No. | Authors | Title / PDF | Reference |
245/227 |
R. Liu, W. Hu, H. Xiao |
Warm and Fuzzy Dark Matter: Free Streaming of Wave Dark Matter |
Phys. Rev. D (submitted)
2406.12970 |
244/226 |
I. Holst, W. Hu, L. Jenks |
Dark Matter Isocurvature from Curvature |
Phys. Rev. D (submitted)
2311.17164 |
243/225 |
J.M. Ezquiaga, W. Hu, R.K.L. Lo |
Identifying Strongly Lensed Gravitational Waves through their Phase Consistency |
Phys. Rev. D (submitted)
2308.06616 |
242/224 |
D. Zegeye, T. Crawford, W. Hu |
Measuring mu-distortions from the Thermal Sunyaev-Zeldovich Effect |
Phys. Rev. D (submitted)
2305.09882 |
241/223 |
K. Inomata, H. Lee, W. Hu |
Synchronizing the Consistency Relation |
JCAP (submitted)
2304.10559 |
240/222 |
M.X. Lin, E. McDonough, J.C. Hill, W. Hu |
Dark Matter Trigger for Early Dark Energy Coincidence |
Phys. Rev. D (submitted)
2212.08098 |
239/221 |
L.F. Secco, T. Karwal, W. Hu, E. Krause |
The Role of the Hubble Scale in the Weak Lensing vs. CMB Tension |
PRD (submitted)
2209.12997 |
238/220 |
J.M. Ezquiaga, W. Hu, M. Lagos, M.X. Lin, F. Xu |
Modified gravitational wave propagation with higher modes and its degeneracies with lensing |
JCAP 08 33 (2022)
2203.13252 |
237/219 |
S. Passaglia, W. Hu |
Accurate effective fluid approximation for ultralight axions |
Phys. Rev. D 105 123529 (2022)
2201.10238 |
236/218 |
E. McDonough, M.X. Lin, J.C. Hill, W. Hu, S. Zhou |
Early dark sector, the Hubble tension, and the swampland |
Phys. Rev. D 106 043525 (2022)
2112.09128 |
235/217 |
D. Zegeye, K. Inomata, W. Hu |
Spectral Distortion Anisotropy from Inflation for Primordial Black Holes |
Phys. Rev. D 105 103535 (2022)
2112.05190 |
234/216 |
K. Inomata, E. McDonough, W. Hu |
Amplification of primordial perturbations from the rise or fall of the inflaton |
JCAP 02 031 (2022)
2110.14641 |
233/215 |
J.M. Ezquiaga, W. Hu, M. Lagos, M.X. Lin |
Gravitational Wave Propagation beyond General Relativity: Waveform Distortions and Echoes |
JCAP 11 048 (2021)
2108.10872 |
232/214 |
S. Passaglia, W. Hu, A.J. Long, D. Zegeye |
The Secret Higgstory of the Highest Temperature during Reheating |
Phys. Rev. D 104 083540 (2021)
2108.00962 |
231/213 |
C. Heinrich, W. Hu |
Reionization Effective Likelihood from Planck 2018 Data |
Phys. Rev. D 104 063505 (2021)
2104.13998 |
230/212 |
K. Inomata, E. McDonough, W. Hu |
Primordial Black Holes Arise When the Inflaton Falls |
Phys. Rev. D 104 123553 (2021)
2104.03972 |
229/211 |
M.-X. Lin, W. Hu, M. Raveri |
Testing H0 in Acoustic Dark Energy with Planck and ACT Polarization |
Phys. Rev. D 102 123523 (2020)
2009.08974 |
228/210 |
J.M. Ezquiaga, D.E. Holz, W. Hu, M. Lagos, R.M. Wald |
Phase Effects from Strong Gravitational Lensing of Gravitational Waves |
Phys. Rev. D 103 064047 (2021)
2008.12814 |
227/209 |
J.M. Ezquiaga, W. Hu, M. Lagos |
Apparent Superluminality of Lensed Gravitational Waves |
Phys. Rev. D 102 023531 (2020)
2005.10702 |
226/208 |
W.L.K. Wu, P. Motloch, W. Hu, M. Raveri |
Hubble Constant Tension between CMB lensing and BAO measurements |
Phys. Rev. D 102 023510 (2020)
2004.10207 |
225/207 |
G. Benevento, W. Hu, M. Raveri |
Can Late Dark Energy Transitions Raise the Hubble Constant |
Phys. Rev. D 101 103517 (2020)
2002.11707 |
224/206 |
H. Motohashi, W. Hu |
Effective Field Theory of Degenerate Higher-Order Inflation |
Phys. Rev. D 101 083531 (2020)
2002.07967 |
223/205 |
P. Motloch, W. Hu |
Lensing-like Tensions in the Planck Lensing Release |
Phys. Rev. D 101 0083515 (2020)
1912.06601 |
222/204 |
M. Raveri, G. Zacharegkas, W. Hu |
Quantifying Concordance of Correlated Cosmological Data Sets |
Phys. Rev. D 101 103527 (2020)
1912.04880 |
221/203 |
S. Passaglia, W. Hu, H. Motohashi |
Primordial Black Holes as Dark Matter through Higgs Criticality |
Phys. Rev. D101 123523 (2020)
1912.02682 |
220/202 |
M. Lagos, M.X. Lin, W. Hu |
Curvature Perturbations in the Effective Field Theory of Inflation |
Phys. Rev D100 123507 (2019)
1908.08785 |
219/201 |
M.-X. Lin, G. Benevento, W. Hu, M. Raveri |
Acoustic Dark Energy: Potential Conversion of the Hubble Tension |
Phys. Rev. D 100 063542 (2019)
1905.12618 |
218/200 |
P. Li, S. Dodelson, W. Hu |
Distortions in the Surface of Last Scattering |
Phys. Rev. D 100 043502 (2019)
1905.03923 |
217/199 |
M. Raveri, W. Hu, S. Sethi |
