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|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
2206.09000 | Giovanni Otalora | Yoelsy Leyva and Giovanni Otalora | Revisiting $f(R)$ gravity's rainbow: Inflation and primordial
fluctuations | 18 pages, 4 figures. Updated to match the published version in JCAP | JCAP 04 (2023) 030 | 10.1088/1475-7516/2023/04/030 | null | gr-qc astro-ph.CO hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " We study inflation and the generation of primordial fluctuations in $f(R)$\ngravity's rainbow. We(...TRUNCATED) | [{"created":"Fri, 17 Jun 2022 20:43:06 GMT","version":"v1"},{"created":"Wed, 12 Apr 2023 14:41:57 GM(...TRUNCATED) | 2023-04-13 | [
[
"Leyva",
"Yoelsy",
""
],
[
"Otalora",
"Giovanni",
""
]
] | "We study inflation and the generation of primordial fluctuations in $f(R)$ gravity's rainbow. We ca(...TRUNCATED) | "We study inflation and the generation of primordial fluctuations in $f(R)$ gravity's rainbow. We ca(...TRUNCATED) | "We contrast the predictions of the model with the current observational data from PLANCK and BICEP/(...TRUNCATED) | "We study inflation and the generation of primordial fluctuations in $f(R)$ gravity's rainbow. We ca(...TRUNCATED) | " We find that the rainbow functions can play a significant role in the evolution of the perturbatio(...TRUNCATED) | "We study inflation and the generation of primordial fluctuations in $f(R)$ gravity's rainbow. We ca(...TRUNCATED) | We find that in this model, the tensor power spectrum is modified. | "We study inflation and the generation of primordial fluctuations in $f(R)$ gravity's rainbow. We ca(...TRUNCATED) | " We find that the power spectrum is red-tilted for the small scale, while it is blue-tilted for the(...TRUNCATED) | [-1.7581044435501099,1.3631465435028076,2.220350742340088,-1.2839934825897217,-1.2147631645202637,0.(...TRUNCATED) | [-1.2681771516799927,0.7135223746299744,2.2048377990722656,-1.0525380373001099,-1.0923027992248535,0(...TRUNCATED) | [-1.4785854816436768,0.6043232679367065,2.2463908195495605,-1.3227494955062866,-1.4953588247299194,0(...TRUNCATED) | [-1.5844978094100952,0.6802815198898315,2.0604562759399414,-1.3918029069900513,-1.153984785079956,0.(...TRUNCATED) | [-1.6261729001998901,0.963344931602478,1.8008793592453003,-1.285820722579956,-1.4485738277435303,0.6(...TRUNCATED) | [-1.285000205039978,1.0834344625473022,1.9664721488952637,-1.2692452669143677,-1.3240199089050293,0.(...TRUNCATED) |
1804.05176 | Yen Chin Ong | Yen Chin Ong | Generalized Uncertainty Principle, Black Holes, and White Dwarfs: A Tale
of Two Infinities | 9 pages, 6 figures; version accepted by JCAP | JCAP 09 (2018) 015 | 10.1088/1475-7516/2018/09/015 | null | gr-qc hep-ph hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " It is often argued that quantum gravitational correction to the Heisenberg's\nuncertainty princip(...TRUNCATED) | [{"created":"Sat, 14 Apr 2018 06:42:19 GMT","version":"v1"},{"created":"Mon, 3 Sep 2018 13:02:08 GMT(...TRUNCATED) | 2018-09-18 | [
[
"Ong",
"Yen Chin",
""
]
] | "It is often argued that quantum gravitational correction to the Heisenberg's uncertainty principle (...TRUNCATED) | "It is often argued that quantum gravitational correction to the Heisenberg's uncertainty principle (...TRUNCATED) | "We show that this problem can be resolved if the parameter in the generalized uncertainty principle(...TRUNCATED) | "It is often argued that quantum gravitational correction to the Heisenberg's uncertainty principle (...TRUNCATED) | " In this paper, we resolve this paradox by showing that quantum gravity also modifies the gravitati(...TRUNCATED) | "It is often argued that quantum gravitational correction to the Heisenberg's uncertainty principle (...TRUNCATED) | " In this paper, we resolve this apparent paradox by showing that the generalized uncertainty princi(...TRUNCATED) | "It is often argued that quantum gravitational correction to the Heisenberg's uncertainty principle (...TRUNCATED) | " In this paper, we resolve this problem by showing that quantum gravity also modifies the gravitati(...TRUNCATED) | [-1.3527727127075195,1.532238245010376,0.8709449172019958,-0.5087658166885376,-1.1111664772033691,0.