Probing alternative theories of gravity with Planck
|
|
- Pearl Webster
- 5 years ago
- Views:
Transcription
1 Probing alternative theories of gravity with Planck Andrea Marchini Sapienza - University of Rome based on Updated constraints from the Planck experiment on modified gravity:prd88, In collaboration with V. Salvatelli January 16, 2014 Cosmology on the Beach 2014
2 Planck results The Planck experiment has provided new and precise measurements of CMB anisotropy. Angular scales covered up to multipole l The new data are in full agreement with the ΛCDM model......with some differences in the content of the Universe. 2 of 24 P. A. R. Ade et al. [ Planck Collaboration], arxiv: [astro-ph.co].
3 Tension with H 0 astrophysical measurements Discrepancy between H 0 measured by Planck compared with the values measured by independent cosmological probes. While systematics can be present, the discrepancy can be explained including new physical phenomena. The Planck determination of H 0 is model dependent. 3 of 24
4 Tension with H 0 astrophysical measurements Discrepancy between H 0 measured by Planck compared with the values measured by independent cosmological probes. While systematics can be present, the discrepancy can be explained including new physical phenomena. The Planck determination of H 0 is model dependent. 4 of 24
5 Anomalous lensing signal Planck+WP Planck+WP+BAO Planck+WP+HST A L scales the lensing power spectrum and modulates the lensing effect in the temperature power spectrum. Probability We expect A L = 1. There is an evidence for A L > A L A L = % c.l. A L = % c.l. A L = % c.l. 5 of 24
6 Hints of New Physics? How can we interpret the tensions? Systematic effects. Signature of New Physics. 6 of 24
7 Hints of New Physics? How can we interpret the tensions? Systematic effects. Signature of New Physics. The solution of the Planck tensions could arise from New Physics effects. We focus on: Alternative theories of gravity 6 of 24
8 The modern theory of gravitation General relativity is the theory of gravity The theory of gravitational fields, constructed on the basis of theory of relativity, is called general relativity. It was established by Einstein (and finally formulated by him 1915), and represents probably the most beautiful of all existing physical theories. Landau & Lifshits. The classical theory of fields. Vol. 2. GR has been tested directly in the Solar System in the weak-field limit. Indirect test in the same regime outside the Solar System from binary pulsar. Strong regime tests are missing and gravity is tested very poorly at the large scales. 7 of 24
9 Cosmology and General Relativity Can the success of ΛCDM be advocated as a clear confirmation that GR works properly at large scales? 8 of 24
10 Cosmology and general relativity Can the success of ΛCDM be advocated as a clear confirmation that GR works properly at large scales? Almost all theories of gravity admit the FLRW as solution of their field equations. Indeed cosmology could indicates that gravity is not exactly described by GR. 9 of 24 To explain the cosmic acceleration within the context of GR, one needs to introduce the dark energy, which is very exotic, comprises approximately 70% of the energy content of the universe, and is not detected in the laboratory.
11 Alternative theories of gravity: f (R) models Generalization of the Einstein-Hilbert action by making it more general function of the Ricci scalar. This choice leads to fourth-order field equations. Possible explanation for the observed late-time accelerating expansion of the Universe. General relativity f (R) S = d 4 x ( ) g f (R) 2κ + L m(ψ, g µν ) R µν 1 2 g µνr = κt µν 3H 2 = κ (ρ m + ρ rad ) 2Ḣ = κ ( ρ m ρ ) rad 10 of 24
12 Alternative theories of gravity: f (R) models Generalization of the Einstein-Hilbert action by making it more general function of the Ricci scalar. This choice leads to fourth-order field equations. Possible explanation for the observed late-time accelerating expansion of the Universe. f (R) theories S = d 4 x g ( ) f (R) 2κ + L m(ψ, g µν ) f R (R)R µν 1 2 f (R)g µν + (g µν µ ν ) f R (R) = κt µν 3f R (R)H 2 = κ (ρ m + ρ rad ) (f R(R)R f (R)) 3Hḟ R (R) 2f R (R)Ḣ = κ ( ρ m ρ rad) + f R (R) Hḟ R(R) 11 of 24
13 Parametrization Poisson and anisotropy equations for ΛCDM k 2 Ψ = 4πGa 2 {ρ + 3(ρ + P)σ} k 2 [Φ Ψ] = 12πGa 2 (ρ + P)σ 12 of 24
