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Here goes the figure above demonstrates onto the evolution of the complex scalar Higgs field. On the left, the temperature dependent potential V(ø) for high temperatures is indicated by the violet surface; the potential at lower temperatures is represented by the yellow surface, and takes the form of the “Mexican hat”. For each of the two fields, the vacuum expectation value resides in the trough of the potential.
As different regions of the space transit from the higher temperature violet potential (indicated by the grey ball) to the lower temperature yellow potential (red or green balls), an arbitrary direction for the phase of the field is chosen. As indicated by the physical space diagram on the right, these random orientations do not always line up; along these boundaries a cosmic string will form (red balls/lines). Cosmic strings are hypothetical remnants of the early universe whose formation is a predicted result of spontaneous symmetry breaking. Detectable cosmic strings, which are on an energy scale of ~1015 GeV, may have formed during symmetry breaking that occurred in certain Grand Unified Theories (GUT) or at the end of inflation. Proof of their existence would excite both particle physicists and astronomers, as strings could connect us directly with exotic matter and conditions of the moments right after the big bang or the transition of mass within energy ant that simple.
As different regions of the space transit from the higher temperature violet potential (indicated by the grey ball) to the lower temperature yellow potential (red or green balls), an arbitrary direction for the phase of the field is chosen. As indicated by the physical space diagram on the right, these random orientations do not always line up; along these boundaries a cosmic string will form (red balls/lines). Cosmic strings are hypothetical remnants of the early universe whose formation is a predicted result of spontaneous symmetry breaking. Detectable cosmic strings, which are on an energy scale of ~1015 GeV, may have formed during symmetry breaking that occurred in certain Grand Unified Theories (GUT) or at the end of inflation. Proof of their existence would excite both particle physicists and astronomers, as strings could connect us directly with exotic matter and conditions of the moments right after the big bang or the transition of mass within energy ant that simple.
Candidate Pairs Observational interest in cosmic strings was recently rekindled by the discovery of Capodimonte–Sternberg–Lens Candidate, No.1, or CSL-1. This pair of galaxies share the same morphology and lie at a redshift of z=0.46. Further analysis shows that the unusual pair could be a result of gravitational lensing, a double image caused by a cosmic string. What Does a Cosmic String Do, Gravitational Lensing by a Cosmic String A cosmic string cuts out from flat space time a deficit at an angle, where m is the string’s energy per unit length. If a string lies between an observer and a galaxy, light from the galaxy travels in two paths around the string. The observer will see an identical pair of galaxies, two distinct images of the same object.
Now as their are a few theories about this one of which is a reverts into 'reaction engine that kinda enveloped its the’jumper design’ How a String Would Look?. Worried no need the field above shows two simulated cosmic strings at redshifts z=1.0 (dash) and z=0.5 (solid), placed in the goods’ Hubble Deep Field North. The red and yellow circles identify lensed pairs that result from the string. A string can be detected by finding identical pairs that follow the line of the string. Detection Method Our method for cosmic string detection involves finding pairs of similar galaxies, an indication of lensing by a string. Similarity can be measured by comparing ellipticities, angles of inclination, redshifts , and fluxes of pairs of objects. Images from the Great Observatories Origins Deep Survey (GOODS) were searched for pairs. This survey used the Hubble Space Telescope to observe the Hubble Deep Field North and the Chandra Deep Field South. Correlation of fluxes is described while shapes (ellipticity and angle of inclination) are described. The plots on the left show the distributions expected as background, obtained by correlating many random galaxies. The plots on the right display the expected signal from identical galaxies, obtained by correlating galaxies with their smoothed and re-realized counterparts.
Conclusions We have not yet found a cosmic string of energy scale 1015 GeV and longer than 10” within the GOODS fields. However, this does not rule out the existence of cosmic strings. GOODS only covered a fraction of the sky, with 123 arcmin2 in the north field and 140 arcmin2 in the south field. More wide-field surveys can be searched for strings using this technique of finding pairs of galaxies that are morphological similar.
Now as their are a few theories about this one of which is a reverts into 'reaction engine that kinda enveloped its the’jumper design’ How a String Would Look?. Worried no need the field above shows two simulated cosmic strings at redshifts z=1.0 (dash) and z=0.5 (solid), placed in the goods’ Hubble Deep Field North. The red and yellow circles identify lensed pairs that result from the string. A string can be detected by finding identical pairs that follow the line of the string. Detection Method Our method for cosmic string detection involves finding pairs of similar galaxies, an indication of lensing by a string. Similarity can be measured by comparing ellipticities, angles of inclination, redshifts , and fluxes of pairs of objects. Images from the Great Observatories Origins Deep Survey (GOODS) were searched for pairs. This survey used the Hubble Space Telescope to observe the Hubble Deep Field North and the Chandra Deep Field South. Correlation of fluxes is described while shapes (ellipticity and angle of inclination) are described. The plots on the left show the distributions expected as background, obtained by correlating many random galaxies. The plots on the right display the expected signal from identical galaxies, obtained by correlating galaxies with their smoothed and re-realized counterparts.
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