(...TRUNCATED) | [-1.5846331119537354,1.396609902381897,1.4090402126312256,-0.2845644950866699,-0.7642229199409485,0.(...TRUNCATED) | [-1.7949730157852173,1.2841145992279053,1.0146629810333252,-0.5739048719406128,-0.5332298874855042,-(...TRUNCATED) | [-1.2897344827651978,1.5332043170928955,1.2030134201049805,-0.44554850459098816,-0.9603905081748962,(...TRUNCATED) | [-1.678576111793518,1.5181611776351929,1.3462762832641602,-0.541201651096344,-0.7079002857208252,0.3(...TRUNCATED) | [-1.5624139308929443,1.1516798734664917,0.6509800553321838,-0.832836925983429,-1.2084490060806274,0.(...TRUNCATED) |
1010.4966 | Khaled Saaidi | Kh. Saaidi, H. Hossienkhani | Gravitational Baryogenesis in Anisotropic Universe | 12 pages, no figure | Astrophys. Space Sci. 333 (2011) 305 | 10.1007/s10509-010-0580-y | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " The interaction between Ricci scalar curvature and the baryon number current,\ndynamically breaks(...TRUNCATED) | [
{
"created": "Sun, 24 Oct 2010 14:32:27 GMT",
"version": "v1"
}
] | 2014-01-20 | [
[
"Saaidi",
"Kh.",
""
],
[
"Hossienkhani",
"H.",
""
]
] | "The interaction between Ricci scalar curvature and the baryon number current, dynamically breaks CP(...TRUNCATED) | "The interaction between Ricci scalar curvature and the baryon number current, dynamically breaks CP(...TRUNCATED) | "We find out the effect of anisotropy of the universe on the baryon asymmetry for the case which the(...TRUNCATED) | "The interaction between Ricci scalar curvature and the baryon number current, dynamically breaks CP(...TRUNCATED) | " In this case, the expansion of the universe is anisotropic. We show that the gravitational baryoge(...TRUNCATED) | "The interaction between Ricci scalar curvature and the baryon number current, dynamically breaks CP(...TRUNCATED) | " In this case, the expansion of the universe is anisotropic. We show that the gravitational baryoge(...TRUNCATED) | "The interaction between Ricci scalar curvature and the baryon number current, dynamically breaks CP(...TRUNCATED) | " In this case, the expansion of the universe is anisotropic. We show that the gravitational baryon (...TRUNCATED) | [-1.8941690921783447,2.173750400543213,0.6835286617279053,-0.1535845696926117,-1.133593201637268,0.2(...TRUNCATED) | [-1.7723321914672852,1.924214482307434,0.707692563533783,-0.41450735926628113,-0.447521835565567,0.1(...TRUNCATED) | [-1.7400022745132446,1.9805116653442383,1.0972833633422852,-0.27371636033058167,-0.7645008563995361,(...TRUNCATED) | [-1.467387080192566,2.060490608215332,0.5638427734375,-1.0076950788497925,-0.736670196056366,-0.1132(...TRUNCATED) | [-1.2357512712478638,1.8751448392868042,0.6369588375091553,-0.3500601053237915,-0.9340974688529968,-(...TRUNCATED) | [-1.4002282619476318,1.479986548423767,0.18285730481147766,0.06285917013883591,-0.8144745826721191,0(...TRUNCATED) |
1410.5882 | John Miller | John Miller, Lisa Barsotti, Salvatore Vitale, Peter Fritschel, Daniel
Sigg and Matthew Evans | Prospects for doubling the range of Advanced LIGO | null | Phys. Rev. D 91, 062005 2015 | 10.1103/PhysRevD.91.062005 | null | gr-qc astro-ph.IM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " In the coming years, the gravitational wave community will be optimizing\ndetector performance fo(...TRUNCATED) | [{"created":"Tue, 21 Oct 2014 23:27:47 GMT","version":"v1"},{"created":"Tue, 30 Dec 2014 18:28:18 GM(...TRUNCATED) | 2015-03-31 | [["Miller","John",""],["Barsotti","Lisa",""],["Vitale","Salvatore",""],["Fritschel","Peter",""],["Si(...TRUNCATED) | "In the coming years, the gravitational wave community will be optimizing detector performance for a(...TRUNCATED) | "In the coming years, the gravitational