Swampland Conjectures and Late-Time Cosmology |
Phys. Rev. D 99 083518 (2019)
1812.10448 |
216/198 |
S. Passaglia, W. Hu, M. Motohashi |
Primordial Black Holes and Local Non-Gaussianity in Canonical Inflation |
Phys. Rev. D 99 043536 (2019)
1812.08243 |
215/197 |
P. Motloch, W. Hu |
Lensing Covariance on Cut Sky and SPT-Planck Lensing Tensions |
Phys. Rev. D 99 023506 (2019)
1810.09347 |
214/196 |
M.-X. Lin, M. Raveri, W. Hu |
Phenomenology of Modified Gravity at Recombination |
Phys. Rev. D 99 043514 (2019)
1810.02333 |
213/195 |
M. Raveri, W. Hu |
Concordance and Discordance in Cosmology |
Phys. Rev. D 99 043506 (2019)
1806.04649 |
212/194 |
S. Passaglia, W. Hu |
Scalar Bispectrum Beyond Slow-Roll in the Unified EFT of Inflation |
Phys. Rev. D 98 023526 (2018)
1804.07741 |
211/193 |
P. Motloch, W. Hu |
Tensions between direct measurements of the lens power spectrum from Planck data |
Phys. Rev. D 97 103536 (2018)
1803.01858 |
210/192 |
G. Obied, C. Dvorkin, C. Heinrich, W. Hu, V. Miranda |
Inflationary vs Reionization Features from Planck 2015 Data |
Phys. Rev. D 98 043518 (2018)
1803.01858 |
209/191 |
H. Ramirez, S. Passaglia, H. Motohashi, W. Hu, O. Mena |
Reconciling tensor and scalar observables in G-inflation |
JCAP 04 039 (2018)
1802.04290 |
208/190 |
C. Heinrich, W. Hu |
Does Planck 2015 polarization favor high redshift reionization? |
Phys. Rev. D 98 063514 (2018)
1802.00791 |
207/189 |
A.J. Long, M. Raveri, W. Hu, S. Dodelson |
Neutrino Mass Priors for Cosmology from Random Matrices |
Phys. Rev. D 97 043510 (2018)
1711.08434 |
206/188 |
C.-T. Chiang, W. Hu, Y. Li, M. LoVerde |
Scale-dependent bias and bispectrum in neutrino separate universe simulations |
Phys. Rev. D. 97 123526 (2018)
1710.01310 |
205/187 |
M. Raveri, W. Hu, T. Hoffman, L.-T. Wang |
Partially Acoustic Dark Matter Cosmology and Cosmological Constraints |
Phys. Rev. D 96 103501 (2017)
1709.04877 |
204/186 |
P. Motloch, W. Hu |
Lens Covariance Effects on Likelihood Analyses of CMB Power Spectra |
Phys. Rev. D 96 103517 (2017)
1709.03599 |
203/185 |
G. Obied, C. Dvorkin, C. Heinrich, W. Hu, V. Miranda |
Inflationary Features and Shifts in Cosmological Parameters from Planck 2015 Data |
Phys. Rev. D 96 083526 (2017)
1706.09412 |
202/184 |
H. Motohashi, W. Hu |
Primordial Black Holes and Slow Roll Violation |
Phys. Rev. D 96 063503 (2017)
1706.06784 |
201/183 |
H. Motohashi, W. Hu |
Generalized Slow Roll in the Unified EFT of Inflation |
Phys. Rev. D 96 023502 (2017)
1704.01128 |
200/182 |
P. Motloch, W. Hu, A. Benoit-Levy |
CMB Lens Sample Covariance and Consistency Relations |
Phys. Rev. D 95 043518 (2017)
1612.05637 |
199/181 |
W. Hu, A. Joyce |
Separate Universes beyond General Relativity |
Phys. Rev. D 95 043529 (2017)
1612.02454 |
198/180 |
V. Miranda, A. Lidz, C.H.. Henrich, W. Hu |
Signatures of Metal-Free Star Formation in Planck 2015 Polarization Data |
MNRAS 467 4050 (2017)
1610.00691 |
197/179 |
C.H. Heinrich, V. Miranda, W. Hu |
Complete Reionization Constraints from Planck 2015 Polarization |
Phys. Rev. D
95 023513 (2017)
1609.04788 |
196/178 |
C-T. Chiang, Y. Li, W. Hu, M. LoVerde |
Quintessential Scale Dependence from Separate Universe Simulations |
Phys. Rev. D 94 123502 (2016)
1609.01701 |
195/177 |
C.H. Heinrich, D. Grin, W. Hu |
Lensing Bias to CMB Measurements of Compensated Isocurvature Perturbations |
Phys. Rev. D 94 043534 (2016)
1605.08439 |
194/176 |
W. Hu, C-T. Chiang, Y. Li, M. LoVerde |
Separating the Universe into the Real and Fake |
Phys. Rev. D 94 023002 (2016)
1605.01412 |
193/175 |
P. Gratia, W. Hu, A. Joyce, R.H. Ribeiro |
Double Screening |
JCAP 06 033 (2016)
1604.00395 |
192/174 |
P. Motloch, W. Hu, H. Motohashi |
Self-accelerating Massive Gravity: Hidden Constraints and Characteristics |
Phys. Rev. D 92 0442024 (2015)
1603.03423 |
191/173 |
Y. Li, W. Hu, M. Takada |
Separate Universe Consistency Relation and Calibration of Halo Bias |
Phys. Rev. D 93 063507 (2016)
1511.01454 |
190/172 |
V. Miranda, W. Hu, C. He, H. Motohashi |
Nonlinear Excitations in Inflationary Power Spectra |
Phys. Rev. D 93 023504 (2016)
1510.07580 |
189/171 |
P. Motloch, W. Hu, A. Joyce, H. Motohashi |
Self-accelerating Massive Gravity: Superluminality, Cauchy Surfaces and Strong Coupling |
