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Visualizzazione dei post in ordine di pertinenza per la query astro. Ordina per data Mostra tutti i post
Visualizzazione dei post in ordine di pertinenza per la query astro. Ordina per data Mostra tutti i post

sabato 5 febbraio 2022

# astro: aprops of horrific encounters, how to survive inside a (virtual) black hole


<< As (eight stars skirt a black hole 1m times the mass of the Sun) approach, all are stretched and deformed by the black hole's gravity. Some are completely pulled apart into a long stream of gas, a cataclysmic phenomenon called a tidal disruption event. Others are only partially disrupted, retaining some of their mass and returning to their normal shapes after their horrific encounters. >>

<< These simulations, (..) are the first to combine the physical effects of Einstein's general theory of relativity with realistic stellar density models. The virtual stars range from about one-tenth to 10 times the Sun's mass. >>

<< The division between stars that fully disrupt and those that endure isn't simply related to mass. Instead, survival depends more on the star's density. >>

Jeanette Kazmierczak. Scientists fling model stars at a virtual black hole to see who survives. NASA's Goddard Space Flight Center. Nov 26, 2021.


<< This paper introduces a series of papers presenting a quantitative theory for the tidal disruption of main-sequence stars by supermassive black holes (the pericenter-dependence of tidal disruption properties for eight stellar masses (..) and six black hole masses (..). >>

Taeho Ryu, Julian Krolik, et al. Tidal Disruptions of Main-sequence Stars. I. Observable Quantities and Their Dependence on Stellar and Black Hole Mass. ApJ 904 98. Nov 25, 2020.


Also

keyword 'black hole' | 'astro' in FonT



keywords: astro, blackhole, tidal disruption, survival, surviving



venerdì 10 gennaio 2020

# astro: you might find erratic massive black holes in dwarf galaxies ...

<< The new VLA (Very Large Array) observations revealed that 13 of these galaxies have strong evidence for a massive black hole that is actively consuming surrounding material. (AA) were very surprised to find that, in roughly half of those 13 galaxies, the black hole is not at the center of the galaxy, unlike the case in larger galaxies, >>  Amy Reines.

<< The scientists said this indicates that the galaxies likely have merged with others earlier in their history. This is consistent with computer simulations predicting that roughly half of the massive black holes in dwarf galaxies will be found wandering in the outskirts of their galaxies. >>

<< This work has taught us that we must broaden our searches for massive black holes in dwarf galaxies beyond their centers to get a more complete understanding of the population and learn what mechanisms helped form the first massive black holes in the early Universe, >> Amy Reines.

Astronomers find wandering massive black holes in dwarf galaxies. National Radio Astronomy Observatory. Jan 6, 2020.

https://m.phys.org/news/2020-01-astronomers-massive-black-holes-dwarf.html    

Amy Reines, James Condon, et al. A New Sample of (Wandering) Massive Black Holes in Dwarf Galaxies from High Resolution Radio Observations. arXiv:1909.04670v1 [astro-ph.GA] Sep 10, 2019.

https://arxiv.org/abs/1909.04670

Also

keyword 'astro' in FonT

https://flashontrack.blogspot.com/search?q=astro

mercoledì 5 agosto 2020

# astro: runaway cooling of intracluster gas during a silent black hole

<< supermassive black holes play a fundamental role in regulating the formation of stars throughout cosmic time. This has been clearly demonstrated in the case of galaxy clusters in which powerful feedback from the central black hole is  preventing the hot intracluster gas from cooling catastrophically, thus reducing the expected star formation rates by orders of magnitude. >>

AA << present the first observational evidence for massive, runaway cooling occurring in the absence of supermassive black hole feedback in the high-redshift galaxy cluster SpARCS104922.6+564032.5 (..) The hot intracluster gas appears to be fueling a massive burst of star formation >>

<< Intracluster stars are therefore not only produced by tidal stripping and the disruption of cluster galaxies, but can also be produced by runaway cooling of hot intracluster gas at early times. Overall, these observations show the dramatic impact when supermassive black hole feedback fails to operate in clusters. They indicate that in the highest overdensities such as clusters and proto-clusters, runaway cooling may be a new and important mechanism for fueling massive bursts of star formation in the early universe. >>

J. Hlavacek-Larrondo, C.L. Rhea, et al. Evidence of runaway gas cooling in the absence of supermassive black hole feedback at the epoch of cluster formation. arXiv:2007.15660v1 [astro-ph.GA]. Jul 30, 2020.