14 Parametrization Poisson and anisotropy equation for alternative theories of gravity k 2 Ψ = µ(a, k) 4πGa 2 {ρ + 3(ρ + P)σ} k 2 [Φ γ(a, k) Ψ] = µ(a, k) 12πGa 2 (ρ + P)σ The background evolution is fixed to ΛCDM but the evolution of matter perturbations can be different. Bertschinger-Zukin parametrization µ(a, k) = 1+β 1λ 2 1 k2 a s, γ(a, k) = 1+β 2λ 2 1+λ 2 1 k2 a s 2 k2 a s 1+λ 2 2 k2 a s (B. & Z., PRD 78, , 2008) The only free parameter for f (R) is λ 2 1. Usually it is expressed as the present length-scale in units of the horizon scale: B 0 = 2λ 2 1 H2 0 /c2. 13 of 24
15 Effect on the Cosmic Microwave Background 14 of 24
16 Constraints PLANCK PLANCK+BAO PLANCK+HST Parameters 68% limit 68% limit 68% limit Ω b h ± ± ± Ω ch ± ± ± θ ± ± ± τ ± ± ± n s ± ± ± log(10 10 A s) ± ± ± B 0 < (95% c.l.) < (95% c.l.) < (95% c.l.) Ω m ± ± ± Ω Λ ± ± ± z re 10.6 ± ± ± 1.1 H 0 [km/s/mpc] 69.1 ± ± ± 1.1 Age/Gyr ± ± ± f (R) models are not favored but we obtain an upper limit on B 0. f (R) theories alleviate the H 0 tension between Planck and HST. 15 of 24
17 Constraints: varying the lensing amplitude PLANCK PLANCK+BAO PLANCK+HST Parameters 68% limit 68% limit 68% limit Ω b h ± ± ± Ω ch ± ± ± θ ± ± ± τ ± ± ± n s ± ± ± log(10 10 A s) ± ± ± B 0 < (95% c.l.) < (95% c.l.) < (95% c.l.) A L Ω m ± ± ± Ω Λ ± ± ± z re 10.8 ± ± ± 1.1 H 0[km/s/Mpc] 68.7 ± ± ± 1.3 Age/Gyr ± ± ± The bimodal behavior of the B 0 posterior distribution appears for all the data sets combinations. In f (R) models A L is in much better agreement with one than in ΛCDM. 16 of 24
18 Conclusions Some tensions can arise comparing Planck results with others independent astrophysical probes. While the systematic effects can be important it is worth to investigate if this discrepancy can be explained by new physics. f (R) theories are compatible but not favored and we obtain a tight upper limit on the length-scale B 0. In this scenario the tensions are alleviated indicating that new physics can be a proper explanation. 17 of 24
19 fffff 18 of 24
20 Why the bimodality? 19 of 24
21 Why the bimodality? Varying A L has the same effect of varying B 0 at the high multipoles. At low multipoles instead increasing B 0 lowers the integrated Sachs-Wolfe effect plateau, contrary to the effect of an increased H 0 value. This favors the match between theory and data even in presence of large H 0 values. The competition between these effects creates the local maximum in the posterior distribution. 19 of 24
22 Conformal transformation We can perform the conformal transformation g µν = e 2β κφ g E µν. We can recast f (R) theories as GR with a scalar field coupled to the matter sector. Action in the Einstein frame S = d 4 x ( ) g E R E 2κ 3 g E β µν µ φ ν φ V (φ) + L 2 m (ψ, e 2β κφ gµν) E V (φ) = Rf R (R) f (R) 2κf 2 R (R) The theory is well-defined as long as V (φ) is bounded from below. The scalar field is defined as φ 1 2β κ ln f R(R). The coupling for f (R) theories is β = 1 6 to obtain a canonical kinetic term (in general f R (R) > 0 to avoid ghost). 20 of 24
23 Coupling with matter The mass of the scalar for viable model is m 0 H Gev. L = κβφm ψ0 ψψ δφ N = 2β 2 G Nm 2 ψ0 r Constrained by Cassini measurements: β (B. Bertotti, L. Iess, and P. Tortora, Nature 425 (2003) 374) f (R) theories violate this condition. Screening mechanisms: chameleons, dilatons, symmetrons, of 24
24 B 0 vs Ω c h 2 and B 0 vs H 0 PLANCK PLANCK+HST PLANCK+BAO Ω c h B 0 H B 0 22 of 24
25 B 0 vs A L PLANCK PLANCK+HST PLANCK+BAO 23 of 24
26 Effect of the potentials 24 of 24
Planck results (1 st release)
General Introduction Planck results (1 st release) From Planck Collaboration.XVI. 2014 Standard cosmological model in good agreement with data but Valentina Salvatelli Interacting Dark Energy in light
More informationarxiv: v1 [astro-ph.co] 8 Jul 2013
Updated constraints from the PLANCK experiment on modified gravity Andrea Marchini 1 and Valentina Salvatelli 1 1 Physics Department and INFN, Università di Roma La Sapienza, Ple Aldo Moro 2, 00185, Rome,
More informationConstraining Modified Gravity and Coupled Dark Energy with Future Observations Matteo Martinelli
Coupled Dark University of Rome La Sapienza Roma, October 28th 2011 Outline 1 2 3 4 5 1 2 3 4 5 Accelerated Expansion Cosmological data agree with an accelerated expansion of the Universe d L [Mpc] 16000
More informationThe dilaton and modified gravity
The dilaton and modified gravity Carsten van de Bruck University of Sheffield Work in collaboration with P. Brax, A. Davis and D. Shaw arxiv:1005.3735 Scalar Fields and Modified Gravity Scalar fields are
More informationAttractor Structure of Gauged Nambu-Jona-Lasinio Model
Attractor Structure of Gauged ambu-jona-lasinio Model Department of Physics, Hiroshima University E-mail: h-sakamoto@hiroshima-u.ac.jp We have studied the inflation theory in the gauged ambu-jona-lasinio
More informationTo Lambda or not to Lambda?