Phys. Rev. D 92 044024 (2015)
1505.03518 |
188/170 |
C. He, D. Grin, W. Hu |
Compensated Isocurvature Perturbations in the Curvaton Model |
Phys. Rev. D 92 063018 (2015)
1505.00639 |
187/169 |
H. Motohashi, W. Hu |
Running from Features: Optimized Evaluation of Inflationary Power Spectra |
Phys. Rev. D 92 043501 (2015)
1503.04810 |
186/168 |
V. Miranda, W. Hu, C. Dvorkin |
Polarization Predictions for Inflationary CMB Power Spectrum Features |
Phys. Rev. D 91 063514 (2014)
1411.5956 |
185/167 |
P. Motloch, W. Hu |
Self-Accelerating Massive Gravity: Covariant Perturbation Theory |
Phys. Rev. D 90 104027 (2014)
1409.2204 |
184/166 |
H. Motohashi, W. Hu |
Stability of cosmological solutions in extended quasidilaton massive gravity |
Phys. Rev. D 90 104008 (2014)
1408.4813 |
183/165 |
Y. Li, W. Hu, M. Takada |
Super-Sample Signal |
Phys. Rev. D 90 103530 (2014)
1408.1081 |
182/164 |
W. Hu |
Generalized Slow Roll for Tensors |
Phys. Rev. D 89 123503 (2014)
1405.2020 |
181/163 |
C. Dvorkin, M. Wyman, D.H. Rudd, W. Hu |
Neutrinos help reconcile Planck measurements with both Early and Local Universe |
Phys. Rev. D 90 083503 (2014)
1403.8049 |
180/162 |
V. Miranda, W. Hu, P. Adshead |
Steps to Reconcile Inflationary Tensor and Scalar Spectra |
Phys. Rev. D 89 101302 (2014)
1403.5231 |
179/161 |
P. Adshead, W. Hu |
Bounds on Non-Adiabatic Evolution in Single-Field Inflation |
Phys. Rev. D89 083531 (2014)
1402.1677 |
178/160 |
A. Manzotti, W. Hu, A. Benoit-Levy |
Super-Sample CMB Lensing |
Phys. Rev. D 90 023003 (2014)
1401.7992 |
176/159 |
Y. Li, W. Hu, M. Takada |
Super-Sample Covariance in Simulations |
Phys. Rev. D 89 083519 (2014)
1401.0385 |
175/158 |
V. Miranda, W. Hu |
Inflationary Steps in the Planck Data |
Phys. Rev. D 89083529 (2014)
1312.0946 |
174/157 |
P. Gratia, W. Hu, M. Wyman |
Self-accelerating Massive Gravity: Bimetric Determinant Singularity |
Phys. Rev. D 89 027502 (2014)
1309.5947 |
173/156 |
M. Wyman, D.H. Rudd, R.A. Vanderveld, W. Hu |
nuLCDM: Neutrinos reconcile Planck with the Local Universe |
Phys. Rev. Lett. 112 051302 (2014)
1307.7715 |
172/155 |
P. Gratia, W. Hu, M. Wyman |
Self-accelerating Massive Gravity: How Zweibeins Walk Through Determinant Singularities |
Class. Quantum Grav. 30 184007 (2013)
1305.2916 |
171/154 |
E. Jennings, Y. Li, W. Hu |
The Abundance of Voids and the Excursion Set Formalism |
MNRAS 434 2167 (2013)
1304.6087 |
170/153 |
P. Adshead, W. Hu, V. Miranda |
Bispectrum in Single-Field Inflation Beyond Slow-Roll |
Phys. Rev. D 88 023507 (2013)
1303.7004 |
169/152 |
M. Takada, W. Hu |
Power Spectrum Super-Sample Covariance |
Phys. Rev. D 87 123504 (2013)
1302.6994 |
168/151 |
R. A. Vanderveld, W. Hu |
Neutrino physics from future weak lensing surveys |
Phys. Rev. D 87 063510 (2013)
1212.3608 |
167/150 |
A. V. Belikov, W. Hu |
Equivalence Principle Violation in Weakly Vainshtein-Screened Systems |
Phys. Rev. D 87 084042 (2013)
1212.0831 |
166/149 |
M. Wyman, W. Hu, P. Gratia |
Self-accelerating Massive Gravity: Time for Field Fluctuations |
Phys. Rev. D 87 084046 (2013)
1211.4576 |
165/148 |
T. Hiramatsu, W. Hu, K. Koyama, F. Schmidt |
Equivalence Principle Violation in Vainshtein Screened Two-Body Systems |
Phys. Rev. D 87 063525 (2013)
1209.3364 |
164/147 |
V. Miranda, W. Hu, P. Adshead |
Warp Features in DBI Inflation |
Phys. Rev. D 86 063529 (2012)
1207.2186 |
163/146 |
P. Gratia, W. Hu, M. Wyman |
Self-accelerating Massive Gravity: Exact Solutions for Any Isotropic Matter Distribution |
Phys. Rev. D. 86 061504 (2012; rapid communications)
1205.4241 |
162/145 |
A. Benoit-Levy, K.M. Smith, W. Hu |
Non-Gaussian Structure of the Lensed CMB Power Spectra Covariance Matrix |
Phys. Rev. D 86 123008 (2012)
1205.0474 |
161/144 |
A. Upadhye, W. Hu, J. Khoury |
Quantum Stability of Chameleon Field Theories |
Phys. Rev. Lett. 109 041301 (2012)
1204.3906 |
160/143 |
R.A. Vanderveld, M.J. Mortonson, W. Hu, T. Eifler |
Testing Dark Energy Paradigms with Weak Gravitational Lensing |
Phys. Rev. D 85 103518 (2012)
1203.3195 |
159/142 |
P. Adshead, W. Hu |
Fast Computation of First-Order Feature-Bispectrum Corrections |
Phys. Rev. D 85 103531 (2012)
1203.0012 |
158/141 |
P. Adshead, C. Dvorkin, W. Hu, E. A. Lim |
Non-Gaussianity from Step Features in the Inflationary Potential |
