Abstract is: Andrew R. Liddle FRSE (born 9 June 1965) is Professor of astrophysics at the Royal Observatory Edinburgh. Publications include books and over 260 papers. He is a theoretical cosmologist and is interested in understanding the properties of the Universe and how these relate to fundamental physical laws.
human | Q5 |
P4594 | arXiv author ID | liddle_a_1 |
P8880 | AstroGen ID | 25325 |
P268 | Bibliothèque nationale de France ID | 14541396b |
P7893 | CIÊNCIAVITAE ID | C516-5189-350B |
P6178 | Dimensions author ID | 014705537145.53 |
P646 | Freebase ID | /m/09ntfw |
P227 | GND ID | 136952208 |
P9467 | IAU member ID | 1041 |
P269 | IdRef ID | 091448417 |
P2930 | INSPIRE-HEP author ID | A.R.Liddle.1 |
P213 | ISNI | 0000000355613341 |
P244 | Library of Congress authority ID | nr95006642 |
P5587 | Libris-URI | 64jln5jq5j524rm |
P8189 | National Library of Israel J9U ID | 987007424314405171 |
P1006 | Nationale Thesaurus voor Auteursnamen ID | 195052927 |
P691 | NL CR AUT ID | jo2012710542 |
P1695 | NLP ID (old) | a0000001206617 |
P1015 | NORAF ID | 99021467 |
P1207 | NUKAT ID | n00068507 |
P496 | ORCID iD | 0000-0002-8164-4830 |
P7293 | PLWABN ID | 9810661360305606 |
P1153 | Scopus author ID | 7006135719 |
P906 | SELIBR ID | 228442 |
P7671 | Semion author ID | 17632560 |
P3987 | SHARE Catalogue author ID | 65972 |
P10861 | Springer Nature person ID | 014705537145.53 |
P214 | VIAF ID | 74089833 |
P10832 | WorldCat Entities ID | E39PBJxWMQ9gkK4chM4QRt6Frq |
P1556 | zbMATH author ID | liddle.andrew-r |
P27 | country of citizenship | United Kingdom | Q145 |
P69 | educated at | University of Glasgow | Q192775 |
P108 | employer | University of Edinburgh | Q160302 |
Imperial College London | Q189022 | ||
University of Glasgow | Q192775 | ||
University of Lisbon | Q1122926 | ||
University of Sussex | Q1161297 | ||
Perimeter Institute for Theoretical Physics | Q2004561 | ||
P734 | family name | Liddle | Q6543617 |
Liddle | Q6543617 | ||
Liddle | Q6543617 | ||
P735 | given name | Andrew | Q18042461 |
Andrew | Q18042461 | ||
P1412 | languages spoken, written or signed | English | Q1860 |
P6104 | maintained by WikiProject | WikiProject Mathematics | Q8487137 |
P463 | member of | International Astronomical Union | Q6867 |
P106 | occupation | astronomer | Q11063 |
physicist | Q169470 | ||
P21 | sex or gender | male | Q6581097 |
Q59450880 | Accurate determination of inflationary perturbations |
Q59450490 | An evolutionary paradigm for dusty active galaxies at low redshift |
Q59450779 | Apparent and actual galaxy cluster temperatures |
Q59450977 | Baryogenesis in extended inflation. I. Baryogenesis via production and decay of supermassive bosons |
Q59450981 | Baryogenesis in extended inflation. II. Baryogenesis via primordial black holes |
Q59450395 | Bayesian model averaging in astrophysics: a review |
Q59450911 | Can the gravitational wave background from inflation be detected locally? |
Q51084903 | Can topological defects mimic the BICEP2 B-mode signal? |
Q59450932 | Characteristics of unwinding textures |
Q58916608 | Cold dark matter models with high baryon content |
Q59450952 | Collapse of spherically symmetric textures |
Q59450888 | Conditions for successful extended inflation |
Q59450400 | Cosmic Microwave Background Anomalies in an Open Universe |
Q59450532 | Cosmic microwave anisotropies from BPS semilocal strings |
Q59450824 | Cosmic microwave background constraints on the epoch of reionization |
Q59450586 | Cosmic reionization constraints on the nature of cosmological perturbations |
Q59450839 | Cosmological parameter estimation and the spectral index from inflation |
Q60908920 | Dark Energy Survey Year 1 Results: A Precise H0 Estimate from DES Y1, BAO, and D/H Data |
Q44853455 | Early assembly of the most massive galaxies. |
Q59450898 | Erratum: Can the gravitational wave background from inflation be detected locally? [Phys. Rev. D49, 3805 (1994)] |
Q52394982 | Exponential Potentials, Scaling Solutions and Inflation. |
Q59450913 | Extended inflation with a curvature-coupled inflaton |
Q59450916 | False vacuum inflation with Einstein gravity |
Q59450901 | False vacuum inflation with a quartic potential |
Q59450355 | Fitting BICEP2 with defects, primordial gravitational waves and dust |
Q59450919 | Formalizing the slow-roll approximation in inflation |