To Lambda or not to Lambda? Supratik Pal Indian Statistical Institute Kolkata October 17, 2015 Conclusion We don t know :) Partly based on my works with Dhiraj Hazra, Subha Majumdar, Sudhakar Panda, Anjan
More informationConstraints on the deviations from general relativity
14/10/2010 Minneapolis Constraints on the deviations from general relativity From local to cosmological scales Jean-Philippe UZAN GR in a nutshell Underlying hypothesis Equivalence principle Universality
More informationThe Influence of DE on the Expansion Rate of the Universe and its Effects on DM Relic Abundance
The Influence of DE on the Expansion Rate of the Universe and its Effects on DM Relic Abundance Esteban Jimenez Texas A&M University XI International Conference on Interconnections Between Particle Physics
More informationTESTING GRAVITY WITH COSMOLOGY
21 IV. TESTING GRAVITY WITH COSMOLOGY We now turn to the different ways with which cosmological observations can constrain modified gravity models. We have already seen that Solar System tests provide
More informationwith EFTCAMB: The Hořava gravity case
Testing dark energy and modified gravity models with EFTCAMB: The Hořava gravity case Noemi Frusciante UPMC-CNRS, Institut d Astrophysique de Paris, Paris ERC-NIRG project no.307934 Based on NF, M. Raveri,
More informationD. f(r) gravity. φ = 1 + f R (R). (48)
5 D. f(r) gravity f(r) gravity is the first modified gravity model proposed as an alternative explanation for the accelerated expansion of the Universe [9]. We write the gravitational action as S = d 4
More informationDark Energy. RESCEU APcosPA Summer School on Cosmology and Particle Astrophysics Matsumoto city, Nagano. July 31 - August
RESCEU APcosPA Summer School on Cosmology and Particle Astrophysics Matsumoto city, Nagano LCC, Université Montpellier 2 July 31 - August 4 2014 More : Friedmann-Lemaître-Robertson-Walker (FLRW) universes:
More informationGalileon Cosmology ASTR448 final project. Yin Li December 2012
Galileon Cosmology ASTR448 final project Yin Li December 2012 Outline Theory Why modified gravity? Ostrogradski, Horndeski and scalar-tensor gravity; Galileon gravity as generalized DGP; Galileon in Minkowski
More informationDark Energy and Dark Matter Interaction. f (R) A Worked Example. Wayne Hu Florence, February 2009
Dark Energy and Dark Matter Interaction f (R) A Worked Example Wayne Hu Florence, February 2009 Why Study f(r)? Cosmic acceleration, like the cosmological constant, can either be viewed as arising from
More informationExperimental Tests and Alternative Theories of Gravity
Experimental Tests and Alternative Theories of Gravity Gonzalo J. Olmo Alba gonzalo.olmo@uv.es University of Valencia (Spain) & UW-Milwaukee Experimental Tests and Alternative Theories of Gravity p. 1/2
More informationCosmic Acceleration from Modified Gravity: f (R) A Worked Example. Wayne Hu
Cosmic Acceleration from Modified Gravity: f (R) A Worked Example Wayne Hu CalTech, December 2008 Why Study f(r)? Cosmic acceleration, like the cosmological constant, can either be viewed as arising from
More informationModified gravity. Kazuya Koyama ICG, University of Portsmouth
Modified gravity Kazuya Koyama ICG, University of Portsmouth Cosmic acceleration Cosmic acceleration Big surprise in cosmology Simplest best fit model LCDM 4D general relativity + cosmological const. H
More informationCONSTRAINTS AND TENSIONS IN MG CFHTLENS AND OTHER DATA SETS PARAMETERS FROM PLANCK, INCLUDING INTRINSIC ALIGNMENTS SYSTEMATICS. arxiv:1501.
CONSTRAINTS AND TENSIONS IN MG PARAMETERS FROM PLANCK, CFHTLENS AND OTHER DATA SETS INCLUDING INTRINSIC ALIGNMENTS SYSTEMATICS arxiv:1501.03119 1 Mustapha Ishak The University of Texas at Dallas Jason
More informationCONSTRAINTS AND TENSIONS IN MG CFHTLENS AND OTHER DATA SETS PARAMETERS FROM PLANCK, INCLUDING INTRINSIC ALIGNMENTS SYSTEMATICS.