Phys. Rev. D 85 023531 (2012)
1110.3050 |
157/140 |
C. Dvorkin, M. Wyman, W. Hu |
Cosmic String constraints from WMAP and SPT |
Phys. Rev. D 84 123519 (2011)
1109.4947 |
156/139 |
H. Gil-Marin, F. Schmidt, W. Hu, R. Jimenez, L. Verde |
The Bispectrum of f(R) Cosmologies |
JCAP 11 019 (2011)
1109.2115 |
155/138 |
Y. Li, W. Hu |
Chameleon Halo Modeling in f(R) Gravity |
Phys. Rev. D 84 084033
1107.5120 |
154/137 |
C. Dvorkin, W. Hu |
Complete WMAP Constraints on Bandlimited Inflationary Features |
Phys. Rev. D 84 063515 (2011)
1106.4016 |
153/136 |
W. Hu |
Generalized Slow Roll for Non-Canonical Kinetic Terms |
Phys. Rev. D 84 027303 (2011)
1104.4500 |
152/135 |
P. Adshead, W. Hu, C. Dvorkin, H.V. Peiris |
Fast Computation of Bispectrum Features with Generalized Slow Roll |
Phys. Rev. D 84 043519 (2011)
1102.3435 |
151/134 |
S. Ferraro, F. Schmidt, W. Hu |
Cluster Abundance in f(R) Gravity Models |
Phys. Rev. D 83 063503 (2011)
1011.0992 |
150/133 |
M. J. Mortonson, W. Hu, D. Huterer |
Simultaneous Falsification of LCDM and Quintessence with Massive Distant Clusters |
Phys. Rev. D 83 023015 (2011)
1011.0004 |
149/132 |
S. S. Seahra, W. Hu |
Analytic Description of DGP Perturbations on All Scales |
Phys. Rev. D 82 124015 (2010)
1007.4242 |
148/131 |
C. Dvorkin, W. Hu |
CMB Constraints on Principal Components of the Inflaton Potential |
Phys. Rev. D 82 043513 (2010)
1007.0215 |
147/130 |
M. J. Mortonson, D. Huterer, W. Hu |
Figures of merit for present and future dark energy probes |
Phys. Rev. D 82 063004 (2010)
1004.0236 |
146/129 |
L. Lombriser, A. Slosar, U. Seljak, W. Hu |
Constraints on f(R) gravity from probing the large-scale structure |
Phys. Rev. D 85 124038 (2012)
1003.3009 |
145/128 |
M. J. Mortonson, W. Hu |
Observational Limits on Patchy Reionization: Implications for B-modes |
Phys. Rev. D 81 067302 (2010)
1001.4803 |
144/127 |
M. J. Mortonson, W. Hu, D. Huterer |
Testable Dark Energy Predictions from Current Data |
Phys. Rev. D 81 063007 (2010)
0912.3816 |
143/126 |
F. Schmidt, W. Hu, M. Lima |
Spherical Collapse and the Halo Model in Braneworld Gravity |
Phys. Rev. D 81 063005 (2010)
0911.5178 |
142/125 |
C. Dvorkin, W. Hu |
Generalized Slow Roll for Large Power Spectrum Features |
Phys. Rev. D 81 023518 (2010)
0910.2237 |
141/124 |
F. Schmidt, A. Vikhlinin, W. Hu |
Cluster Constraints on f(R) Gravity |
Phys. Rev. D 80 083505 (2009)
0908.2457 |
140/123 |
M. J. Mortonson, W. Hu, D. Huterer |
Hiding Dark Energy Transitions at Low Redshift |
Phys. Rev. D 80 067301 (2009)
0908.1408 |
139/122 |
M. J. Mortonson, W. Hu |
Evidence for Horizon-Scale Power from CMB Polarization |
Phys. Rev. D 80 027301 (2009)
0906.3016 |
138/-- |
W. Hu |
Acceleration from Modified Gravity: Lessons from Worked Examples |
Nuc. Phys. Proc. Suppl. 194 230 (2009)
0906.2024 |
137/121 |
A. Upadhye, W. Hu |
The Existence of Relativistic Stars in f(R) Gravity |
Phys. Rev. D 80 064002
0905.4055 |
136/120 |
L. Lombriser, W. Hu, W. Fang, U. Seljak |
Cosmological Constraints on DGP Braneworld Gravity with Brane Tension |
Phys. Rev. D 80 063536
0905.1112 |
135/119 |
M.J.Mortonson, C. Dvorkin, H. V. Peiris, W. Hu |
Things that Go Bump in the CMB Polarization: features from Inflation vs. Reionization |
Phys. Rev. D 79 103519 (2009)
0903.4920 |
134/118 |
C. Dvorkin, W. Hu, K. M. Smith |
B-mode CMB Polarization from Patchy Screening during Reionization |
Phys. Rev. D 79 107302 (2009)
0902.4413 |
133/117 |
F. Schmidt, M.V. Lima, H. Oyaizu, W. Hu |
Non-linear Evolution of f(R) Cosmologies III: Halo Statistics |
Phys. Rev. D 79 083518 (2009)
0812.0545 |
132/116 |
M. J. Mortonson, W. Hu, D. Huterer |
Falsifying Paradigms for Cosmic Acceleration |
Phys. Rev. D 79 023004 (2009)
0810.1744 |
131/115 |
W. Fang, W. Hu, A. Lewis |
Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy |
Phys. Rev. D 78 087303 (2008)
0808.3125 |
130/114 |
W. Fang et al. |
Challenges to the DGP Model from Horizon-Scale Growth and Geometry |
Phys. Rev. D 78 103509 (2008)
0808.2208 |
129/113 |
H. Oyaizu, M. Lima, W. Hu |
Non-linear evolution of f(R) cosmologies II: power spectrum |
Phys. Rev. D 78 123524 (2008)
0807.2462 |
128/112 |
M.J. Mortonson, W. Hu |
Reionization Constraints from Five-Year WMAP Data |
Astrophys. J. Lett. 686 L53 (2008)
0804.2631 |
127/--
|
W.
