Dipolar Electromagetic Condensate

Page 3 - Seeking answers about space? Join the Space community: the premier source of space exploration, innovation, and astronomy news, chronicling (and celebrating) humanity's ongoing expansion across the final frontier.
Apr 13, 2021
627
63
1,960
Dipolar fields exist in Stars and planets and Black Holes and Galactic centers.

The core creates magnetic fields around.
In Stars it creates turbulence within the star envelope.
In Galactic center it creates the dipolar jets that evolve as spiral arms turbulence in forming elliptical galaxy.
 
Jun 11, 2023
78
2
35
Understanding Neutron stars allows us to further understand Transients from Neutron Matter to the complex Quark, Partonic and Axion Gluon matter.
Harry,
Understanding Neutron Stars given as mostly made up of reverse beta decay hydrogen to Neutron Matter can't have anything to do with quarks or gluon matter because neither can survive outside the nucleon envelope/indestructible nucleon permeable mass-energy vessel sacs.
While nucleons, electrons, neutrinos and valence quarks are proven to exist as mass-energy vessel permeable sacs): The valence quarks and gluons can't exist outside the nucleon envelope and are irrelevent to understanding Neutron Stars Or Magnetars.
We are given that gluons are virtual particles that exist only inside the nucleon envelope and, possibly, nucleus of an atom!!

Under unique temporary circunstance per wikipedia): Quark-Gluon Plasma Is alleged): Production of QGP in the laboratory is achieved by colliding heavy atomic nuclei (called heavy ions as in an accelerator atoms are ionized) at relativistic energy in which matter is heated well above the Hagedorn Temperature TH = 150 MeV per particle, which amounts to a temperature exceeding 1.66×10e12 K. This can be accomplished by colliding two large nuclei at high energy (note that 175 MeV is not the energy of the colliding beam). Lead and gold nuclei have been used for such collisions at CERN SPSt and BNL RHIC , respectively. The nuclei are accelerated to ultrarelativistic speeds (contracting their length) and directed towards each other, creating a "fireball", in the rare event of a collision. Hydrodynamic simulation predicts this Fireball will expand under its own pressure, and cool while expanding. By carefully studying the spherical and elliptic flow, experimentalists put the theory to test.

Does Wiki support my postulate that gravity is a direct function of matter heating up with the given): "The nuclei are accelerated to ultrarelativistic speeds (contracting their length)" and that as the Fireball matter cools Dark Energy is released with the given): The Fireball will expand under its own pressure and ool while expanding!!
Sooooo): What comes first the cooling or the expansion??
 
Last edited:
Apr 13, 2021
627
63
1,960
Adoni
Once you understand compact objects and transients of condensates. You will look at alot of theings differently.
95% of all matter is in condensates.
 
Apr 13, 2021
627
63
1,960
The general question is:
Do the jets form from falling matter?
Or the compact object within itself generates dipolar electromagnetic field expelling matter away from the core.?

[Submitted on 18 Sep 2020 (v1), last revised 9 Nov 2020 (this version, v2)]

Magnetic Ergostars, Jet Formation and Gamma-Ray Bursts: Ergoregions versus Horizons​

Milton Ruiz, Antonios Tsokaros, Stuart L. Shapiro, Kyle C. Nelli, Sam Qunell
We perform the first fully general relativistic, magnetohydrodynamic simulations of dynamically stable hypermassive neutron stars with and without ergoregions to assess the impact of ergoregions on launching magnetically--driven outflows. The hypermassive neutron stars are modeled by a compressible and causal equation of state and are initially endowed with a dipolar magnetic field extending from the stellar interior into its exterior. We find that, after a few Alfvén times, magnetic field lines in the ergostar (star that contains ergoregions) and the normal star have been tightly wound in both cases into a helical funnel within which matter begins to flow outward. The maximum Lorentz factor in the outflow is ΓL∼2.5, while the force-free parameter holds at B2/8πρ0≲10. These values are incompatible with highly relativistic, magnetically-driven outflows (jets) and short γ-ray bursts. We compare these results with those of a spinning black hole surrounded by a magnetized, massless accretion disk that launches a bona fide jet. Our simulations suggest that the Blandford-Znajek mechanism for launching relativistic jets only operates when a black hole is present, though the Poynting luminosity in all cases is comparable. Therefore, one cannot distinguish a magnetized, accreting black hole from a magnetized hypermassive neutron star in the so-called mass-gap based solely on the value of the observed Poynting luminosity. These results complement our previous studies of supramassive remnants and suggest that it would be challenging for either normal neutron stars or ergostars in a hypermassive state to be the progenitors of short γ-ray bursts.
 
Apr 13, 2021
627
63
1,960
Although the paper is worth reading.
It's the assumption that the BBT applies.
The dipolar fields are worth investigating.

[Submitted on 5 Jul 2023]

Anisotropic Inflation in Dipolar Bose-Einstein Condensates​

Arun Rana, Abhijit Pendse, Sebastian Wüster, Sukanta Panda
Early during the era of cosmic inflation, rotational invariance may have been broken, only later emerging as a feature of low-energy physics. This motivates ongoing searches for residual signatures of anisotropic space-time, for example in the power spectrum of the cosmic microwave background. We propose that dipolar Bose-Einstein condensates (BECs) furnish a laboratory quantum simulation platform for the anisotropy evolution of fluctuation spectra during inflation, exploiting the fact that the speed of dipolar condensate sound waves depends on direction. We construct the anisotropic analogue space-time metric governing sound, by linking the time-varying strength of dipolar and contact interactions in the BEC to the scale factors in different coordinate directions. Based on these, we calculate the dynamics of phonon power spectra during an inflation that renders the initially anisotropic universe isotropic. We find that the expansion speed provides an experimental handle to control and study the degree of final residual anisotropy. Gravity analogues using dipolar condensates can thus provide tuneable experiments for a field of cosmology that was until now confined to a single experiment, our universe.
 
Apr 13, 2021
627
63
1,960
Chiral Supersymmetry plays an important role in Neutron Star Spin.
The dipolar Vector fields that are expelled from the star, is generated from the core. Just like a magnet it will have dipolar fields.


[Submitted on 7 Sep 2022 (v1), last revised 9 Oct 2022 (this version, v2)]

Intrinsic chiral field as vector potential of the magnetic current in the zig-zag lattice of magnetic dipoles​

Paula Mellado, Kevin Hofhuis, Ignacio Tapia, Andres Concha
Chiral magnetic insulators manifest novel phases of matter where the sense of rotation of the magnetization is associated with exotic transport phenomena. Effective control of such phases and their dynamical evolution points to the search and study of chiral fields like the Dzyaloshinskii-Moriya interaction. Here we combine experiments, numerics, and theory to study a zig-zag dipolar lattice as a model of an interface between magnetic in-plane layers with perpendicular magnetization. The zig-zag lattice comprises two parallel sublattices of dipoles with perpendicular easy plane of rotation. The dipolar energy of the system is exactly separable into a sum of symmetric and antisymmetric long-range exchange interactions between dipoles, where the antisymmetric coupling generates a nonlocal Dzyaloshinskii-Moriya field which stabilizes winding textures with the form of chiral solitons. The Dzyaloshinskii-Moriya interaction acts as a vector potential or gauge field of the magnetic current and gives rise to emergent magnetic and electric fields that allow the manifestation of the magnetoelectric effect in the system.