CONSTRAINTS AND TENSIONS IN MG PARAMETERS FROM PLANCK, CFHTLENS AND OTHER DATA SETS INCLUDING INTRINSIC ALIGNMENTS SYSTEMATICS 1 Mustapha Ishak The University of Texas at Dallas Jason Dossett INAF Osservatorio
More informationModified Gravity (MOG) and Dark Matter: Can Dark Matter be Detected in the Present Universe?
Modified Gravity (MOG) and Dark Matter: Can Dark Matter be Detected in the Present Universe? John Moffat Perimeter Institute, Waterloo, Ontario, Canada Talk given at the Miami 2014 topical conference on
More informationThe Once and Future CMB
The Once and Future CMB DOE, Jan. 2002 Wayne Hu The On(c)e Ring Original Power Spectra of Maps 64º Band Filtered Ringing in the New Cosmology Gravitational Ringing Potential wells = inflationary seeds
More informationChallenges in Cosmology and why (may be) Modified Gravity
Challenges in Cosmology and why (may be) Modified Gravity David F. Mota Institute for Research in Fundamental Sciences IPM-Teheran 2016 Two Pillars in Cosmology Understanding the Universe and its laws
More informationInflationary cosmology from higher-derivative gravity
Inflationary cosmology from higher-derivative gravity Sergey D. Odintsov ICREA and IEEC/ICE, Barcelona April 2015 REFERENCES R. Myrzakulov, S. Odintsov and L. Sebastiani, Inflationary universe from higher-derivative
More informationSMALL COSMOLOGICAL CONSTANT FROM RUNNING GRAVITATIONAL COUPLING
SMALL COSMOLOGICAL CONSTANT FROM RUNNING GRAVITATIONAL COUPLING arxiv:1101.4995, arxiv:0803.2500 Andrei Frolov Department of Physics Simon Fraser University Jun-Qi Guo (SFU) Sternberg Astronomical Institute
More informationDark Energy & General Relativity «Some theoretical thoughts»
IAS workshop 24/11/2008 Dark Energy & General Relativity «Some theoretical thoughts» Jean-Philippe UZAN Cosmological models Theoretical physics Principles Local law of nature Extrapolations Cosmology models
More informationThe Theory of Inflationary Perturbations
The Theory of Inflationary Perturbations Jérôme Martin Institut d Astrophysique de Paris (IAP) Indian Institute of Technology, Chennai 03/02/2012 1 Introduction Outline A brief description of inflation
More informationDark Energy to Modified Gravity
Dark Energy to Modified Gravity Philippe Brax IPhT Saclay Workshop Invisibles July 2014 Paris The Big Puzzle Acceleration of the expansion Dark Energy? Modified gravity on large enough scales? The acceleration
More informationCosmological Tests of Gravity
Cosmological Tests of Gravity Levon Pogosian Simon Fraser University, Canada VIA Lecture, 16 May, 2014 Workshop on Testing Gravity at SFU Harbour Centre January 15-17, 2015 Alternative theories of gravity
More informationGravitational waves, solitons, and causality in modified gravity
Gravitational waves, solitons, and causality in modified gravity Arthur Suvorov University of Melbourne December 14, 2017 1 of 14 General ideas of causality Causality as a hand wave Two events are causally
More informationParameterizing. Modified Gravity. Models of Cosmic Acceleration. Wayne Hu Ann Arbor, May 2008
Parameterizing Modified Gravity Models of Cosmic Acceleration Wayne Hu Ann Arbor, May 2008 Parameterizing Acceleration Cosmic acceleration, like the cosmological constant, can either be viewed as arising
More informationA Panorama of Modified Gravity. Philippe Brax IPhT Saclay
A Panorama of Modified Gravity Philippe Brax IPhT Saclay The Universe accelerates: why? Maybe a landscape of Universes? Or not? The acceleration of the Universe could also be due to many mundane causes:
More informationModifications of gravity induced by abnormally weighting dark matter
Modifications of gravity induced by abnormally weighting dark matter André Füzfa NAXYS & CP3 University of Namur-Louvain (Belgium) in collaboration with J.-M. Alimi (Obs. Paris), B. Famaey (Obs. Strasbourg),
More informationCosmological perturbations in f(r) theories
5 th IBERIAN COSMOLOGY MEETING 30 th March 2010, Porto, Portugal Cosmological perturbations in f(r) theories Álvaro de la Cruz-Dombriz Theoretical Physics Department Complutense University of Madrid in
More informationGalaxies 626. Lecture 3: From the CMBR to the first star
Galaxies 626 Lecture 3: From the CMBR to the first star Galaxies 626 Firstly, some very brief cosmology for background and notation: Summary: Foundations of Cosmology 1. Universe is homogenous and isotropic
More informationDark Forces and the ISW Effect
Dark Forces and the ISW Effect Finn Ravndal, University of Oslo Introduction Chaplygin gases Cardassian fluids The integrated Sachs-Wolfe effect Demise of unified dark models Modified gravity: A resurrection?
