidelberg), Ghazal Geshnizjani (UW-Madison)

Comments: 10 pages, 5 figures, submitted to PRD

In a companion paper (hep-th/0609150), we have introduced a model of scalar field dark energy, Cuscuton, which can be realized as the incompressible (or infinite speed of sound) limit of a k-essence fluid. In this paper, we study how Cuscuton modifies the constraint sector of Einstein gravity. In particular, we study Cuscuton cosmology and show that even though Cuscuton can have an arbitrary equation of state, or time dependence, and is thus inhomogeneous; its perturbations do not introduce any additional dynamical degree of freedom and only satisfy a constraint equation, amounting to an effective modification of gravity on large scales. Therefore, Cuscuton can be considered to be a minimal theory of evolving dark energy, or a minimal modification of a cosmological constant, as it has no internal dynamics. Moreover, this is the only modification of Einstein gravity to our knowledge that does not introduce any additional degrees freedom. We then study two simple Cuscuton models, with quadratic and exponential potentials. The quadratic model has the exact same expansion history as LCDM, and yet contains an early dark energy component with constant energy fraction, which is constrained to < 2%, mainly from WMAP Cosmic Microwave Background (CMB) and SDSS Lyman-alpha forest observations. The exponential model has the same expansion history as the DGP self-accelerating braneworld model, but generates a much smaller Integrated Sachs-Wolfe (ISW) effect, and is thus consistent with the CMB observations. Finally, we show that the evolution is local on super-horizon scales, implying that there is no gross violation of causality, despite Cuscuton's infinite speed of sound.

 

Astrophysics, abstract
astro-ph/0702003
From: Federico Piazza [view email]
Date: Thu, 1 Feb 2007 20:09:58 GMT (213kb)

Measuring deviations from a cosmological constant: a field-space parameterization

Authors: Robert Crittenden, Elisabetta Majerotto, Federico Piazza

Comments: 5 pages, 6 figures

Most parameterizations of the dark energy equation of state do not reflect realistic underlying physical models. Here, we develop a relatively simple description of dark energy based on the dynamics of a scalar field which is exact in the limit that the equation of state approaches a cosmological constant, assuming some degree of smoothness of the potential. By introducing just two parameters defined in the configuration space of the field we are able to reproduce a wide class of quintessence models. We examine the observational constraints on these models as compared to linear evolution models, and show how priors in the field space translate into priors on observational parameters.

 

Astrophysics, abstract
astro-ph/0612642
From: Xin Zhang [view email]
Date (v1): Thu, 21 Dec 2006 14:07:16 GMT (56kb)
Date (revised v2): Sun, 4 Feb 2007 12:49:02 GMT (56kb)

Reconstructing generalized ghost condensate model with dynamical dark energy parametrizations and observational datasets


Authors: Jingfei Zhang, Xin Zhang, Hongya Liu

Comments: 8 pages, 3 figures; references added

Observations of high-redshift supernovae indicate that the universe is accelerating at the present stage, and we refer to the cause for this cosmic acceleration as ``dark energy''. In particular, the analysis of current data of type Ia supernovae (SNIa), cosmic large-scale structure (LSS), and the cosmic microwave background (CMB) anisotropy implies that, with some possibility, the equation-of-state parameter of dark energy may cross the cosmological-constant boundary ($w=-1$) during the recent evolution stage. The model of ``quintom'' has been proposed to describe this $w=-1$ crossing behavior for dark energy. As a single-real-scalar-field model of dark energy, the generalized ghost condensate model provides us with a successful mechanism for realizing the quintom-like behavior. In this paper, we reconstruct the generalized ghost condensate model in the light of three forms of parametrization for dynamical dark energy, with the best-fit results of up-to-date observational data.

 

General Relativity and Quantum Cosmology, abstract
gr-qc/0702030
From: Abhay Ashtekar [view email]
Date: Mon, 5 Feb 2007 22:26:44 GMT (56kb)
An Introduction to Loop Quantum Gravity Through Cosmology
Authors: Abhay Ashtekar
Comments: 20 pages, 4 figures, Introductory Review
Report-no: IGPG-07/01-02, NSF-KITP-07-05

This introductory review is addressed to beginning researchers. Some of the distinguishing features of loop quantum gravity are illustrated through loop quantum cosmology of FRW models. In particular, these examples illustrate: i) how `emergent time' can arise; ii) how the technical issue of solving the Hamiltonian constraint and constructing the \emph{physical} sector of the theory can be handled; iii) how questions central to the Planck scale physics can be answered using such a framework; and, iv) how quantum geometry effects can dramatically change physics near singularities and yet naturally turn themselves off and reproduce classical general relativity when space-time curvature is significantly weaker than the Planck scale.

 

0707.1678
From: A. Perez-Lorenzana [view email]
[v1] Wed, 11 Jul 2007 18:29:09 GMT (10kb)
Cosmological Scalar Fields Unification
Authors: Abdel Pérez-Lorenzana, Merced Montesinos, Tonatiuh Matos
(Submitted on 11 Jul 2007)

Abstract: We present a model where early inflation and late accelerating expansion of the Universe are driven by the real and imaginary parts of a single complex scalar field, which we identified as inflaton and phantom field, respectively. This inflaton-phantom unification is protected by an internal SO(1,1) symmetry, with the two cosmological scalars appearing as the degrees of freedom of a sole fundamental representation. The unification symmetry allows to build successful potentials. We observe that our theory provides a matter-phantom duality, which transforms scalar matter cosmological solutions into phantom solutions and vice versa. We also suggest that a complete unification of all scalar fields of cosmological interest is yet possible under a similar footing.

 

Good news about SNAP

BERKELEY, CA -- The National Research Council's Beyond 
Einstein Program Assessment Committee has recommended that the 
Joint Dark Energy Mission (JDEM), jointly supported by the 
National Aeronautics and Space Administration and the 
Department of Energy, be the first of NASA's Beyond Einstein 
cosmology missions to be developed and launched.

Read the note in:
http://www.lbl.gov/Science-Articles/Archive/Phys-JDEM.html

Subject: LAMBDA Announcement: WMAP Five Years of Data Released!
Dear colleagues:

We are pleased to announce that the 5-year WMAP data, along with 7 papers
describing the results, are now available on LAMBDA,

http://lambda.gsfc.nasa.gov/

Please forward this announcement to colleagues of yours whom you think may
be interested. Thank you very much - we look forward to seeing your
analyses of the data!

Sincerely,
Gary Hinshaw
NASA/GSFC
for the Legacy Archive for Microwave Background Data Analysis (LAMBDA)

See also: http://www.nasa.gov/topics/universe/features/wmap_five.html

Subject: No dark matter
No dark matter

http://www.interactions.org/cms/?pid=1025916

 

 


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Agosto 19, 2008 1:37 PM


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