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Related papers: Dark Energy as the Remnant of Inflation

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A QED--based "bootstrap" mechanism is suggested as an explanation for the vacuum energy that furnished the initial impulse for Inflation, and continues on to provide present day Dark Energy. Virtual vacuum fluctuations are assumed to…

High Energy Physics - Theory · Physics 2015-06-15 H. M. Fried , Y. Gabellini

A QED-based model of a new version of Vacuum Energy has recently been suggested, which leads to a simple, finite, one parameter representation of Dark Energy. An elementary, obvious, but perhaps radical generalization is then able to…

General Physics · Physics 2015-06-19 H. M. Fried , Y. Gabellini

A QED-based mechanism, breaking translational invariance of the vacuum at sufficiently small distance scales, is suggested as an explanation for the vacuum energy pressure that accelerates the universe. Very-small-scale virtual vacuum…

High Energy Physics - Theory · Physics 2007-05-23 H. M. Fried

A QED-based bootstrap mechanism, appearing at sufficiently small space-time scales, is suggested as an explanation for the "dark" vacuum energy that may be able to accelerate the universe. Very small-scale vacuum currents are allowed to…

High Energy Physics - Theory · Physics 2011-04-11 H. M. Fried

Standard cosmology poses a number of important questions. Apart from its singular origin, it possesses early and late accelerating phases required to account for observations. The vacuum energy has been considered as a possible way to…

Cosmology and Nongalactic Astrophysics · Physics 2011-04-25 Saulo Carneiro , Reza Tavakol

The discovery of dark energy (DE) as the physical cause for the accelerated expansion of the Universe is the most remarkable experimental finding of modern cosmology. However, it leads to insurmountable theoretical difficulties from the…

High Energy Physics - Theory · Physics 2008-11-26 Joan Sola

It is shown that dark energy can be obtained from the interplay of the Higgs boson and the inflaton. A key element is the realization that electroweak symmetry breaking can trigger a second phase of rolling of the inflaton, which, when…

Cosmology and Nongalactic Astrophysics · Physics 2019-01-08 Konstantinos Dimopoulos , Tommi Markkanen

In recent years different explanations are provided for both an inflation and a recent acceleration in the expansion of the universe. In this Letter we show that a model of physical interest is the modification of general relativity with a…

High Energy Physics - Theory · Physics 2010-04-05 Ishwaree P. Neupane , Benedict M. N. Carter

The expansion of the Universe is understood to have accelerated during two epochs: in its very first moments during a period of Inflation and much more recently, at $z < 1$, when Dark Energy is hypothesized to drive cosmic acceleration. The…

Cosmology and Nongalactic Astrophysics · Physics 2019-03-25 Simone Ferraro , Michael J. Wilson , Muntazir Abidi , David Alonso , Behzad Ansarinejad , Robert Armstrong , Jacobo Asorey , Arturo Avelino , Carlo Baccigalupi , Kevin Bandura , Nicholas Battaglia , Chetan Bavdhankar , José Luis Bernal , Florian Beutler , Matteo Biagetti , Guillermo A. Blanc , Jonathan Blazek , Adam S. Bolton , Julian Borrill , Brenda Frye , Elizabeth Buckley-Geer , Philip Bull , Cliff Burgess , Christian T. Byrnes , Zheng Cai , Francisco J Castander , Emanuele Castorina , Tzu-Ching Chang , Jonás Chaves-Montero , Shi-Fan Chen , Xingang Chen , Christophe Balland , Christophe Yèche , J. D. Cohn , William Coulton , Helene Courtois , Rupert A. C. Croft , Francis-Yan Cyr-Racine , Guido D'Amico , Kyle Dawson , Jacques Delabrouille , Arjun Dey , Olivier Doré , Kelly A. Douglass , Duan Yutong , Cora Dvorkin , Alexander Eggemeier , Daniel Eisenstein , Xiaohui Fan , Pedro G. Ferreira , Andreu Font-Ribera , Simon Foreman , Juan García-Bellido , Martina Gerbino , Vera Gluscevic , Satya Gontcho A Gontcho , Daniel Green , Julien Guy , ChangHoon Hahn , Shaul Hanany , Will Handley , Nimish Hathi , Adam J. Hawken , César Hernández-Aguayo , Renée Hložek , Dragan Huterer , Mustapha Ishak , Marc Kamionkowski , Dionysios Karagiannis , Ryan E. Keeley , Robert Kehoe , Rishi Khatri , Alex Kim , Jean-Paul Kneib , Juna A. Kollmeier , Ely D. Kovetz , Elisabeth Krause , Alex Krolewski , Benjamin L'Huillier , Martin Landriau , Michael Levi , Michele Liguori , Eric Linder , Zarija Lukić , Axel de la Macorra , Andrés A. Plazas , Jennifer L. Marshall , Paul Martini , Kiyoshi Masui , Patrick McDonald , P. Daniel Meerburg , Joel Meyers , Mehrdad Mirbabayi , John Moustakas , Adam D. Myers , Nathalie Palanque-Delabrouille , Laura Newburgh , Jeffrey A. Newman , Gustavo Niz , Hamsa Padmanabhan , Povilas Palunas , Will J. Percival , Francesco Piacentini , Matthew M. Pieri , Anthony L. Piro , Abhishek Prakash , Jason Rhodes , Ashley J. Ross , Graziano Rossi , Gwen C. Rudie , Lado Samushia , Misao Sasaki , Emmanuel Schaan , David J. Schlegel , Marcel Schmittfull , Michael Schubnell , Neelima Sehgal , Leonardo Senatore , Hee-Jong Seo , Arman Shafieloo , Huanyuan Shan , Joshua D. Simon , Sara Simon , Zachary Slepian , Anže Slosar , Srivatsan Sridhar , Albert Stebbins , Stephanie Escoffier , Eric R. Switzer , Gregory Tarlé , Mark Trodden , Cora Uhlemann , L. Arturo Urenña-López , Eleonora Di Valentino , M. Vargas-Magaña , Yi Wang , Scott Watson , Martin White , Weishuang Xu , Byeonghee Yu , Gong-Bo Zhao , Yi Zheng , Hong-Ming Zhu