More informationCosmology in generalized Proca theories
3-rd Korea-Japan workshop on dark energy, April, 2016 Cosmology in generalized Proca theories Shinji Tsujikawa (Tokyo University of Science) Collaboration with A.De Felice, L.Heisenberg, R.Kase, S.Mukohyama,
More informationNon-linear structure formation in modified gravity
Non-linear structure formation in modified gravity Kazuya Koyama Institute of Cosmology and Gravitation, University of Portsmouth Cosmic acceleration Many independent data sets indicate the expansion of
More informationGravitational waves from the early Universe
Gravitational waves from the early Universe Part 1 Sachiko Kuroyanagi (Nagoya University) 26 Aug 2017 Summer Institute 2017 What is a Gravitational Wave? What is a Gravitational Wave? 11 Feb 2016 We have
More informationModified Theories of Gravity in Cosmology
Modified Theories of Gravity in Cosmology Gonzalo J. Olmo University of Wisconsin-Milwaukee (USA) Gonzalo J. Olmo About this talk... Motivation: General Relativity by itself seems unable to justify the
More informationEffective Field Theory approach for Dark Energy/ Modified Gravity. Bin HU BNU
Effective Field Theory approach for Dark Energy/ Modified Gravity Bin HU BNU NAOC Nov. 2016 Outline 1. Evidence of late-time cosmic acceleration 2. Effective Field Theory approach for DE/MG 3. The structure
More informationExamining the Viability of Phantom Dark Energy
Examining the Viability of Phantom Dark Energy Kevin J. Ludwick LaGrange College 11/12/16 Kevin J. Ludwick (LaGrange College) Examining the Viability of Phantom Dark Energy 11/12/16 1 / 28 Outline 1 Overview
More informationThermal Axion Cosmology
Thermal Axion Cosmology 19th June 2015, Santander Eleonora Di Valentino Institut d Astrophysique de Paris Axions The most elegant and promising solution of the so-called strong CP problem in Quantum Chromodynamics
More informationTesting Gravity Cosmologically
Testing Gravity Cosmologically Philippe Brax IPhT Saclay Asphon Toulouse March 2013 The Big Puzzle How do we know? measuring distances! Absolute luminosity. Received flux: what we see in the telescope
More informationExamining the Viability of Phantom Dark Energy
Examining the Viability of Phantom Dark Energy Kevin J. Ludwick LaGrange College 12/20/15 (11:00-11:30) Kevin J. Ludwick (LaGrange College) Examining the Viability of Phantom Dark Energy 12/20/15 (11:00-11:30)
More informationEquation of state of dark energy. Phys. Rev. D 91, (2015)
Equation of state of dark energy in f R gravity The University of Tokyo, RESCEU K. Takahashi, J. Yokoyama Phys. Rev. D 91, 084060 (2015) Motivation Many modified theories of gravity have been considered
More informationTesting parity violation with the CMB
Testing parity violation with the CMB Paolo Natoli Università di Ferrara (thanks to Alessandro Gruppuso)! ISSS L Aquila 24 April 2014 Introduction The aim is to use observed properties of CMB pattern to
More informationModified gravity as an alternative to dark energy. Lecture 3. Observational tests of MG models
Modified gravity as an alternative to dark energy Lecture 3. Observational tests of MG models Observational tests Assume that we manage to construct a model How well can we test the model and distinguish
More informationA brief introduction to modified theories of gravity
(Vinc)Enzo Vitagliano CENTRA, Lisboa May, 14th 2015 IV Amazonian Workshop on Black Holes and Analogue Models of Gravity Belém do Pará The General Theory of Relativity dynamics of the Universe behavior
More informationVasiliki A. Mitsou. IFIC Valencia TAUP International Conference on Topics in Astroparticle and Underground Physics
Vasiliki A. Mitsou IFIC Valencia TAUP 2009 International Conference on Topics in Astroparticle and Underground Physics Rome, Italy, 1-5 July 2009 Dark energy models CDM Super-horizon CDM (SHCDM) [Kolb,
More informationInflation in a general reionization scenario
Cosmology on the beach, Puerto Vallarta,, Mexico 13/01/2011 Inflation in a general reionization scenario Stefania Pandolfi, University of Rome La Sapienza Harrison-Zel dovich primordial spectrum is consistent
More informationCosmological parameters of modified gravity
Cosmological parameters of modified gravity Levon Pogosian Simon Fraser University Burnaby, BC, Canada In collaborations with R. Crittenden, A. Hojjati, K. Koyama, A. Silvestri, G.-B. Zhao Two questions
More informationAdvantages and unexpected shortcomings of extended theories of gravity
Institute of Theoretical Physics, Heidelberg June 17 2015 Advantages and unexpected shortcomings of extended theories of gravity Álvaro de la Cruz-Dombriz Collaborators: J. Beltrán, V. Busti, P. K. S.
