Genesis of Dark Energy: Dark Energy as Consequence of Release and Two-Stage Tracking of Cosmological Nuclear Energy

R. C. Gupta; Anirudh Pradhan

doi:10.1007/s10773-010-0261-1

Genesis of Dark Energy: Dark Energy as Consequence of Release and Two-Stage Tracking of Cosmological Nuclear Energy

International Journal of Theoretical Physics ◽

10.1007/s10773-010-0261-1 ◽

2010 ◽

Vol 49 (4) ◽

pp. 821-834 ◽

Cited By ~ 27

Author(s):

R. C. Gupta ◽

Anirudh Pradhan

Keyword(s):

Dark Energy ◽

Nuclear Energy ◽

Two Stage

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Understanding the innovative developments with two-stage technology S-curve of nuclear energy projects

Progress in Nuclear Energy ◽

10.1016/j.pnucene.2021.103924 ◽

2021 ◽

Vol 140 ◽

pp. 103924

Author(s):

Yue Meng ◽

Hasan Diner ◽

Serhat Yüksel

Keyword(s):

Nuclear Energy ◽

Two Stage ◽

Energy Projects ◽

S Curve

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Cross-correlating spectroscopic and photometric galaxy surveys

Proceedings of the International Astronomical Union ◽

10.1017/s174392131401374x ◽

2014 ◽

Vol 10 (S306) ◽

pp. 213-215

Author(s):

Martin B. Eriksen ◽

Enrique Gaztañaga

Keyword(s):

Dark Energy ◽

Figure Of Merit ◽

Stage Iv ◽

The Other ◽

Sample Variance ◽

Two Stage ◽

Galaxy Surveys ◽

Other Hand ◽

Growth History ◽

Cross Correlations

AbstractDoes photometric and spectroscopic survey benefit from overlapping areas? The photometric survey measures 2D Weak Lensing (WL) information from galaxy shape distortions. On the other hand, the higher redshift precision of an spectroscopic survey allows measurements of redshift space distortions (RSD) and baryonic accustic oscillations (BAO) from 3D galaxy counts.The two surveys are combined using 2D-correlations, using sufficiently narrow bins to capture the radial information. This poster present effects of RSD and intrinsic correlations between narrow redshift bins. In understanding how the effects affects cosmological constrains, we first define two stage-IV and then present forecast for various configurations. When surveys overlap, they benefit from additional cross-correlations and sample variance cancellations from overlapping volumes. For a combined dark energy and growth history figure of merit, the result increase 50% for overlapping surveys, corresponding to 30% larger area.

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Review of low energy nuclear astrophysics

Modern Physics Letters A ◽

10.1142/s0217732321300196 ◽

2021 ◽

Vol 36 (22) ◽

pp. 2130019

Author(s):

Leonard S. Kisslinger ◽

Debasish Das

Keyword(s):

Dark Matter ◽

Dark Energy ◽

Star Formation ◽

Neutron Star ◽

Neutron Stars ◽

Nuclear Energy ◽

Massive Stars ◽

Nuclear Astrophysics ◽

Low Energy ◽

The Sun

In this review of Low Energy Nuclear Astrophysics, we review the nuclear energy and evolution of the sun. Then we review the estimate of dark matter from galaxy rotation. Next, we discuss neutron star formation from the gravitational collapse of massive stars which produces neutron stars and their velocity. Then the origin of supernovae, the estimate of dark energy from supernovae acceleration, and experiments related to low energy nuclear astrophysics are reviewed.

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Nuclear Energy Levels ofC13; Two-Stage ReactionN14(t, n)O16*(α)C12

Physical Review ◽

10.1103/physrev.127.2113 ◽

1962 ◽

Vol 127 (6) ◽

pp. 2113-2122 ◽

Cited By ~ 6

Author(s):

M. G. Silbert

Keyword(s):

Nuclear Energy ◽

Energy Levels ◽

Two Stage ◽

Nuclear Energy Levels

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Two-stage self-seeding method for preparation of single crystals of poly(phenylene sulfide)

Proceedings, annual meeting, Electron Microscopy Society of America ◽

10.1017/s0424820100153816 ◽

1989 ◽

Vol 47 ◽

pp. 368-369

Author(s):

Sengshiu Chung ◽

Peggy Cebe

Keyword(s):

Single Crystals ◽

High Performance ◽

Dilute Solution ◽

Two Stage ◽

Annealing Behavior ◽

High Performance Polymers ◽

Seeding Method ◽

Phenylene Sulfide

We are studying the crystallization and annealing behavior of high performance polymers, like poly(p-pheny1ene sulfide) PPS, and poly-(etheretherketone), PEEK. Our purpose is to determine whether PPS, which is similar in many ways to PEEK, undergoes reorganization during annealing. In an effort to address the issue of reorganization, we are studying solution grown single crystals of PPS as model materials.Observation of solution grown PPS crystals has been reported. Even from dilute solution, embrionic spherulites and aggregates were formed. We observe that these morphologies result when solutions containing uncrystallized polymer are cooled. To obtain samples of uniform single crystals, we have used two-stage self seeding and solution replacement techniques.

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