Lucas Lombriser

Q: What Schools Are Affiliated With Lucas Lombriser

Lucas Lombriser is affiliated with the following schools: University of Edinburgh, University of Geneva, University of Zurich

Lucas Lombriser's AcademicInfluence.com Rankings

Lucas Lombriser

Physics

#7731

World Rank

#9783

Historical Rank

physics Degrees

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Physics

Lucas Lombriser's Degrees

PhD Physics University of Geneva
Masters Physics University of Geneva
Bachelors Physics University of Geneva

Why Is Lucas Lombriser Influential?

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According to Wikipedia, Lucas Lombriser is a Swiss National Science Foundation Professor at the Department of Theoretical Physics, University of Geneva. His research is in Theoretical Cosmology, Dark Energy, and Alternative Theories of Gravity. In 2020 and 2021 Lombriser proposed that the Hubble tension and other discrepancies between cosmological measurements imply significant evidence that we are living in a Hubble Bubble of 250 million light years in diameter which is 20% less dense than the cosmic average and lowers the locally measured cosmic microwave background temperature over its cosmic average. Previously, in 2019, he has proposed a solution to the cosmological constant problem from arguing that Newton's constant varies globally. In 2015 and 2016, Lombriser predicted the measurement of the gravitational wave speed with a neutron star merger and that this would rule out alternative theories of gravity as the cause of the late-time accelerated expansion of our Universe, a prediction that proved true with GW170817. Lombriser is a member of the Romansh-speaking minority in Switzerland.

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Lucas Lombriser's Published Works

Number of citations in a given year to any of this author's works

Total number of citations to an author for the works they published in a given year. This highlights publication of the most important work(s) by the author