Hu
|
Lecture Notes on CMB Theory: From Nucleosynthesis to Recombination
|
XIX Canary Island Winter School
0802.3688
|
126/111 |
W. Hu |
Parametrized Post-Friedmann Signatures of Acceleration in the CMB |
Phys. Rev. D 77 103524 (2008)
0801.2433 |
125/110 |
C. Dvorkin, H. V. Peiris, W. Hu |
Testable Polarization Predictions for Models of CMB Isotropy Anomalies |
Phys. Rev. D 77 063008 (2008)
0711.2321 |
124/109 |
M. J. Mortonson, W. Hu |
Impact of Reionization on CMB Polarization Tests of Slow-Roll Inflation |
Phys. Rev. D 77 043506 (2008)
0710.4162 |
123/108 |
A.R. Zentner, D.H. Rudd, W. Hu |
Self Calibration of Tomographic Weak Lensing for the Physics of Baryons to Constrain Dark Energy |
Phys. Rev. D 77 043507 (2008)
0709.4029 |
122/107 |
M. Lima, W. Hu |
Photometric Redshift Requirements for Self-Calibration of Cluster Dark Energy Studies |
Phys. Rev. D 76 123013 (2007)
0709.2871 |
121/106 |
W. Hu, D.E. Holz, C. Vale |
CMB Cluster Lensing: Cosmography with the Longest Lever Arm |
Phys. Rev. D 76 127301 (2007)
0708.4391 |
120/105 |
W. Hu, I. Sawicki |
A Parameterized Post-Friedmann Framework for Modified Gravity |
Phys. Rev. D 76 104043 (2007)
0708.1190 |
119/104 |
Y.S. Song, H. Peiris, W. Hu |
Cosmological Constraints on f(R) Acceleration Models |
Phys. Rev. D 76 063517 (2007)
0706.2399 |
118/103 |
W. Hu, I. Sawicki |
Models of f(R) Cosmic Acceleration that Evade Solar-System Tests |
Phys. Rev. D 76 064004 (2007)
0705.1158 |
117/102 |
M. J. Mortonson, W. Hu |
Model-Independent Constraints on Reonization from Large-Scale CMB Polarization |
Astrophys. J 672 737 (2008)
0705.1132 |
116/101 |
I. Sawicki, W. Hu |
Stability of Cosmological Solutions in f(R) Models of Gravity |
Phys. Rev. D 75 127502 (2007)
astro-ph/0702278 |
115/100 |
W. Hu, S. DeDeo, C. Vale |
Cluster Mass Estimators from CMB Temperature and Polarization Lensing |
New J. of Phys. 9 441 2007
astro-ph/0701276 |
114/99 |
Y.S. Song, W. Hu, I. Sawicki |
The Large Scale Structure of f(R) Gravity |
Phys. Rev. D 75 044004 (2007)
astro-ph/0610532 |
113/98 |
A. Albrecht et al. |
Report of the Dark Energy Task Force |
AAAC/HEPAP
astro-ph/0609591 |
112/98 |
M. J. Mortonson, W. Hu |
The Maximum B-mode Polarization of the Cosmic Microwave Background from Inhomogeneous Reionization |
Astrophys. J 657 1 (2007)
astro-ph/0607652 |
111/97 |
W. Hu, D. Huterer, K. M. Smith |
Supernovae, Lensed CMB and Dark Energy |
Astrophys. J. Lett. 650 L13 (2006)
astro-ph/0607316 |
110/96 |
K. M. Smith, W. Hu, M. Kaplinghat |
Cosmological Information from Lensed CMB Power Spectra |
Phys. Rev. D 74 123002 (2006)
astro-ph/0607315 |
109/95 |
Y.S. Song, I. Sawicki, W. Hu |
Large Scale Tests of the DGP Model |
Phys. Rev. D 75 064003 (2007)
astro-ph/0606286 |
108/94 |
I. Sawicki, Y.S. Song, W. Hu |
Near-Horizon Solution for DGP Perturbations |
Phys. Rev. D 75 064002 (2007)
astro-ph/0606285 |
107/93 |
W. Hu, J. D. Cohn |
Likelihood Methods for Cluster Dark Energy Surveys |
Phys. Rev. D 73 067301 (2006)
astro-ph/0602147 |
106/92 |
X. Wang, W. Hu |
Redshift Space 21cm Power Spectra from Reionization |
Astrophys. J 643 585 (2006)
astro-ph/0511141 |
105/91 |
C. Gordon, W. Hu, D. Huterer, T. Crawford |
Spontaneous Isotropy Breaking: A Mechanism for CMB Multipole Alignments |
Phys. Rev. D 72 103002 (2005)
astro-ph/0509301 |
104/90 |
Y. S. Song, W. Hu |
Constraints on Supernovae Dimming from Photon-Pseudo Scalar Coupling |
Phys. Rev. D 73 023003 (2006)
astro-ph/0508002 |
103/89 |
Z.Ma, W.Hu, D.Huterer |
Effects of Photometric Redshift Uncertainties on Weak Lensing Tomography |
Astrophys. J. 636 21 (2005)
astro-ph/0506614 |
102/88 |
S.Wang, Z.Haiman, W.Hu, J.Khoury, M.May |
Weighing Neutrinos with Galaxy Cluster Surveys |
Phys. Rev. Lett. 95 011302 (2005)
astro-ph/0505390 |
101/87 |
K.Kadota, S.Dodelson, W.Hu, E.D.Stewart |
Precision of Inflaton Potential Reconstruction from CMB Using the General Slow-Roll Approximation |
Phys. Rev. D 72 023510 (2005)
astro-ph/0505158 |
100/86 |
M.Lima, W.Hu |
Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution |
Phys. Rev. D 72 043006 (2005)
astro-ph/0503363 |
99/85 |
D.Giannakis, W.Hu |
Challenges for Kinetic Unified Dark Matter |
Phys. Rev. D 72 063502 (2005)
astro-ph/0501423 |
98/84 |
W.Hu |
Crossing the Phantom Divide: Dark Energy Internal Degrees of Freedom |
Phys. Rev. D 71 047301 (2005)
astro-ph/0410680 |
97/83 |
W.Hu, R.Scranton |
Measuring Dark Energy Clustering with CMB-Galaxy Correlations |
Phys. Rev. D 70 123002 (2004)
astro-ph/0408456 |
96/-- |
W.Hu |
Dark Energy Probes in Light of the CMB |
ASPCS 339 215 (2005)
astro-ph/0407158 |
95/82 |
C.Gordon, W.Hu |
A Low CMB Quadrupole from Dark Energy Isocurvature Perturbations |
Phys. Rev. D 70 083003 (2004)
astro-ph/0406496 |
94/81 |
K.M.Smith, W.Hu, M.Kaplinghat |
Weak Lensing of the CMB: Sampling Errors on B-modes |
Phys. Rev. D 70 043002 (2004)
astro-ph/0402442 |
93/-- |
W.Hu
|
Covariant Linear Perturbation Formalism
|
ICTP Summer School (G. Dvali et al. eds, ICTP Trieste 2003) p. 149
astro-ph/0402060 |
92/80 |
M.Lima, W.Hu
|
Self-Calibration of Cluster Dark Energy
Studies: Counts in Cells
|
Phys. Rev. D 70 043504 (2004)
