Andrew R. Liddle

British astrophysicist and cosmologist

DBpedia resource is: http://dbpedia.org/resource/Andrew_R._Liddle

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.

Born 1965-06-09 in Glasgow (Q4093)

Andrew R. Liddle is …
instance of (P31):
humanQ5

External links are
P4594arXiv author IDliddle_a_1
P8880AstroGen ID25325
P268Bibliothèque nationale de France ID14541396b
P7893CIÊNCIAVITAE IDC516-5189-350B
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P646Freebase ID/m/09ntfw
P227GND ID136952208
P9467IAU member ID1041
P269IdRef ID091448417
P2930INSPIRE-HEP author IDA.R.Liddle.1
P213ISNI0000000355613341
P244Library of Congress authority IDnr95006642
P5587Libris-URI64jln5jq5j524rm
P8189National Library of Israel J9U ID987007424314405171
P1006Nationale Thesaurus voor Auteursnamen ID195052927
P691NL CR AUT IDjo2012710542
P1695NLP ID (old)a0000001206617
P1015NORAF ID99021467
P1207NUKAT IDn00068507
P496ORCID iD0000-0002-8164-4830
P7293PLWABN ID9810661360305606
P1153Scopus author ID7006135719
P906SELIBR ID228442
P7671Semion author ID17632560
P3987SHARE Catalogue author ID65972
P10861Springer Nature person ID014705537145.53
P214VIAF ID74089833
P10832WorldCat Entities IDE39PBJxWMQ9gkK4chM4QRt6Frq
P1556zbMATH author IDliddle.andrew-r

P27country of citizenshipUnited KingdomQ145
P69educated atUniversity of GlasgowQ192775
P108employerUniversity of EdinburghQ160302
Imperial College LondonQ189022
University of GlasgowQ192775
University of LisbonQ1122926
University of SussexQ1161297
Perimeter Institute for Theoretical PhysicsQ2004561
P734family nameLiddleQ6543617
LiddleQ6543617
LiddleQ6543617
P735given nameAndrewQ18042461
AndrewQ18042461
P1412languages spoken, written or signedEnglishQ1860
P6104maintained by WikiProjectWikiProject MathematicsQ8487137
P463member ofInternational Astronomical UnionQ6867
P106occupationastronomerQ11063
physicistQ169470
P21sex or gendermaleQ6581097