<< It reminds me of the old expression of 'when the cat's away, the mice will play,' (..) Here the cat, or black hole, is quiet and the mice, or stars, are very busy. >> Julie Hlavacek

Black hole fails to do its job. Chandra X-ray Center. Aug 3, 2020. 



sabato 25 giugno 2022

# astro: eight new echoing black hole binaries (in Milky Way)

<< Scattered across our Milky Way galaxy are tens of millions of black holes—immensely strong gravitational wells of spacetime, from which infalling matter, and even light, can never escape. Black holes are dark by definition, except on the rare occasions when they feed. As a black hole pulls in gas and dust from an orbiting star, it can give off spectacular bursts of X-ray light that bounce and echo off the inspiraling gas, briefly illuminating a black hole's extreme surroundings. >>

<< In a study appearing (..) in the The Astrophysical Journal, (AA) report (..) eight new echoing black hole binaries in our galaxy. Previously, only two such systems in the Milky Way were known to emit X-ray echoes. >>️

 << Kara (Erin Kara) and her colleagues are using X-ray echoes to map a black hole's vicinity, much the way that bats use sound echoes to navigate their surroundings. (..)  As a side project, Kara is working with MIT education and music scholars, Kyle Keane and Ian Condry, to convert the emission from a typical X-ray echo into audible sound waves. >>️️

Jennifer Chu. Search reveals eight new sources of black hole echoes. MIT.  May 2, 2022. 



Jingyi Wang, Erin Kara, et al. The NICER "Reverberation Machine": A Systematic Study of Time Lags in Black Hole X-Ray Binaries. ApJ. 930, 18. May 2, 2022. 


Also

keyword 'black hole' in FonT


keyword 'waves' in FonT


keyword 'onda' in Notes 
(quasi-stochastic poetry)


Keywords: astro, black hole, echoes, waves

mercoledì 6 aprile 2022

# astro: going beyond a performance by Frank Zappa (or a speech by – for example – a political entity), two speeds of sound found on Mars

AA << find that atmospheric sounds extend measurements of pressure variations down to 1,000 times smaller scales than ever observed before, revealing a dissipative regime extending over 5 orders of magnitude in energy. Using point sources of sound (Ingenuity rotorcraft, laser-induced sparks), (AA) highlight two distinct values for the speed of sound that are ~10 m/s apart below and above 240 Hz, a unique characteristic of low-pressure CO2-dominated atmosphere. (They) also provide the acoustic attenuation with distance above 2 kHz, allowing to elucidate the large contribution of the CO2 vibrational relaxation in the audible range. >>

Maurice, S., Chide, B., Murdoch, N. et al. In situ recording of Mars soundscape. Nature. doi: 10.1038/ s41586-022-04679-0. Apr 1, 2022. 


<< All of these factors would make it difficult for two people to have a conversation only five meters (16 feet) apart >> Sylvestre Maurice.

Juliette Collen and Daniel Lawler. First audio recorded on Mars reveals two speeds of sound. Phys.org. Apr 1, 2022. 


NASA Perseverance Rover Captures 
Puff, Whir, Zap Sounds from Mars 


Also

Frank Zappa 


image from  


keywords: astro, mars, acoustics, sound, speed of sound, dissipative regimes, music, jazz, freejazz









mercoledì 28 ottobre 2020

# astro: the effect of Yarkovsky acceleration to direct the asteroid Apophis (towards us, hypothetically)

<< A University of Hawai Institute for Astronomy (IfA) astronomer has revealed critical new findings linked to a large asteroid expected to pass extremely close to Earth. Dave Tholen and collaborators have announced the detection of Yarkovsky acceleration on the near-Earth asteroid Apophis. This acceleration arises from an extremely weak force on an object due to non-uniform thermal radiation. This force is particularly important for the asteroid Apophis, as it affects the probability of an Earth impact in 2068. >>

Massive asteroid subject of new findings. Oct 26, 2020. 


"2068" –Massive Asteroid Apophis on Path for Earth Impact. Oct 27, 2020.