wave community will be optimizing detector performance for a(...TRUNCATED) | "Specifically, we consider squeezed light injection for reduction of quantum noise, detector design (...TRUNCATED) | "In the coming years, the gravitational wave community will be optimizing detector performance for a(...TRUNCATED) | " These upgrades include the use of cryogenic test masses, the addition of a higher power laser, and(...TRUNCATED) | "In the coming years, the gravitational wave community will be optimizing detector performance for a(...TRUNCATED) | " These include new test masses made from silicon, novel suspensions for the test masses that are le(...TRUNCATED) | "In the coming years, the gravitational wave community will be optimizing detector performance for a(...TRUNCATED) | " These upgrades include the incorporation of squeezed vacuum into the power recycling and the signa(...TRUNCATED) | [-1.1792715787887573,1.9056568145751953,1.2010579109191895,-1.0735771656036377,-0.7128375172615051,0(...TRUNCATED) | [-1.615400791168213,2.10168194770813,1.6010199785232544,-1.4297281503677368,-0.5121473670005798,-0.0(...TRUNCATED) | [-1.7472670078277588,1.7169915437698364,1.5255316495895386,-1.6873408555984497,-0.1844012290239334,0(...TRUNCATED) | [-1.2366915941238403,1.5375900268554688,1.9947627782821655,-2.1800482273101807,-0.35555556416511536,(...TRUNCATED) | [-1.5928055047988892,2.2624855041503906,1.6392415761947632,-2.043419599533081,-0.16507433354854584,0(...TRUNCATED) | [-1.1998951435089111,2.509512424468994,1.5154749155044556,-1.615876317024231,-0.42672526836395264,0.(...TRUNCATED) |
gr-qc/0609059 | Saulo Carneiro | A. E. Montenegro Jr. and S. Carneiro | Exact solutions of Brans-Dicke cosmology with decaying vacuum density | "Minor changes, references added. Version accepted for publication in\n Classical and Quantum Gravi(...TRUNCATED) | Class.Quant.Grav.24:313-327,2007 | 10.1088/0264-9381/24/2/004 | null | gr-qc astro-ph hep-th | null | " We investigate cosmological solutions of Brans-Dicke theory with both the\nvacuum energy density (...TRUNCATED) | [{"created":"Sat, 16 Sep 2006 13:59:07 GMT","version":"v1"},{"created":"Thu, 16 Nov 2006 00:21:15 GM(...TRUNCATED) | 2010-03-19 | [
[
"Montenegro",
"A. E.",
"Jr."
],
[
"Carneiro",
"S.",
""
]
] | "We investigate cosmological solutions of Brans-Dicke theory with both the vacuum energy density and(...TRUNCATED) | "We investigate cosmological solutions of Brans-Dicke theory with both the vacuum energy density and(...TRUNCATED) | "In addition, we have three other solutions, with Brans-Dicke parameter w = -1 and negative cosmolog(...TRUNCATED) | "We investigate cosmological solutions of Brans-Dicke theory with both the vacuum energy density and(...TRUNCATED) | " The time variation of the gravitational constant is also consistent with recent experimental data.(...TRUNCATED) | "We investigate cosmological solutions of Brans-Dicke theory with both the vacuum energy density and(...TRUNCATED) | The solution also provides a good fit to the distance and luminosity data. | "We investigate cosmological solutions of Brans-Dicke theory with both the vacuum energy density and(...TRUNCATED) | " Our solutions also predict the existence of a phantom-like component, and a non-vanishing value fo(...TRUNCATED) | [-2.383946418762207,1.4274474382400513,1.422061800956726,0.0802113488316536,-1.2294710874557495,0.31(...TRUNCATED) | [-1.766131043434143,1.1894259452819824,1.6585488319396973,0.2671806216239929,0.030692938715219498,0.(...TRUNCATED) | [-2.261566400527954,1.5146458148956299,1.6454780101776123,-0.15687398612499237,-0.425577849149704,0.(...TRUNCATED) | [-1.836361289024353,1.2584209442138672,1.462222695350647,-0.026757564395666122,-0.5375149250030518,0(...TRUNCATED) | [-2.1235761642456055,0.8030813932418823,1.499552607536316,-0.12334368377923965,-0.8556692600250244,0(...TRUNCATED) | [-1.7653062343597412,1.4025851488113403,0.755748450756073,-0.038314588367938995,-1.2760432958602905,(...TRUNCATED) |