Reverse relations

author (P50)
Q59450880Accurate determination of inflationary perturbations
Q59450490An evolutionary paradigm for dusty active galaxies at low redshift
Q59450779Apparent and actual galaxy cluster temperatures
Q59450977Baryogenesis in extended inflation. I. Baryogenesis via production and decay of supermassive bosons
Q59450981Baryogenesis in extended inflation. II. Baryogenesis via primordial black holes
Q59450395Bayesian model averaging in astrophysics: a review
Q59450911Can the gravitational wave background from inflation be detected locally?
Q51084903Can topological defects mimic the BICEP2 B-mode signal?
Q59450932Characteristics of unwinding textures
Q58916608Cold dark matter models with high baryon content
Q59450952Collapse of spherically symmetric textures
Q59450888Conditions for successful extended inflation
Q59450400Cosmic Microwave Background Anomalies in an Open Universe
Q59450532Cosmic microwave anisotropies from BPS semilocal strings
Q59450824Cosmic microwave background constraints on the epoch of reionization
Q59450586Cosmic reionization constraints on the nature of cosmological perturbations
Q59450839Cosmological parameter estimation and the spectral index from inflation
Q60908920Dark Energy Survey Year 1 Results: A Precise H0 Estimate from DES Y1, BAO, and D/H Data
Q44853455Early assembly of the most massive galaxies.
Q59450898Erratum: Can the gravitational wave background from inflation be detected locally? [Phys. Rev. D49, 3805 (1994)]
Q52394982Exponential Potentials, Scaling Solutions and Inflation.
Q59450913Extended inflation with a curvature-coupled inflaton
Q59450916False vacuum inflation with Einstein gravity
Q59450901False vacuum inflation with a quartic potential
Q59450355Fitting BICEP2 with defects, primordial gravitational waves and dust
Q59450919Formalizing the slow-roll approximation in inflation
Q59450890Four-year COBE normalization of inflationary cosmologies
Q58982256Galaxies in X-ray selected clusters and groups in Dark Energy Survey data. I. Stellar mass growth of bright central galaxies since z~1.2
Q59450956Hyperextended inflation: Dynamics and constraints
Q59450905Inflation as the unique causal mechanism for generating density perturbations on scales well above the Hubble radius
Q59450589Inflation, Dark Matter, and Dark Energy in the String Landscape
Q57310182Information criteria for astrophysical model selection
Q59450683Microwave background constraints on inflationary parameters
Q59450935Modern cosmology
Q59450992Neutron stars and extra dimensions
Q59450467Non-Gaussianity in AxionN-flation Models
Q59450939Observing the inflaton potential
Q59450909Open universe Grishchuk-Zel’dovich effect
Q59450942Perturbation spectra from intermediate inflation
Q15217920Planck 2013 results. I. Overview of products and scientific results
Q57549018Planck 2013 results. XX. Cosmology from Sunyaev–Zeldovich cluster counts
Q57549031Planck 2013 results. XXIX. The Planck catalogue of Sunyaev-Zeldovich sources
Q57617347Planck 2013 results. XXXII. The updated Planck catalogue of Sunyaev-Zeldovich sources
Q57549152Planck early results. IX. XMM-Newton follow-up for validation of Planck cluster candidates
Q57549158Planck early results. VIII. The all-sky early Sunyaev-Zeldovich cluster sample
Q57549162Planck early results. XI. Calibration of the local galaxy cluster Sunyaev-Zeldovich scaling relations
Q27019857Planck 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
Q57617377Planck intermediate results (Corrigendum) V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect
Q57549112Planck intermediate results I. Further validation of new Planck clusters with XMM-Newton
Q57549066Planck intermediate results II. Comparison of Sunyaev-Zeldovich measurements from Planck and from the Arcminute Microkelvin Imager for 11 galaxy clusters
Q57549067Planck intermediate results III. The relation between galaxy cluster mass and Sunyaev-Zeldovich signal
Q57549070Planck intermediate results IV. The XMM-Newton validation programme for new Planck galaxy clusters
Q57549076Planck intermediate results V. Pressure profiles of galaxy clusters from the Sunyaev-Zeldovich effect
Q57549048Planck intermediate results XVI. Profile likelihoods for cosmological parameters
Q56039944Probing Inflation with CMB Polarization
Q59450895Pursuing parameters for critical-density dark matter models
Q59450944Reconstructing the inflaton potential: In principle and in practice
Q59450921Reconstructing the inflaton potential: Perturbative reconstruction to second order
Q17323608Review of Particle Physics
Q53953395Review of Particle Physics
Q54207951Review of Particle Physics
Q59450924Second-order reconstruction of the inflationary potential
Q59450800Sunyaev-Zel'dovich predictions for the Planck Surveyor satellite using the Hubble Volume simulations
Q57821510Sunyaev-Zel’dovich clusters in Millennium gas simulations
Q59450927Texture-induced microwave background anisotropies
Q59733013The Dark Energy Survey: Data Release 1
Q59450819The Dearth of Halo Dwarf Galaxies: Is There Power on Short Scales?
Q52394978The End for Extended Inflation?
Q59450483The XMM cluster survey: the build-up of stellar mass in brightest cluster galaxies at high redshift
Q59450969The cosmology of black hole relics
Q59450801The effect of reionization on the COBE normalization
Q59450571The evolution of clusters in the CLEF cosmological simulation: X-ray structural and scaling properties
Q59450930The inflationary energy scale
Q59450803The lepton asymmetry: the last chance for a critical-density cosmology?
Q59450697The power spectrum amplitude from clusters revisited: 8 using simulations with pre-heating and cooling
Q59450368The universe, darkly
Q59450974There is a big-bubble problem in extended inflation
Q59451001Topological defects in extended inflation
Q59451005Vacuum instability near compact stars

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