Also

il ciottolo Apophis. Notes. May 05, 2006 (quasi-stochastic poetry). 


A wicked list in the dino-killing range; waiting for new entries. FonT. Jun 29, 2017. 



A few hints of our presence. Notes. Oct 13, 2006 (quasi-stochastic poetry)





martedì 22 febbraio 2022

# gst: apropos of a immaginary transition (with a tipping point), which simulates the chaotic interactions of three black holes.


<< The interactions between three bodies such as stars or planets or black holes cannot be predicted with an elegant formula. Moerman (Arend Moerman) therefore used a computer that calculates what happens for a short period of time and then uses the result for the next period of time. >>

AA << varied the masses of the three interacting black holes. They started with one solar mass and went up to a billion times the mass of the sun. >>

<< Around ten million solar masses, there appeared to be a tipping point. In the simulations, black holes that are lighter than about ten million solar masses mostly eject each other through a gravitational slingshot. Black holes heavier than about ten million solar masses start to merge. First, two black holes merge. The third black hole will follow later. The black holes merge because they lose kinetic energy and that is because they emit gravitational waves. >>

<< Arend's work (..) has led to a new understanding of how black holes become supermassive. In the simulations, we see that heavy black holes no longer endlessly move around each other, but that, if they are heavy enough, they collide pretty much instantly. >> Simon Portegies Zwart. 

Simulating chaotic interactions of three black holes. Netherlands Research School for Astronomy. Oct 20, 2021. 


Tjarda C. N. Boekholt, Arend Moerman, Simon F. Portegies Zwart. Relativistic Pythagorean three-body problem. Phys. Rev. D 104, 083020. 14 Oct 14,  2021. 


Also

more on the three-body problem (695 families of collisionless orbits). FonT. Oct 16, 2017. 


keyword 'black hole' | 'astro' in FonT



keyword 'transition' | 'transitional' in FonT



keyword 'transition' | 'transizion*' in Notes (quasi-stochastic poetry)




keywords: gst, black hole, three-body problem, transition, chaos, chaotic interaction, tipping point.



lunedì 19 settembre 2022

# astro: black holes (as Q-ball-type saturons) could admit multi-vortex dynamics

<< Theoretical physicists argue that black holes admit vortex structures >>

Img << Sketch of a black hole endowed with multiple vortices. Colors denote the orientation, with the associated trapped magnetic field lines in black. Credit: Dvali et al. >>️

<< Recently, a new quantum framework for black holes, namely in terms of Bose-Einstein condensates of gravitons (the quanta of gravity itself), has been introduced, (..) Up until our article was published, rotating black holes have not been thoroughly studied within this framework. However, they might not only exist, but also be the rule rather than the exception. >> Florian Kühnel. 
Ingrid Fadelli. Theoretical physicists argue that black holes admit vortex structures. Phys.org. Sep 09, 2022. 

AA << argue that black holes admit vortex structure. This is based both on a graviton-condensate description of a black hole as well as on a correspondence between black holes and generic objects with maximal entropy compatible with unitarity, so-called saturons. (They) show that due to vorticity, a Q-ball-type saturon of a calculable renormalizable theory obeys the same extremality bound on the spin as the black hole. Correspondingly, a black hole with extremal spin emerges as a graviton condensate with vorticity. (..) Next, (AA) show that in the presence of mobile charges, the global vortex traps a magnetic flux of the gauge field. This can have macroscopically observable consequences. >>
Gia Dvali, Florian Kuhnel, Michael Zantedeschi. Vortices in Black Holes. Phys. Rev. Lett. 129, 061302. Aug 3, 2022.  

Also

keyword 'black hole' in FonT  

Keywords: astro, astrophysics, black hole, rotating black hole, vortex, vorticity








venerdì 18 maggio 2018

# astro: crazy chaotic encounters (and megamerger)

<< Binary black holes are basically like giant targets hanging out in the cluster, and as you throw other black holes or stars at them, they undergo these crazy chaotic encounters >>

<< What people had done in the past was to treat this as a purely Newtonian problem, (..)  Newton’s theory of gravity works in 99.9 percent of all cases. The few cases in which it doesn’t work might be when you have two black holes whizzing by each other very closely, which normally doesn’t happen in most galaxies >> Carl Rodriguez

Jennifer Chu. Dense stellar clusters may foster black hole megamergers. MIT News Office. Apr 10, 2018.

http://news.mit.edu/2018/dense-stellar-clusters-may-foster-black-hole-megamergers-0410

Carl L. Rodriguez, Pau Amaro-Seoane, et al. Post-Newtonian Dynamics in Dense Star Clusters: Highly-Eccentric, Highly-Spinning, and Repeated Binary Black Hole Mergers.