Q59450890 | Four-year COBE normalization of inflationary cosmologies |
Q58982256 | Galaxies in X-ray selected clusters and groups in Dark Energy Survey data. I. Stellar mass growth of bright central galaxies since z~1.2 |
Q59450956 | Hyperextended inflation: Dynamics and constraints |
Q59450905 | Inflation as the unique causal mechanism for generating density perturbations on scales well above the Hubble radius |
Q59450589 | Inflation, Dark Matter, and Dark Energy in the String Landscape |
Q57310182 | Information criteria for astrophysical model selection |
Q59450683 | Microwave background constraints on inflationary parameters |
Q59450935 | Modern cosmology |
Q59450992 | Neutron stars and extra dimensions |
Q59450467 | Non-Gaussianity in AxionN-flation Models |
Q59450939 | Observing the inflaton potential |
Q59450909 | Open universe Grishchuk-Zel’dovich effect |
Q59450942 | Perturbation spectra from intermediate inflation |
Q15217920 | Planck 2013 results. I. Overview of products and scientific results |
Q57549018 | Planck 2013 results. XX. Cosmology from Sunyaev–Zeldovich cluster counts |
Q57549031 | Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources |
Q57617347 | Planck 2013 results. XXXII. The updated Planck catalogue of Sunyaev-Zeldovich sources |
Q57549152 | Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates |
Q57549158 | Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample |
Q57549162 | Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations |
Q27019857 | Planck early results. XXVI. Detection with Planck and confirmation by XMM-Newton of PLCK G266.6–27.3, an exceptionally X-ray luminous and massive galaxy cluster at z ~ 1 |
Q57617377 | Planck intermediate results (Corrigendum) V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect |
Q57549112 | Planck intermediate results I. Further validation of new Planck clusters with XMM-Newton |
Q57549066 | Planck intermediate results II. Comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters |
Q57549067 | Planck intermediate results III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal |
Q57549070 | Planck intermediate results IV. The XMM-Newton validation programme for new Planck galaxy clusters |
Q57549076 | Planck intermediate results V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect |
Q57549048 | Planck intermediate results XVI. Profile likelihoods for cosmological parameters |
Q56039944 | Probing Inflation with CMB Polarization |
Q59450895 | Pursuing parameters for critical-density dark matter models |
Q59450944 | Reconstructing the inflaton potential: In principle and in practice |
Q59450921 | Reconstructing the inflaton potential: Perturbative reconstruction to second order |
Q17323608 | Review of Particle Physics |
Q53953395 | Review of Particle Physics |
Q54207951 | Review of Particle Physics |
Q59450924 | Second-order reconstruction of the inflationary potential |
Q59450800 | Sunyaev-Zel'dovich predictions for the Planck Surveyor satellite using the Hubble Volume simulations |
Q57821510 | Sunyaev-Zel’dovich clusters in Millennium gas simulations |
Q59450927 | Texture-induced microwave background anisotropies |
Q59733013 | The Dark Energy Survey: Data Release 1 |
Q59450819 | The Dearth of Halo Dwarf Galaxies: Is There Power on Short Scales? |
Q52394978 | The End for Extended Inflation? |
Q59450483 | The XMM cluster survey: the build-up of stellar mass in brightest cluster galaxies at high redshift |
Q59450969 | The cosmology of black hole relics |
Q59450801 | The effect of reionization on the COBE normalization |
Q59450571 | The evolution of clusters in the CLEF cosmological simulation: X-ray structural and scaling properties |
Q59450930 | The inflationary energy scale |
Q59450803 | The lepton asymmetry: the last chance for a critical-density cosmology? |
Q59450697 | The power spectrum amplitude from clusters revisited: 8 using simulations with pre-heating and cooling |
Q59450368 | The universe, darkly |
Q59450974 | There is a big-bubble problem in extended inflation |
Q59451001 | Topological defects in extended inflation |
Q59451005 | Vacuum instability near compact stars |
azb | اندرو آر لیدل | wikipedia |
Andrew R. Liddle | wikipedia | |
Persian (fa / Q9168) | اندرو آر لیدل | wikipedia |
Andrew Liddle | wikipedia | |
ta | ஆந்திரூ இலிடில் | wikipedia |
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