1008.2644 | Sumit Ghosh | Rabin Banerjee, Sumit Ghosh, Dibakar Roychowdhury | "New type of phase transition in Reissner Nordstr\\\"om - AdS black hole\n and its thermodynamic ge(...TRUNCATED) | "Major revisions in Sec. 3. New results and interpretations. 2 new\n references. To appear in Phys.(...TRUNCATED) | Phys.Lett.B696:156-162,2011 | 10.1016/j.physletb.2010.12.010 | null | gr-qc hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " The phase transition of a RN-AdS black hole is studied in details using\nEhrenfest's equations. T(...TRUNCATED) | [{"created":"Mon, 16 Aug 2010 13:11:57 GMT","version":"v1"},{"created":"Thu, 9 Dec 2010 18:08:09 GMT(...TRUNCATED) | 2012-02-10 | [
[
"Banerjee",
"Rabin",
""
],
[
"Ghosh",
"Sumit",
""
],
[
"Roychowdhury",
"Dibakar",
""
]
] | "The phase transition of a RN-AdS black hole is studied in details using Ehrenfest's equations. Ther(...TRUNCATED) | "The phase transition of a RN-AdS black hole is studied in details using Ehrenfest's equations. Ther(...TRUNCATED) | "However this deviation from the second Ehrenfest's equation, for a certain range of the black hole (...TRUNCATED) | "The phase transition of a RN-AdS black hole is studied in details using Ehrenfest's equations. Ther(...TRUNCATED) | " This is in agreement with the previous results which showed that the phase transition of a RN-AdS (...TRUNCATED) | "The phase transition of a RN-AdS black hole is studied in details using Ehrenfest's equations. Ther(...TRUNCATED) | " The phase transition is therefore of higher order. We calculate the critical exponents and find th(...TRUNCATED) | "The phase transition of a RN-AdS black hole is studied in details using Ehrenfest's equations. Ther(...TRUNCATED) | " The phase transition is of the higher order type and it is characterized by a zero value of the he(...TRUNCATED) | [-1.040454626083374,2.164729356765747,0.07052432745695114,-0.18033555150032043,-0.6810446381568909,1(...TRUNCATED) | [-1.57611083984375,2.1663386821746826,0.3895927965641022,-0.05889892578125,-0.33218804001808167,1.28(...TRUNCATED) | [-2.0426745414733887,2.0137670040130615,0.46638578176498413,-0.1289457380771637,-0.3409271240234375,(...TRUNCATED) | [-1.4756828546524048,2.0995187759399414,1.0325335264205933,-0.48252958059310913,-0.2926905155181885,(...TRUNCATED) | [-1.248455286026001,2.5366241931915283,-0.14581298828125,-0.3564551770687103,-0.350341796875,0.56427(...TRUNCATED) | [-1.1788510084152222,2.695061206817627,0.2693450152873993,-0.33526521921157837,-0.37192490696907043,(...TRUNCATED) |
1509.08771 | Victor Ars\`ene Kpadonou | A. V. Kpadonou, M. J. S. Houndjo, M. E. Rodrigues | "Tolman-Oppenheimer-Volkoff Equations and their implications or the\n structures of relativistic St(...TRUNCATED) | null | Astrophys. Space Sci. (2016) 361:244 | 10.1007/s10509-016-2805-1 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " We investigate in this paper the structures of neutron and quark stars in\nf(T) theory of gravity(...TRUNCATED) | [
{
"created": "Sun, 27 Sep 2015 17:45:29 GMT",
"version": "v1"
}
] | 2016-11-29 | [
[
"Kpadonou",
"A. V.",
""
],
[
"Houndjo",
"M. J. S.",
""
],
[
"Rodrigues",
"M. E.",
""
]
] | "We investigate in this paper the structures of neutron and quark stars in f(T) theory of gravity wh(...TRUNCATED) | "We investigate in this paper the structures of neutron and quark stars in f(T) theory of gravity wh(...TRUNCATED) | "We search for the deviation of the mass-radius diagrams for power-law and exponential type correcti(...TRUNCATED) | "We investigate in this paper the structures of neutron and quark stars in f(T) theory of gravity wh(...TRUNCATED) | " The mass-radius relations and mass-central density (M-R) relations of the stars are obtained. The (...TRUNCATED) | "We investigate in this paper the structures of neutron and quark stars in f(T) theory of gravity wh(...TRUNCATED) | " The results of the integrations are compared with the corresponding