Phys. Rev. Lett. 120, 151101 (2018). doi: 10.1103/PhysRevLett.120.151101.

arXiv:1712.04937 [astro-ph.HE]. Mar 14, 2018

https://arxiv.org/abs/1712.04937

mercoledì 6 marzo 2019

# gst astro: when a superbubble can generate trains of shock waves

<< Sixty-seven million light-years away, a galaxy is blowing enormous bubbles. We know what they are. Known as nuclear superbubbles, the structures are likely created by the supermassive black hole in the galaxy's centre. Now, thanks to new data, we know something incredible is occurring inside them. >>

<< Observations from NASA's Chandra X-ray Observatory of spiral galaxy NGC 3079 have revealed that the bubbles are actually a huge cosmic particle accelerator, producing energetic high-speed particles around their edges.  >>

<< As the bubbles expand into the surrounding gas of the interstellar medium, they generate shock waves, which in turn produce tangled magnetic fields. (..)  particles ricochet around these shock magnetic fields; when they pass through the shock front, they get an acceleration boost.  >>

Michelle Starr. Astronomers Have Found 'Superbubbles' Producing Shock Waves in Another Galaxy.  Mar 4, 2019.

https://www.sciencealert.com/colossal-bubbles-blown-by-a-supermassive-black-hole-are-a-cosmic-particle-accelerator

Jiang-Tao Li, Edmund Hodges-Kluck, et al. Detection of non-thermal hard X-ray emission from the "Fermi bubble" in an external galaxy.  ApJ in press. arXiv:1901.10536v1 [astro-ph.HE] Jan 31, 2019.

https://arxiv.org/abs/1901.10536

lunedì 4 marzo 2019

# astro: quiescent black holes abound in our Galaxy

AA << results provide new circumstantial evidences for a wandering intermediate-mass black hole in the Galactic center, suggesting also that high-velocity compact clouds can be probes of quiescent black holes abound in our Galaxy. >>

Shunya Takekawa, Tomoharu Oka, et al.  Indication of Another Intermediate - mass Black Hole in the Galactic Center. arXiv: 1812.10733v1 [astro-ph.GA]  doi: 10.3847/2041-8213/aafb07

https://arxiv.org/abs/1812.10733

"The Invisible Galaxy" - 100 Million Black Holes Lurking in the Milky Way (Weekend Feature). Mar 2, 2019

https://dailygalaxy.com/2019/03/the-invisible-galaxy-100-million-black-holes-lurking-in-the-milky-way-weekend-feature/

mercoledì 7 novembre 2018

# astro: the strange behavior of Oumuamua (Hawaiian for "scout")

<<  'Oumuamua (1I/2017 U1) is the first object of interstellar origin observed in the Solar system. >>

AA << discuss the possible origins of such an object including the possibility that it might be a lightsail of artificial origin. >>

Shmuel Bialy, Abraham Loeb. Could Solar Radiation Pressure Explain 'Oumuamua's Peculiar Acceleration? arXiv:1810.11490 [astro-ph.EP]. Oct 30, 2018.

https://arxiv.org/abs/1810.11490

Robby Berman. Harvard scientists suggest 'Oumuamua is an alien device. It's an asteroid, it's a comet, it's actually a spacecraft? Nov 6, 2018.

https://bigthink.com/surprising-science/oumuamua-spacecraft-alien-device

NASA utd about 'Oumuamua:

Calla Cofield. NASA Learns More About Interstellar Visitor 'Oumuamua. Nov. 14, 2018.

https://www.nasa.gov/feature/jpl/nasa-learns-more-about-interstellar-visitor-oumuamua




mercoledì 7 ottobre 2020

# astro: the turbulent history of Ryugu

<< The asteroid Ryugu may look like a solid piece of rock, but it's more accurate to liken it to an orbiting pile of rubble. >>