More informationThe State of Tension Between the CMB and LSS
The State of Tension Between the CMB and LSS Tom Charnock 1 in collaboration with Adam Moss 1 and Richard Battye 2 Phys.Rev. D91 (2015) 10, 103508 1 Particle Theory Group University of Nottingham 2 Jodrell
More informationIntroduction to hi class
CLASSy Tests of Gravity and Dark Energy Nordic Institute for Theoretical Physics and UC Berkeley Cosmology in Theory and Practice September 2017 Fundamental physics and cosmology Initial conditions, Dark
More informationCosmological and astrophysical applications of vector-tensor theories
Cosmological and astrophysical applications of vector-tensor theories Shinji Tsujikawa (Tokyo University of Science) Collaboration with A.De Felice, L.Heisenberg, R.Kase, M.Minamitsuji, S.Mukohyama, S.
More informationScale symmetry a link from quantum gravity to cosmology
Scale symmetry a link from quantum gravity to cosmology scale symmetry fluctuations induce running couplings violation of scale symmetry well known in QCD or standard model Fixed Points Quantum scale symmetry
More informationEl Universo en Expansion. Juan García-Bellido Inst. Física Teórica UAM Benasque, 12 Julio 2004
El Universo en Expansion Juan García-Bellido Inst. Física Teórica UAM Benasque, 12 Julio 2004 5 billion years (you are here) Space is Homogeneous and Isotropic General Relativity An Expanding Universe
More informationarxiv: v2 [gr-qc] 28 Nov 2018
Can Inflation Solve The Cosmological Constant Problem? Yousef Bisabr arxiv:1711.06582v2 [gr-qc] 28 Nov 2018 Department of Physics, Shahid Rajaee Teacher Training University, Lavizan, Tehran 16788, Iran
More informationThermodynamics of f(r) Gravity with the Disformal Transformation
Thermodynamics of f(r) Gravity with the Disformal Transformation Jhih-Rong Lu National Tsing Hua University(NTHU) Collaborators: Chao-Qiang Geng(NCTS, NTHU), Wei-Cheng Hsu(NTHU), Ling-Wei Luo(AS) Outline
More informationBeyond ΛCDM: Dark energy vs Modified Gravity
Beyond ΛCDM: Dark energy vs Modified Gravity Bhuvnesh Jain University of Pennsylvania References BJ et al, arxiv:1309.5389 (Snowmass) Joyce, BJ, Khoury, Trodden, arxiv:1407.0059 (Review) Cosmology probes:
More informationAstrophysical observations preferring Modified Gravity
Astrophysical observations preferring Modified Gravity A natural approach to extended Newtonian gravity: tests and predictions across astrophysical scales. Mon.Not.Roy.Astron.Soc. 411 (2011) 226-234 Wide
More informationPrimordial gravitational waves detected? Atsushi Taruya
21 May 2014 Lunch seminar @YITP Primordial gravitational waves detected? Atsushi Taruya Contents Searching for primordial gravitational waves from cosmic microwave background polarizations Gravitational-wave
More information2 Post-Keplerian Timing Parameters for General Relativity
1 Introduction General Relativity has been one of the pilars of modern physics for over 100 years now. Testing the theory and its consequences is therefore very important to solidifying our understand
More informationDetermining neutrino masses from cosmology
Determining neutrino masses from cosmology Yvonne Y. Y. Wong The University of New South Wales Sydney, Australia NuFact 2013, Beijing, August 19 24, 2013 The cosmic neutrino background... Embedding the
More informationFirst Cosmology Results from Planck. Alessandro Melchiorri University of Rome La Sapienza On behalf of the Planck collaboration
First Cosmology Results from Planck Alessandro Melchiorri University of Rome La Sapienza On behalf of the Planck collaboration Planck Collaboration 300+ names Planck Core-Team (a fraction of it) Planck
More informationA Unified Description of Screened Modified Gravity
A Unified Description of Screened Modified Gravity Philippe Brax IPhT Saclay P.B,C. van de Bruck, A.C. Davis, B. Li, H. Winther, G. Zhao etc «Microscope» workshop, ONERA January 2013 Outline 1) Dark energy
More informationCHAPTER 4 INFLATIONARY MODEL BUILDING. 4.1 Canonical scalar field dynamics. Non-minimal coupling and f(r) theories
CHAPTER 4 INFLATIONARY MODEL BUILDING Essentially, all models are wrong, but some are useful. George E. P. Box, 1987 As we learnt in the previous chapter, inflation is not a model, but rather a paradigm
More informationA Panorama of Modified Gravity. Philippe Brax IPhT Saclay (associate researcher IAP)
A Panorama of Modified Gravity Philippe Brax IPhT Saclay (associate researcher IAP) The Universe accelerates: why? Maybe a landscape of Universes? Or not? The acceleration of the Universe could also be