astro-ph/0401559 |
91/79 |
W.Hu, M.White
|
The Cosmic Symphony
|
Sci. Am. 290N2 44 (2004) |
90/78 |
W.Hu, B.Jain
|
Joint Galaxy-Lensing Observables and the Dark Energy
|
Phys. Rev. D 70 043009 (2004) astro-ph/0312395 |
89/77 |
M. Bowden et al.
|
Scientific Optimization of a Ground-Based CMB Polarization Experiment
|
Mon. Not. R. Astron. Soc. 349 321 (2004) astro-ph/0309610 |
88/76 |
W.Hu, T.Okamoto
|
Principal Power of the CMB
|
Phys. Rev. D 69 043004 (2004) astro-ph/0308049 |
87/75 |
W.Hu, Z.Haiman
|
Redshifting Rings of Power
|
Phys. Rev. D 68 063004 (2003) astro-ph/0306053 |
86/74 |
W.Hu, G.P.Holder
|
Model-Independent Reionization Observables in the CMB
|
Phys. Rev. D 68 023001 (2003) astro-ph/0303400 |
85/73 |
W.Hu |
Self-Consistency and Calibration of Cluster Number Count Surveys for Dark Energy
|
Phys. Rev. D 67 081304 (2003) astro-ph/0301416 |
84/72 |
T. Okamoto, W.Hu
|
CMB Lensing Reconstruction on the Full Sky
|
Phys. Rev. D 67 083002 (2003) astro-ph/0301031 |
83/71 |
W.Hu |
CMB Temperture and Polarization Anisotropy
Fundamentals (high res.)
|
Annals of Physics 303 203 (2003) astro-ph/0210696 |
82/70 |
W.Hu, M.M.Hedman, M.Zaldarriaga
|
Benchmark Parameters for CMB Polarization Experiments
|
Phys. Rev. D 67 043004 (2003) astro-ph/0210096 |
81/69 |
W.Hu |
Dark Energy and Matter Evolution from Lensing Tomography
|
Phys. Rev. D 66 083515 (2003) astro-ph/0208093 |
80/68 |
T.Okamoto, W.Hu |
The Angular Trispectra of CMB Temperature and Polarization
|
Phys. Rev. D 66 063008 (2003) astro-ph/0206155 |
79/67 |
W.Hu, C.R.Keeton |
Three-Dimensional Mapping of the Dark Matter
|
Phys. Rev. D 66 063506 (2003) astro-ph/0205412 |
78/66 |
W.Hu, A.V.Kravtsov |
Sample Variance Considerations for Cluster Surveys
|
Astrophys. J. 584 702 (2003) astro-ph/0203169 |
77/65 |
A.Cooray, W.Hu |
Second Order Corrections to Weak Lensing by
Large-Scale Structure
|
Astrophys. J. 574 19 (2002) astro-ph/0202411 |
76/64 |
W.Hu, T.Okamoto |
Mass Reconstruction with CMB Polarization
|
Astrophys. J. 574 566 (2002) astro-ph/0111606 |
75/63 |
W.Hu,S.Dodelson |
Cosmic Microwave Background Anisotropies
(pub. vers.) |
Ann. Rev. Astron. Astrophys. 40 171 (2002) astro-ph/0110414 |
74/62 |
W.Hu |
Dark Synergy: Gravitational Lensing and the CMB
|
Phys. Rev. D 65 023003 (2002) astro-ph/0108090 |
73/61 |
W.Hu |
Mapping the Dark Matter through the CMB Damping Tail
|
Astrophys. J. Lett. 557 L79 (2001) astro-ph/0105424 |
72/60 |
W.Hu |
The Angular Trispectrum of the CMB
|
Phys. Rev. D. 64 083005 (2001) astro-ph/0105117 |
71/59 |
A.R.Cooray, W.Hu, D.Huterrer, M.Joffre |
Measuring Angular Diameter Distances
Through Halo Clustering
|
Astrophys. J. Lett. 557 L7 (2001) astro-ph/0105061 |
70/-- |
W.Hu |
Physics of CMB Anisotropies
(2001) |
Warner Prize Lecture Jan. 2001 AAS Meeting (San Diego) |
69/58 |
A.R.Cooray, W.Hu |
Power Spectrum Covariance of
Weak Gravitational Lensing |
Astrophys. J. 554 56 (2001) astro-ph/0012087 |
68/57 |
W.Hu, M.White |
Power Spectra Estimation for Weak Lensing |
Astrophys. J. 554 67 (2001) astro-ph/0010352 |
67/56 |
W.Hu, A.R.Cooray |
Gravitational Time Delay Effects on
CMB Anisotropies |
Phys. Rev. D. 63 023504 (2001) astro-ph/0008001 |
66/55 |
W.Hu, M.Fukugita, M.Zaldarriaga, M.Tegmark |
CMB Observables
and Their Cosmological Implications |
Astrophys. J. 549 669 (2001) astro-ph/0006436 |
65/54 |
P.J.E. Peebles, S.Seager, W.Hu |
Delayed Recombination |
Astrophys. J. Lett. 539 L1 (2000) astro-ph/0004389 |
64/53 |
W.Hu |
Ringing in the
New Cosmology |
Nature 404 939 (News and Views on BOOMERanG) |
63/52 |
A.R.Cooray, W.Hu |
Weak
Gravitational Lensing Bispectrum |
Astrophys. J 548 7 (2001) astro-ph/0004151 |
62/51 |
W.Hu, R.Barkana, A.Gruzinov |
Cold and Fuzzy
Dark Matter |
Phys. Rev. Lett. 85 1158 (2000) astro-ph/0003365 |
61/50 |
A.R.Cooray, W.Hu, J.Miralda-Escude |
Weak Lensing
by Large-Scale Structure: A Dark Matter Halo Approach |
Astrophys. J. 535 L9 (2000) astro-ph/0003205 |
60/-- |
W.Hu |
CMB Anisotropies:
A Decadal Survey |
Invited Review for Birth and Evolution of the Universe RESCEU
1999 astro-ph/0002520 |
59/49 |
A.R.Cooray, W.Hu, M.Tegmark |
Large-Scale
Sunyaev-Zel'dovich Effect: Measuring Statistical Properties with Multifrequency