ones in general relativity. It(...TRUNCATED) | "We investigate in this paper the structures of neutron and quark stars in f(T) theory of gravity wh(...TRUNCATED) | " It is found that the mass-radius relation of the neutron star is modified by the torsion effect. T(...TRUNCATED) | [-2.7360479831695557,1.9306460618972778,2.475517988204956,-0.1423148810863495,-0.777031660079956,0.4(...TRUNCATED) | [-2.460602045059204,1.71897292137146,2.6092112064361572,-0.35155826807022095,-0.1687818467617035,0.8(...TRUNCATED) | [-2.52957820892334,1.91670560836792,3.1333389282226562,-0.4808211624622345,0.007358584087342024,0.43(...TRUNCATED) | [-2.3992526531219482,1.779097318649292,2.5925400257110596,-0.49366191029548645,-0.27264776825904846,(...TRUNCATED) | [-2.4421815872192383,1.4206839799880981,2.2020199298858643,0.08759129047393799,-0.238325834274292,1.(...TRUNCATED) | [-2.5135445594787598,1.7456340789794922,1.8000774383544922,0.060830820351839066,-0.8055267333984375,(...TRUNCATED) |
1304.0330 | Jeandrew Brink | Jeandrew Brink, Marisa Geyer and Tanja Hinderer | Orbital resonances around Black holes | 5 pages, 5 figures | Phys. Rev. Lett. 114, 081102 (2015) | 10.1103/PhysRevLett.114.081102 | null | gr-qc astro-ph.GA math.CA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " We compute the length and timescales associated with resonant orbits in the\nKerr Metric for all (...TRUNCATED) | [
{
"created": "Mon, 1 Apr 2013 11:01:36 GMT",
"version": "v1"
}
] | 2015-03-05 | [
[
"Brink",
"Jeandrew",
""
],
[
"Geyer",
"Marisa",
""
],
[
"Hinderer",
"Tanja",
""
]
] | "We compute the length and timescales associated with resonant orbits in the Kerr Metric for all orb(...TRUNCATED) | "We compute the length and timescales associated with resonant orbits in the Kerr Metric for all orb(...TRUNCATED) | "The onset of geodesic chaos for non-Kerr spacetimes should occur at the resonance locations quantif(...TRUNCATED) | "We compute the length and timescales associated with resonant orbits in the Kerr Metric for all orb(...TRUNCATED) | We present a set of tools that can be used to compute resonances for any given metric. | "We compute the length and timescales associated with resonant orbits in the Kerr Metric for all orb(...TRUNCATED) | " We present a set of analytic fits to the timescales as a function of the orbital radius and spin o(...TRUNCATED) | "We compute the length and timescales associated with resonant orbits in the Kerr Metric for all orb(...TRUNCATED) | " We find that for a Kerr black hole with spin a=0.5 and mass 4.5x10^6 solar masses the correspondin(...TRUNCATED) | [-1.6309760808944702,1.26171875,2.3091542720794678,-0.3653145134449005,-0.6981275677680969,0.1448709(...TRUNCATED) | [-1.767693281173706,1.30524742603302,3.003214120864868,-0.670514702796936,-0.7031451463699341,-0.030(...TRUNCATED) | [-1.660597801208496,0.994584321975708,2.7275633811950684,-1.0444972515106201,-0.303899884223938,0.50(...TRUNCATED) | [-1.814303994178772,1.019533395767212,2.6084749698638916,-1.2030061483383179,-0.4286719262599945,0.3(...TRUNCATED) | [-1.6754416227340698,1.308791160583496,2.917391300201416,-0.801758885383606,-0.45019373297691345,0.2(...TRUNCATED) | [-1.527577519416809,1.4083219766616821,2.065584659576416,-1.0112813711166382,-0.3686056435108185,0.3(...TRUNCATED) |
2305.19819 | Yongqiang Wang | Peng-Bo Ding, Tian-Xiang Ma, Yong-Qiang Wang | Study of Boson Stars with Wormhole | 23 pages, 17 figures | null | null | null | gr-qc hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " In this paper, we reconsider the mixed system of BSs with wormholes at their\ncenter which perfor(...TRUNCATED) | [
{
"created": "Wed, 31 May 2023 13:02:09 GMT",
"version": "v1"
}
] | 2023-06-01 | [
[
"Ding",
"Peng-Bo",
""
],
[
"Ma",
"Tian-Xiang",
""
],
[
"Wang",
"Yong-Qiang",
""
]