Inflation is a necessary cosmic mechanism to cure basic inconsistencies of the standard model of cosmology. These problems are usually `fixed' by postulating the existence of a scalar field (called the ``inflaton''). However, other less ad…

General Relativity and Quantum Cosmology · Physics 2026-01-16 Joan Solà Peracaula , Àlex González-Fuentes , Cristian Moreno-Pulido

Astronomical observations indicate an accelerated cosmic expansion, the cause of which is explained by the action of `dark energy'. Here we show that in discrete expanding space-time, only a tiny fraction of the vacuum fluctuations can…

Cosmology and Nongalactic Astrophysics · Physics 2012-11-21 Bruno M. Deiss

I propose a new mechanism to account for the observed tiny but finite dark energy in terms of a non-Abelian Higgs theory, which has infinitely many perturbative vacua characterized by a winding number, in the framework of inflationary…

General Relativity and Quantum Cosmology · Physics 2009-11-07 Jun'ichi Yokoyama

The metastable dark energy scenario is revisited by assuming that the current false vacuum energy density is the remnant from a primeval inflationary stage. The zero temperature scalar field potential is here described by an even power…

General Relativity and Quantum Cosmology · Physics 2020-09-01 J. A. S. Lima , G. J. M. Zilioti , L. C. T. Brito

We suggest that vacuum entanglement energy associated with the entanglement entropy of the universe is the origin of dark energy. The observed properties of dark energy can be explained by using the nature of entanglement energy without…

High Energy Physics - Theory · Physics 2010-10-27 Jae-Weon Lee , Jungjai Lee , Hyeong-Chan Kim

We show that current cosmic acceleration can be explained by an almost massless scalar field experiencing quantum fluctuations during primordial inflation. Provided its mass does not exceed the Hubble parameter today, this field has been…

Cosmology and Nongalactic Astrophysics · Physics 2012-05-08 Christophe Ringeval , Teruaki Suyama , Tomo Takahashi , Masahide Yamaguchi , Shuichiro Yokoyama

We suggest that the current acceleration of the universe may be explained by the vacuum energy of a hidden sector which is stuck in a state of equilibrium between phases. The phases are associated to a late-time first-order phase…

Astrophysics · Physics 2009-11-13 Ariel Megevand

The accelerating expansion of universe can be described by the non-zero cosmological constant or the dark energy. However, the origin of the dark energy remains a mystery of modern physics. The local Lorentz invariance is the most exact…

General Relativity and Quantum Cosmology · Physics 2018-10-16 Jiayin Shen , Xun Xue

It is shown that quantum vacuum fluctuations give rise to a curvature of space-time of the order appropriate to explain the observed accelerated expansion of the universe. The fact that the fluctuations produce curvature, even if the…

General Relativity and Quantum Cosmology · Physics 2011-03-21 Emilio Santos

We propose a model which produces dark energy perturbations large enough to explain the lack of power seen at the quadrupole scale in the cosmic microwave background. If the dark energy is frozen from horizon exit during inflation until…

Astrophysics · Physics 2011-05-12 Christopher Gordon , David Wands

Phantom Cosmology provides an unique opportunity to "connect" the phantom driven (low en- ergy meV scale) dark energy phase to the (high energy GUT scale) inflationary era. This is possible because the energy density increases in phantom…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-29 Cosmin Ilie , Tirthabir Biswas , Katherine Freese
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