Published Works

Breaking a dark degeneracy with gravitational waves (2015) (329)
Confirmation of general relativity on large scales from weak lensing and galaxy velocities (2010) (280)
Challenges to Self-Acceleration in Modified Gravity from Gravitational Waves and Large-Scale Structure (2016) (240)
Dark Energy vs. Modified Gravity (2016) (238)
The clustering of galaxies in the SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: testing deviations from Λ and general relativity using anisotropic clustering of galaxies (2012) (184)
Prospects for fundamental physics with LISA (2020) (183)
Testing general relativity with current cosmological data (2010) (141)
Testing modified gravity at cosmological distances with LISA standard sirens (2019) (139)
Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces (2016) (133)
Constraints on f(R) gravity from probing the large-scale structure (2010) (123)
Cluster density profiles as a test of modified gravity (2011) (100)
Testing chameleon gravity with the Coma cluster (2013) (85)
Cosmological Constraints on DGP Braneworld Gravity with Brane Tension (2009) (84)
Constraining chameleon models with cosmology (2014) (79)
Modeling halo mass functions in chameleon f(R) gravity (2013) (74)
Chameleon f(R) gravity in the virialized cluster (2012) (62)
Halo modelling in chameleon theories (2013) (61)
Relativistic effects in galaxy clustering in a parametrized post-Friedmann universe (2013) (57)
On the road to percent accuracy: non-linear reaction of the matter power spectrum to dark energy and modified gravity (2018) (55)
Halo model and halo properties in Galileon gravity cosmologies (2014) (54)
Finding Horndeski theories with Einstein gravity limits (2016) (52)
Cluster abundance in chameleon f(R) gravity I: toward an accurate halo mass function prediction (2016) (43)
On the cosmological constant problem (2019) (43)
New horizons for fundamental physics with LISA (2022) (35)
A parametrisation of modified gravity on nonlinear cosmological scales (2016) (34)
Reconstructing Horndeski theories from phenomenological modified gravity and dark energy models on cosmological scales (2018) (34)
Novel Probes Project: Tests of gravity on astrophysical scales (2019) (34)
KiDS-1000 Cosmology: Constraints beyond flat ΛCDM (2020) (34)
Unscreening Modified Gravity in the Matter Power Spectrum. (2015) (33)
Classifying linearly shielded modified gravity models in effective field theory. (2014) (31)
Consistency of the local Hubble constant with the cosmic microwave background (2019) (30)
Emulators for the nonlinear matter power spectrum beyond ΛCDM (2019) (28)
Semi-dynamical perturbations of unified dark energy (2015) (28)
Cosmology with the Laser Interferometer Space Antenna (2022) (27)
Limitations on Standard Sirens tests of gravity from screening (2019) (26)
EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade (2021) (26)
Dark degeneracy I: Dynamical or interacting dark energy? (2019) (23)
Rapid simulation rescaling from standard to modified gravity models (2014) (22)
N-body simulations for parametrized modified gravity (2020) (22)
Consistency check of {Lambda}CDM phenomenology (2011) (22)
On the road to per cent accuracy IV: ReACT – computing the non-linear power spectrum beyond ΛCDM (2020) (21)
Reconstructing Horndeski models from the effective field theory of dark energy (2017) (21)
Horndeski gravity and standard sirens (2020) (18)
Constraints on decaying early modified gravity from cosmological observations (2016) (15)
How chameleons core dwarfs with cusps (2014) (15)
Comparison of different approaches to the quasi-static approximation in Horndeski models (2020) (15)
Parameterised post-Newtonian expansion in screened regions (2017) (13)
Measuring the propagation speed of gravitational waves with LISA (2022) (13)
Scalar and tensor gravitational waves (2020) (13)
Inherently stable effective field theory for dark energy and modified gravity (2018) (12)
Local self-tuning mechanism for the cosmological constant (2020) (11)
Distinguishing cosmologies using the turn-around radius near galaxy clusters (2019) (11)
Is there another coincidence problem at the reionization epoch (2017) (10)
Easing cosmic tensions with an open and hotter universe (2020) (10)
Parameterised post-Newtonian formalism for the effective field theory of dark energy via screened reconstructed Horndeski theories (2020) (9)
Parametrizations for Tests of Gravity (2018) (9)
Modelling the matter bispectrum at small scales in modified gravity (2019) (9)
On the road to per cent accuracy – V. The non-linear power spectrum beyond ΛCDM with massive neutrinos and baryonic feedback (2021) (9)
Late-time acceleration by a residual cosmological constant from sequestering vacuum energy in ultimate collapsed structures (2018) (8)
Horndeski theories and beyond from higher dimensions (2020) (7)
Hybrid Pℓ(k): general, unified, non-linear matter power spectrum in redshift space (2019) (7)
Screening and degenerate kinetic self-acceleration from the nonlinear freedom of reconstructed Horndeski theories (2019) (7)
Horndeski and the Sirens (2019) (6)
On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos (2021) (5)
Exploring the self-tuning of the cosmological constant from Planck mass variation (2020) (5)
Euclid : Forecast constraints on consistency tests of the Λ CDM model (2021) (5)
Challenges to Self-Acceleration in Modified Gravity (2016) (4)
Positivity bounds on reconstructed Horndeski models (2020) (4)
The effect of screening mechanisms on black hole binary inspiral waveforms (2021) (4)
Euclid: Testing the Copernican principle with next-generation surveys (2022) (3)
Euclid: Forecast constraints on consistency tests of the LambdaCDM model (2021) (3)
Seeking new physics in cosmology with Bayesian neural networks: Dark energy and modified gravity (2020) (2)
Baryogenesis through asymmetric Hawking radiation from primordial black holes as dark matter (2020) (2)
Modelling the non-linear bispectrum in modified gravity (2019) (2)
Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity (2022) (2)
Scalar Čerenkov radiation from high-energy cosmic rays (2021) (1)
M ar 2 01 0 Constraints on f ( R ) gravity from probing the large-scale structure (2010) (0)
A pr 2 01 1 Constraints on f ( R ) gravity from probing the large-scale structure (2017) (0)
2 7 A pr 2 02 0 Prospects for Fundamental Physics with LISA (2020) (0)
C O ] 4 J an 2 01 5 Constraining chameleon models with cosmology (2015) (0)
New horizons for fundamental physics with LISA (2022) (0)
Confronting theories of gravity with large-scale structures (2011) (0)
Modeling and Testing Dark Energy and Gravity with Galaxy Cluster Data (2018) (0)
Deposited in DRO : 07 December 2016 Version of attached le : Accepted Version Peer-review status of attached (2017) (0)
Training and Test data for BaCoN (2020) (0)
C O ] 1 1 A pr 2 01 1 Consistency check of Λ CDM phenomenology (2011) (0)
Constraining Gravity at Large Scales with Clusters of Galaxies (2017) (0)
Deposited in DRO : 06 May 2014 Version of attached le : Other Peer-review status of attached (2015) (0)
Berezinski-Kosterlitz-Thouless Transition in Spin Systems (2006) (0)
0 Ju n 20 10 Testing General Relativity with Current Cosmological Data (2017) (0)
Deposited in DRO : 16 July 2019 Version of attached le : Accepted Version Peer-review status of attached (2019) (0)

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Other Resources About Lucas Lombriser

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What Schools Are Affiliated With Lucas Lombriser?

Lucas Lombriser is affiliated with the following schools:

Lucas Lombriser's Academic­Influence.com Rankings