] | "In this paper, we reconsider the mixed system of BSs with wormholes at their center which performed(...TRUNCATED) | "In this paper, we reconsider the mixed system of BSs with wormholes at their center which performed(...TRUNCATED) | "However, when it comes to excited state, the properties of solutions of symmetry is similar to the (...TRUNCATED) | "In this paper, we reconsider the mixed system of BSs with wormholes at their center which performed(...TRUNCATED) | " In the excited state, we find that the charge $Q$ and mass $M$ are only related to the frequency $(...TRUNCATED) | "In this paper, we reconsider the mixed system of BSs with wormholes at their center which performed(...TRUNCATED) | " In excited state, we find that the mass and charge of solutions increase with the increase of $\\o(...TRUNCATED) | "In this paper, we reconsider the mixed system of BSs with wormholes at their center which performed(...TRUNCATED) | " Besides, the relationship between the potential $U(\\phi)$ and the number of solutions is also dis(...TRUNCATED) | [-2.034358263015747,1.9914389848709106,1.0676889419555664,-0.6986922025680542,-0.7639468312263489,0.(...TRUNCATED) | [-1.7531421184539795,1.841132402420044,1.7633960247039795,-1.0762511491775513,-0.2162351757287979,1.(...TRUNCATED) | [-2.097670078277588,1.8376764059066772,2.0351881980895996,-0.8994139432907104,-0.45559921860694885,0(...TRUNCATED) | [-1.8787184953689575,2.514220952987671,1.9916601181030273,-0.7485053539276123,-0.6027032136917114,0.(...TRUNCATED) | [-1.5688281059265137,2.193798542022705,1.8229542970657349,-0.5262802243232727,-0.2933378517627716,1.(...TRUNCATED) | [-1.7128322124481201,1.7420982122421265,1.4165560007095337,-0.4542967677116394,-0.8944270014762878,1(...TRUNCATED) |
1409.0105 | Flavio Mercati | Flavio Mercati | A Shape Dynamics Tutorial | "v2.0 (greatly extended and updated), 133 pages, two columns in\n landscape format, for optimal rea(...TRUNCATED) | null | null | null | gr-qc hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | " Shape Dynamics (SD) is a new theory of gravity that is based on fewer and\nmore fundamental first(...TRUNCATED) | [{"created":"Sat, 30 Aug 2014 11:58:29 GMT","version":"v1"},{"created":"Mon, 29 May 2017 08:33:38 GM(...TRUNCATED) | 2017-05-30 | [
[
"Mercati",
"Flavio",
""
]
] | "Shape Dynamics (SD) is a new theory of gravity that is based on fewer and more fundamental first pr(...TRUNCATED) | "Shape Dynamics (SD) is a new theory of gravity that is based on fewer and more fundamental first pr(...TRUNCATED) | "The Tutorial is sufficiently self-contained for an undergrad student with some basic background in (...TRUNCATED) | "Shape Dynamics (SD) is a new theory of gravity that is based on fewer and more fundamental first pr(...TRUNCATED) | " The SD action is derived from the most general action that is invariant under the group of spatial(...TRUNCATED) | "Shape Dynamics (SD) is a new theory of gravity that is based on fewer and more fundamental first pr(...TRUNCATED) | " The new results in SD that are described in this Tutorial include the derivation of a new set of f(...TRUNCATED) | "Shape Dynamics (SD) is a new theory of gravity that is based on fewer and more fundamental first pr(...TRUNCATED) | " The Tutorial is intended for the general reader with some background in physics but no expertise i(...TRUNCATED) | [-1.037041425704956,1.4933580160140991,1.0300508737564087,-0.1103372722864151,-1.2712879180908203,0.(...TRUNCATED) | [-1.0915766954421997,1.304999589920044,1.3562058210372925,0.03998807072639465,-1.5511034727096558,1.(...TRUNCATED) | [-1.0702166557312012,1.528196096420288,1.3219380378723145,-0.21121950447559357,-1.0703504085540771,0(...TRUNCATED) | [-1.066670536994934,1.1285693645477295,1.1893665790557861,-0.6155804991722107,-1.5827574729919434,0.(...TRUNCATED) | [-0.9532856941223145,1.221015214920044,1.1189196109771729,-0.3501634895801544,-1.3403691053390503,0.(...TRUNCATED) | [-0.9134100675582886,1.2721987962722778,1.0703186988830566,-0.8911105990409851,-1.3495583534240723,0(...TRUNCATED) |
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