More informationProbing gravity theory and cosmic acceleration using (in)consistency tests between cosmological data sets
Probing gravity theory and cosmic acceleration using (in)consistency tests between cosmological data sets Prof. Mustapha Ishak Cosmology and Astrophysics Group The University of Texas at Dallas work done
More informationCosmic Acceleration from Modified Gravity:
Cosmic Acceleration from Modified Gravity: Lessons from Worked Examples Wayne Hu II Workshop Challenges Campos do Jordao, December 2009 Outline Three Regimes of Modified Gravity Horizon scale - acceleration
More informationN-body Simulations and Dark energy
N-Body Simulations and models of Dark Energy Elise Jennings Supported by a Marie Curie Early Stage Training Fellowship N-body Simulations and Dark energy elise jennings Introduction N-Body simulations
More informationUNIVERSITY OF OSLO Faculty of Mathematics and Natural Sciences
UNIVERSITY OF OSLO Faculty of Mathematics and Natural Sciences Exam for AST5220 Cosmology II Date: Tuesday, June 4th, 2013 Time: 09.00 13.00 The exam set consists of 13 pages. Appendix: Equation summary
More informationHighlights from Planck 2013 cosmological results Paolo Natoli Università di Ferrara and ASI/ASDC DSU2013, Sissa, 17 October 2013
Highlights from Planck 2013 cosmological results Paolo Natoli Università di Ferrara and ASI/ASDC DSU2013, Sissa, 17 October 2013 On behalf of the Planck collaboration Fluctuation and GW generator Fluctuation
More informationIs Cosmic Acceleration Telling Us Something About Gravity?
Is Cosmic Acceleration Telling Us Something About Gravity? Mark Trodden Syracuse University [See many other talks at this meeting; particularly talks by Carroll, Dvali, Deffayet,... ] NASA Meeting: From
More informationThe Early Universe John Peacock ESA Cosmic Vision Paris, Sept 2004
The Early Universe John Peacock ESA Cosmic Vision Paris, Sept 2004 The history of modern cosmology 1917 Static via cosmological constant? (Einstein) 1917 Expansion (Slipher) 1952 Big Bang criticism (Hoyle)
More information1 Introduction. 1.1 Notations and conventions
The derivation of the coupling constant in the new Self Creation Cosmology Garth A Barber The Vicarage, Woodland Way, Tadworth, Surrey, England KT206NW Tel: +44 01737 832164 e-mail: garth.barber@virgin.net
More informationDilaton gravity at the brane with general matter-dilaton coupling
Dilaton gravity at the brane with general matter-dilaton coupling University of Würzburg, Institute for Theoretical Physics and Astrophysics Bielefeld, 6. Kosmologietag May 5th, 2011 Outline introduction
More informationarxiv: v2 [astro-ph.co] 6 Dec 2013
arxiv:1308.1019v [astro-ph.co] 6 Dec 013 Variable gravity Universe C. Wetterich Institut für Theoretische Physik Universität Heidelberg Philosophenweg 16, D-6910 Heidelberg For variable gravity models
More informationCMB Polarization in Einstein-Aether Theory
CMB Polarization in Einstein-Aether Theory Masahiro Nakashima (The Univ. of Tokyo, RESCEU) With Tsutomu Kobayashi (RESCEU) COSMO/CosPa 2010 Introduction Two Big Mysteries of Cosmology Dark Energy & Dark
More informationConsistent Parameterization of Modified Gravity
arxiv 1107.0491 Consistent Parameterization of Modified Gravity Tessa Baker Oxford University Outline The Parameterized Post-Friedmann form. An alternative construction for modified gravity. Hidden assumptions
More informationAstro 448 Lecture Notes Set 1 Wayne Hu
Astro 448 Lecture Notes Set 1 Wayne Hu Recombination Equilibrium number density distribution of a non-relativistic species n i = g i ( mi T 2π ) 3/2 e m i/t Apply to the e + p H system: Saha Equation n
More informationTesting vector-tensor gravity with current cosmological observations
Journal of Physics: Conference Series PAPER OPEN ACCESS Testing vector-tensor gravity with current cosmological observations To cite this article: Roberto Dale and Diego Sáe 15 J. Phys.: Conf. Ser. 1 View
More informationTheoretical Models of the Brans-Dicke Parameter for Time Independent Deceleration Parameters
Theoretical Models of the Brans-Dicke Parameter for Time Independent Deceleration Parameters Sudipto Roy 1, Soumyadip Chowdhury 2 1 Assistant Professor, Department of Physics, St. Xavier s College, Kolkata,
More informationCosmology: An Introduction. Eung Jin Chun
Cosmology: An Introduction Eung Jin Chun Cosmology Hot Big Bang + Inflation. Theory of the evolution of the Universe described by General relativity (spacetime) Thermodynamics, Particle/nuclear physics
More informationThe ultimate measurement of the CMB temperature anisotropy field UNVEILING THE CMB SKY
