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[PDF] Top 20 Gravitino condensates in the early universe and inflation

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Gravitino condensates in the early universe and inflation

Gravitino condensates in the early universe and inflation

... where gravitino condensate fields near the origin of the effective potential play the role of the inflation ...massive gravitino phase, near the non-trivial minimum of the e ff ective ... See full document

17

Conformality Lost: Broken Symmetries in the Early Universe

Conformality Lost: Broken Symmetries in the Early Universe

... from inflation through sharp observational ...to inflation: violation of the null energy condition ...the universe transitioning from a contracting epoch to an expanding phase is intimately tied to ... See full document

165

Several Routes to Determining Entropy Generation in the Early Universe

Several Routes to Determining Entropy Generation in the Early Universe

... of early universe entropy being proportional to the spatial integral of energy minus an interaction between particles or ...pre inflation space3, and then how to form worm hole bridge between a prior ... See full document

26

Domain Walls and Matter-Antimatter Domains in the Early Universe

Domain Walls and Matter-Antimatter Domains in the Early Universe

... baryo-symmetric universe with cos- mologically large domains of matter and antimatter, avoiding the domain wall ...rather early in the universe. Inflation is an essential ingredient of the ... See full document

11

Turbulence of weak gravitational waves in the early universe

Turbulence of weak gravitational waves in the early universe

... the Universe (see Supplemental Material ...the inflation and the transition to the radiation dominated ...the early Universe that might be detected in the future ... See full document

7

Early Universe and Evolution of the Present Universe: Exact Solution Models

Early Universe and Evolution of the Present Universe: Exact Solution Models

... the universe find Robertson-Walker models starting either from a non-singular origin with a minimum, non-zero G or from a singularity with a vanishing G, where G increases continuously in the radiation dominated ... See full document

9

Status of the GroundBIRD Telescope

Status of the GroundBIRD Telescope

... of Universe right after the big bang, and in order to solve them, a model of rapid, superluminal expansion of space in very early Universe, commonly called the inflationary cosmology is proposed in ... See full document

9

Initial conditions in chaotic inflation with modified gravity

Initial conditions in chaotic inflation with modified gravity

... homogeneous Universe may form spherical or hyperbolic 3-dimensional manifold, its flatness at present is ...the Universe expansion the size of causally connected region, particle horizon, grows faster than ... See full document

8

The Propagation Delay Effect of the Expansion and Inflation of the Universe

The Propagation Delay Effect of the Expansion and Inflation of the Universe

... the Universe. Stephen Hawking in his Inflation Model also dis- cusses a delay type ...the early Universe. Since the Universe is thought to occupy all of space-time, one cannot define a ... See full document

8

Is the Cosmological Constant, a “Vacuum” Field? We Explore This by Squeezing Early Universe “Coherent Semi Classical States”, and Compare This to Energy from the Early Universe Heisenberg Uncertainty Principle

Is the Cosmological Constant, a “Vacuum” Field? We Explore This by Squeezing Early Universe “Coherent Semi Classical States”, and Compare This to Energy from the Early Universe Heisenberg Uncertainty Principle

... of early universe vacuum fields, and if this initial vacuum field corresponds to a configuration of early universe space-time at the start of ... See full document

17

Isolating a Minimum Radius of the Universe Consistent with the Production of at Least 1 Unit of Entropy, at the Start of Inflation

Isolating a Minimum Radius of the Universe Consistent with the Production of at Least 1 Unit of Entropy, at the Start of Inflation

... count of n , as referenced to entropy is in common with gravitons. Also, our analysis should be further refined to take into account [20], which may be with initial doable instrument refinements. Even so, we also point ... See full document

6

Evolution of a domain wall in expanding universe: inflation and after it

Evolution of a domain wall in expanding universe: inflation and after it

... the universe and possible existence of the cosmological antimatter crucially depends upon the version of C and CP violation realized in the early ... See full document

8

(Pseudo)goldstinos, SUSY fluids, Dirac gravitino and gauginos

(Pseudo)goldstinos, SUSY fluids, Dirac gravitino and gauginos

... is broken by a non-vanishing energy-momentum tensor. The modification to the Rarita-Schwinger Lagrangian appears as a deformation of the quadratic mass term. This allows to describe di ff erent propagation velocities of ... See full document

18

A Brief Review of  the Dynamical Universe in the Early and Late Stages

A Brief Review of the Dynamical Universe in the Early and Late Stages

... the universe there may be situation for the universe as the ‘point of no ...the universe will come to an end, although it cannot be negated the possibility of the evolution of new physics at this ... See full document

6

Cadamuro, Davide
  

(2012):


	Cosmological limits on axions and axion-like particles.


Dissertation, LMU München: Fakultät für Physik

Cadamuro, Davide (2012): Cosmological limits on axions and axion-like particles. Dissertation, LMU München: Fakultät für Physik

... where the subsript 0 means quantities at present time, n ¯ φ0 is the putative number density if φ would be stable, and E 0 is the energy at whih the photon would be seen today. The photon initial energy is m φ /2 and ... See full document

147

Evolution of Primordial Dark Matter Planets in the Early Universe

Evolution of Primordial Dark Matter Planets in the Early Universe

... Abstract: In a recent paper we had discussed possibility of DM at high redshifts forming primordial planets composed entirely of DM to be one of the reasons for not detecting DM (as the flux of ambient DM particles would ... See full document

10

Symmetry Breaking and the Structure Formation of the Expanded Early Universe

Symmetry Breaking and the Structure Formation of the Expanded Early Universe

... The curves show that at the higher temperatures only neutrons and protons exist, with there being more protons than neutrons while with the decrease of temperature, there is an increase amount of deuterium and helium ... See full document

7

The Effectiveness of Learning Instruction in Improving Teacher’s Competency in Teaching Gorontalo Language for Early Childhood and the Early Childhood’s Skills in Using the Language

The Effectiveness of Learning Instruction in Improving Teacher’s Competency in Teaching Gorontalo Language for Early Childhood and the Early Childhood’s Skills in Using the Language

... (c) Providing pictures that best describe the vocabulary of Gorontalo language to help the children understand the meaning of the words. A Chinese proverb says that picture worth ten thousand words. A picture can ... See full document

7

The Introduction and Regulation of Network Approach in the Integrated Early Childhood  Development in Nigeria

The Introduction and Regulation of Network Approach in the Integrated Early Childhood Development in Nigeria

... public early education ...for early childhood services to education ministries – as was the case with Norway (2005) and Sweden (1996) – continue to open all year round on a full-day basis and practise low ... See full document

6

The composition and formation of the Allende meteorite

The composition and formation of the Allende meteorite

... More specifically Anderson suggests that, since in his view the Ca, Al-rich aggregates in the Allende meteorite represent early condensates from the cooling solar nebula, the bulk chemic[r] ... See full document

118

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