Maps |
Astrophys. J. 540 1 (2000) astro-ph/0002238 |
58/48 |
W.Hu |
Weak Lensing
of the CMB: A Harmonic Approach |
Phys. Rev. D. 62 043007 (2000) astro-ph/0001303 |
57/47 |
A.R.Cooray, W.Hu |
Imprint
of Reionization on the Cosmic Microwave Background Bispectrum |
Astrophys. J. 534 533 (2000) astro-ph/9910397 |
56/46 |
W.Hu, P.J.E.Peebles |
A Model for
Structure Formation seeded by Gravitationally Produced Matter |
Astrophys. J. Lett. 528 61 (2000) astro-ph/9910222 |
55/45 |
M.White,W.Hu |
A New Algorithm
for Computing Statistics of Weak Lensing by Large-Scale Structure |
Astrophys. J. 537 1 (2000) astro-ph/9909165 |
54/44 |
W.Hu |
Reionization
Revisited: Secondary CMB Anisotropies and Polarization |
Astrophys. J. 529 12 (2000) astro-ph/9907103 |
53/-- |
W.Hu |
CMB
Episode II: Theory or Reality? |
invited talk for ISOSII |
52/43 |
M.Tegmark, D.J.Eisenstein, W.Hu,A.de Oliviera Costa |
Foregrounds
and Forecasts for the Cosmic Microwave Background |
Astrophys. J. 530 133 (2000) astro-ph/9905257 |
51/42 |
W.Hu |
Power Spectrum
Tomography with Weak Lensing |
Astrophys. J. Lett. 522 21 (1999) astro-ph/9904153 |
50/41 |
R.A.C.Croft, W.Hu, R. Dave |
Cosmological
Limits on the Neutrino Mass from the Lya Forest |
Phys. Rev. Lett. 83 1092 (1999) astro-ph/9903335 |
49/-- |
W.Hu |
Probing
the Dark Side of Structure Formation |
invited talk for Omega Workshop, Pucon, Chile a.k.a. the job
talk |
48/40 |
W.Hu, M.Tegmark |
Weak Lensing:
Prospects for Cosmological Parameter Measurements |
Astrophys. J. Lett. 514 65 (1999) astro-ph/9811168 |
47/39 |
W.Hu, D.J.Eisenstein |
The Structure
of Structure Formation Theories |
Phys. Rev. D. 59 083509 (1999) astro-ph/9809368 |
46/38 |
W.Hu |
An Isocurvature
Mechanism for Structure Formation |
Phys. Rev. D. 59 021301 (1998; rapid communications) astro-ph/9809142 |
45/37 |
D.J.Eisenstein, W.Hu, M. Tegmark |
Cosmic Complementarity:
Joint Parameter Estimation from CMB Experiments and Redshift Surveys |
Astrophys. J. 518 2 (1999) astro-ph/9807130 |
44/36 |
W.Hu, D.J.Eisenstein, M.Tegmark, M.White |
Observationally
Determining the Properties of Dark Matter |
Phys. Rev. D. 59 023512 (1999) astro-ph/9806362 |
43/35 |
D.J.Eisenstein, W.Hu, M.Tegmark |
Cosmic Complementarity:
H0 and Omegam from Combining CMB Experiments and
Redshift Surveys |
Astrophys. J. Lett. 504 L57 (1998) astro-ph/9805239 |
42/34 |
M.Tegmark, D.J.Eisenstein, W.Hu, R.Kron |
Probing
the Acceleration of the Universe |
astro-ph/9805117 |
41/-- |
W.Hu |
Toward
Observationally Determining the Nature of the Missing Energy |
Fermilab Workshop on The Missing Energy in the Universe |
40/-- |
M.Tegmark, D.J.Eisenstein, W.Hu |
Cosmic Complementarity:
Combining CMB and Supernova Observations |
Proceedings of the XXXIIIrd Moriond Meeting, Fundamental Parameters in Cosmology,
ed. J. Tran Thanh Van, Y. Giraud-Heraud, F. Bouchet, T. Damour, Y. Mellier (Edition Frontieres 1998) astro-ph/9804168 |
39/33 |
A.Gruzinov, W.Hu |
Secondary CMB
Anisotropies in a Universe Reionized in Patches |
Astrophys. J. 508 435 (1998) astro-ph/9803188 |
38/32 |
W.Hu |
Structure Formation
with Generalized Dark Matter |
Astrophys. J. 506 485 (1998) astro-ph/9801234 |
37/31 |
W.Hu, D.J.Eisenstein, M.Tegmark |
Weighing
Neutrinos with Galaxy Surveys |
Phys. Rev. Lett. 80 5255 (1998) astro-ph/9712057 |
36/30 |
D.J.Eisenstein, W.Hu, J.Silk, A.S.Szalay |
Can Baryonic
Features Produce the Observed 100h-1 Mpc Clustering |
Astrophys. J. Lett 494 1 (1998) astro-ph/9710303 |
35/29 |
D.J.Eisenstein, W.Hu |
Power Spectra
for Cold Dark Matter and Its Variants |
Astrophys. J. 511 5 (1999) astro-ph/9710252 |
34/28 |
W.Hu, D.J.Eisenstein |
Small Scale
Perturbations in a General MDM Cosmology |
Astrophys. J. 498 497 (1998) astro-ph/9710216 |
33/27 |
D.J.Eisenstein, W.Hu |
Baryonic Features
in the Matter Transfer Function |
Astrophys. J. 496 605 (1998) astro-ph/9709112 |
32/26 |
W.Hu, U.Seljak, M.White, M.Zaldarriaga |
A Complete Treatment
of CMB Anisotropies in a FRW Universe |
Phys. Rev. D 57 3290 (1998) astro-ph/9709066 |
31/-- |
W.Hu |
An
Introduction to the CMB |
IAS Trustees Meeting (Fall 1996) |
30/25 |
W.Hu, M.White |
A CMB Polarization Primer |