The ultimate measurement of the CMB temperature anisotropy field UNVEILING THE CMB SKY PARAMETRIC MODEL 16 spectra in total C(θ) = CMB theoretical spectra plus physically motivated templates for the
More informationDark Energy at the Speed of Gravitational Waves
New probes of gravity and cosmic acceleration Nordita & BCCP Theoretical Cosmology in the Light of Data - July 2017 with A. Barreira, F. Montanari, J. Renk (1707.xxxxx) D. Bettoni, JM Ezquiaga, K. Hinterbichler
More informationLecture 09. The Cosmic Microwave Background. Part II Features of the Angular Power Spectrum
The Cosmic Microwave Background Part II Features of the Angular Power Spectrum Angular Power Spectrum Recall the angular power spectrum Peak at l=200 corresponds to 1o structure Exactly the horizon distance
More informationarxiv: v2 [astro-ph.co] 3 Sep 2014
Releasing scalar fields: cosmological simulations of scalar-tensor theories for gravity beyond the static approximation Claudio Llinares and David F. Mota Institute of Theoretical Astrophysics, University
More informationModified Gravity and Cosmology
Modified Gravity and Cosmology Kazuya Koyama Institute of Cosmology and Gravitation, University of Portsmouth Cosmic acceleration Many independent data sets indicate the expansion of the Universe is accelerating
More informationThe nonlinear dynamical stability of infrared modifications of gravity
The nonlinear dynamical stability of infrared modifications of gravity Aug 2014 In collaboration with Richard Brito, Vitor Cardoso and Matthew Johnson Why Study Modifications to Gravity? General relativity
More informationModern Cosmology / Scott Dodelson Contents
Modern Cosmology / Scott Dodelson Contents The Standard Model and Beyond p. 1 The Expanding Universe p. 1 The Hubble Diagram p. 7 Big Bang Nucleosynthesis p. 9 The Cosmic Microwave Background p. 13 Beyond
More informationEFTCAMB: exploring Large Scale Structure observables with viable dark energy and modified gravity models
EFTCAMB: exploring Large Scale Structure observables with viable dark energy and modified gravity models Noemi Frusciante Instituto de Astrofísica e Ciências do Espaço, Faculdade de Ciências da Universidade
More informationGeneral Relativistic N-body Simulations of Cosmic Large-Scale Structure. Julian Adamek
General Relativistic N-body Simulations of Cosmic Large-Scale Structure Julian Adamek General Relativistic effects in cosmological large-scale structure, Sexten, 19. July 2018 Gravity The Newtonian limit
More informationA Framework for. Modified Gravity. Models of Cosmic Acceleration. Wayne Hu EFI, November 2008
A Framework for Modified Gravity Models of Cosmic Acceleration Wayne Hu EFI, November 2008 Candidates for Acceleration Cosmological constant (cold dark matter) model ΛCDM is the standard model of cosmology
More informationInstabilities during Einstein-Aether Inflation
Instabilities during Einstein-Aether Inflation Adam R Solomon DAMTP, University of Cambridge, UK Based on work to appear soon: AS & John D Barrow arxiv:1309.xxxx September 3 rd, 2013 Why consider Lorentz
More informationTesting Lorentz invariance of Dark matter with cosmological data
Testing Lorentz invariance of Dark matter with cosmological data Mikhail Ivanov in collaboration with B. Audren, D. Blas, J.Lesgourges and S. Sibiryakov based on JCAP 10 (2012) 057 [arxiv:1209.0464] arxiv:1212.xxxx
More informationFuture precision cosmology and neutrinos
Future precision cosmology and neutrinos Universitá di Roma Sapienza, Ple Aldo Moro 2, 00185, Rome, Italy E-mail: alessandro.melchiorri@uniroma1.it In the next decade future measurements of the Cosmic
More informationPossible Connections in Colliders, Dark Matter, and Dark Energy
Possible Connections in Colliders, Dark Matter, and Dark Energy 0704.3285 [hep-ph] 0706.2375 [hep-ph] Daniel Chung (U. Wisconsin Madison) Collaborators: L. Everett, K. Kong, K. Matchev Quiz Which of the
More informationCan kinetic Sunyaev-Zel dovich effect be used to detect the interaction between DE and DM? Bin Wang Shanghai Jiao Tong University
Can kinetic Sunyaev-Zel dovich effect be used to detect the interaction between DE and DM? Bin Wang Shanghai Jiao Tong University Outline: The interaction model between DE&DM The ISW effect as a probe
More informationUNIVERSITÁ DEGLI STUDI DI PARMA Dottorato di Ricerca in Fisica Ciclo XXVII. Observational Constraints on Modified Gravity Models
UNIVERSITÁ DEGLI STUDI DI PARMA Dottorato di Ricerca in Fisica Ciclo XXVII Observational Constraints on Modified Gravity Models COORDINATORE: Prof. CRISTIANO VIAPPIANI TUTORS: Prof. MASSIMO PIETRONI Dott.
More information