New Astronomy 2 323 (1997) astro-ph/9706147 |
29/24 |
W.Hu, M.White |
CMB Anisotropies:
Total Angular Momentum Method |
Phys. Rev. D 56 596 (1997) astro-ph/9702170 |
28/23 |
W.Hu, M.White |
Tensor
Anisotropies in an Open Universe |
Astrophys. J. Lett. 486 L1 (1997) astro-ph/9701210 |
27/22 |
M.White, W.Hu |
The Sachs-Wolfe
Effect |
Astron. & Astrophys. 321 8 (1997) astro-ph/9609105 |
26/21 |
W.Hu, M.White |
The Damping Tail
of CMB Anisotropies |
Astrophys. J. 479 568 (1997) astro-ph/9609079 |
25/-- |
W.Hu, M.White |
Measuring
the Curvature of the Universe |
Proceedings of the XXXIth Moriond Meeting, Microwave Background
Anisotropies, ed. F.R. Bouchet, R. Gispert, B. Guiderdoni, J.T.T. Van,
Editions Frontieres (Singapore 1997) p. 333. astro-ph/9606140 |
24/-- |
M.White, W.Hu |
Testing
Inflation with Small Scale CMB Anisotropies |
Proceedings of the XXXIth Moriond Meeting, Microwave Background
Anisotropies, ed. F.R. Bouchet, R. Gispert, B. Guiderdoni, J.T.T. Van,
Editions Frontieres (Singapore 1997) p. 339. astro-ph/9606138 |
23/20 |
W.Hu, D.N.Spergel,
M.White |
Distinguishing
Causal Seeds from Inflation |
Phys. Rev. D 51 3288 (1997) astro-ph/9605193 |
22/19 |
W.Hu, N.Sugiyama,
J.Silk |
The
Physics of CMB Anisotropies |
Nature 386 37-43 (1997) astro-ph/9604166 |
21/18 |
W.Hu, M.White |
A New Test
of Inflation |
Phys. Rev. Lett. 77, 1687 (1996) astro-ph/9602020 |
20/17 |
W.Hu, M.White |
Acoustic
Signatures in the Cosmic Microwave Background |
Astrophys. J. 471 30 (1996) astro-ph/9602019 |
19/16 |
W.Hu, N.Sugiyama |
Small Scale
Cosmological Perturbations: An Analytic Approach |
Astrophys. J. 471 542 (1996) astro-ph/9510117 |
18/-- |
W.Hu |
Concepts
in CMB Anisotropy Formation |
The Universe at High-z, LSS & the CMB (eds. E. Martinez-Gonzalez,
J.L. Sanz, Springer Verlag, 1996) p. 207 astro-ph/9511130 |
17/-- |
W.Hu |
Wandering in
the Background: A CMB Explorer |
PhD Thesis, UC Berkeley (1995) astro-ph/9508126 |
16/15 |
W.Hu, M.White |
CMB Anisotropies
in the Weak Coupling Limit |
Astron. & Astrophys. 315 33 (1996) astro-ph/9507060 |
15/14 |
W.Hu, D.Scott,
N.Sugiyama,
M.White |
The Effect of
Physical Assumptions on the Calculation of Microwave Background Anisotropies |
Phys. Rev. D 52, 5498 (1995) astro-ph/9505043 |
14/13 |
W.Hu, E.Bunn, N.Sugiyama |
COBE Constraints
on Isocurvature Baryon Models |
Astrophys. J. Lett. 447, L59 (1995) astro-ph/9501034 |
13/12 |
W.Hu, N.Sugiyama, |
Toward Understanding
CMB Anisotropies and Their Implications |
Phys. Rev. D 51, 2599 (1995) astro-ph/9411008 |
12/11 |
W.Hu, N.Sugiyama, |
Anisotropies
in the CMB: An Analytic Approach |
Astrophys. J. 444 , 489 (1995) astro-ph/9407093 |
11/-- |
W.Hu, |
The Nature
vs. Nurture of Anisotropies |
CMB Anisotropies Two Years after COBE: Observations, Theory, and
the Future ed. L.M. Krauss, p. 188. astro-ph/9406071 |
10/10 |
W.Hu, N.Sugiyama, |
Thermal History
Constraints on the Isocurvature Baryon Model |
Astrophys. J. 436, 456 (1994) astro-ph/9403031 |
9/9 |
M.Tegmark, E.Bunn,
W.Hu |
Power Spectrum
Independent Constraints on Cosmological Models |
Astrophys. J. 431, 1 (1994) astro-ph/9311053 |
8/8 |
W.Hu, N.Sugiyama |
Small Scale Integrated
Sachs-Wolfe Effect |
Phys. Rev. D 50, 627 (1994) astro-ph/9310046 |
7/7 |
W.Hu, D.Scott,
J.Silk |
Power
Spectrum Constraints from Spectral Distortions in the CMB |
Astrophys. J. Lett. 430, L5 (1994) astro-ph/9402045 |
6/6 |
W.Hu, D.Scott,
J.Silk |
Reionization
and CMB Distortions: A Complete Treatment of Second Order Compton Scattering |
Phys. Rev. D 49, 648 (1994) astro-ph/9305038 |
5/5 |
W.Hu, J.Silk |
Thermalization
and Spectral Distortions of the CBR |
Phys. Rev. D 48, 485 (1994) |
4/4 |
W.Hu, J.Silk |
Thermalization
Constraints and Spectral Distortions for Massive Unstable Relic Particles |
Phys. Rev. Lett. 70, 2661 (1993) |
3/3 |
K.Griest,
W.Hu |
Effect of Binary
Sources on the Search for MACHOS via Microlensing |
Astrophys. J. 397, 362 (1992) |
2/2 |
W.Hu, R.W.Romani, D.R.Stinebring |
Refractive
Interstellar Scintillation and Millisecond Pulsar Timing |
Astrophys. J. Lett. 366, L33 (1991) |
1/1 |
W.Hu |
The Curious Quantum Mechanics of Pre- and Post-Selected Ensembles |
Foundations of Physics 20, 447 (1990) |