<< Ryugu is considered a C-type, or carbonaceous, asteroid, meaning it's primarily composed of rock that contains a lot of carbon and water (..) As expected, most of the surface boulders are also C-type; however, there are a large number of S-type, or siliceous, rocks as well. These are silicate-rich, lack water-rich minerals and are more often found in the inner, rather than outer, solar system. Given the presence of S- as well as C-type rocks on Ryugu, researchers are led to believe the little rubble-pile asteroid likely formed from the collision between a small S-type asteroid and Ryugu's larger C-type parent asteroid.  If the nature of this collision had been the other way around, the ratio of C- to S-type material in Ryugu would also be reversed. >>

Rock types on Ryugu provide clues to the asteroid's turbulent history. University of Tokyo. Sep 21, 2020. 


Tatsumi E., Sugimoto C., et al. Collisional history of Ryugu’s parent body from bright surface boulders. Nat Astron. doi: 10.1038/ s41550-020-1179-z. Sep 21, 2020.


Also

How small particles could reshape an asteroid. FonT. Sep 26, 2020.





venerdì 21 luglio 2017

# s-astro: the “mudball” model; a terrestrial muddiness from carbonaceous asteroids

<< Scientists have long held the belief that planets – including Earth – were built from rocky asteroids, but new research challenges that view >>

Planets like earth may have had muddy origins. July 14, 2017

https://m.phys.org/news/2017-07-planets-earth-muddy.html

<< It would have been a mud, rather than a rock >>

Philip A. Bland, Bryan J. Travis. Giant convecting mud balls of the early solar system. Science  Advances 14 Jul 2017: Vol.  3,  no.  7,  e1602514 doi: 10.1126/sciadv.1602514

http://advances.sciencemag.org/content/3/7/e1602514

lunedì 31 dicembre 2018

# astro: sources of ripples of spacetime: a brief history of black holes

<< The history of (..) hunt for these enigmatic objects traces back to the 18th century, but the crucial phase took place in a suitably dark period of human history - World War II. >>

Carla Rodrigues Almeida. A brief history of black holes. Max Planck Institute for the History of Science. Dec 27, 2018.

http://theconversation.com/a-brief-history-of-black-holes-107298

lunedì 28 agosto 2017

# astro: the binary black hole spin distribution, a sort of cosmic estension of Mr. Jelly Roll

<< The direct detection of gravitational waves from merging binary black holes opens up a window into the environments in which binary black holes form. One signature of such environments is the angular distribution of the black hole spins >>

AA << report that, if the magnitudes of the black hole spins are allowed to extend to high values, the effective spins for these systems indicate a 0.015 odds ratio against an aligned angular distribution compared to an isotropic one [isotropic spin orientation: the spins of the black holes are randomly oriented with respect to the orbit of the binary system]. When considering the effect of ten additional detections, this odds ratio decreases to 2.9 × 10−7 against alignment >>

Will M. Farr, Simon Stevenson, et al. Distinguishing spin-aligned and isotropic black hole populations with gravitational waves. Nature 548, 426–429 Aug 24, 2017 doi: 10.1038/nature23453

http://www.nature.com/nature/journal/v548/n7668/full/nature23453.html

https://arxiv.org/abs/1706.01385

<< Amico, qualunque  cosa suonerai . . . suonerai Jelly Roll >>

Jelly Roll Morton (opp. Mouton, alias di Ferdinand La Menthe, opp. La Mothe, New Orleans, 20 ott ~1885 - Los Angeles, 10 luglio 1941, ~56a).  Ref: Alan Lomax. "Mister Jelly Roll". Duell, Sloan & Pearce, New York (1950);  cit. in: Arrigo Polillo, "JAZZ". Oscar Saggi Mondadori. (1977):315,325.

http://inkpi.blogspot.it/search?q=jelly+roll

martedì 1 agosto 2017

# s-astro: cosmic nomads, transfers, impacts

a) cosmic nomads

Lee Billings. Wandering in the Void, Billions of Rogue Planets without a Home. New results suggest free-floating giant planets are less common than previously believed, but hint at vast numbers of smaller castaway worlds. July 24, 2017

https://www.scientificamerican.com/article/wandering-in-the-void-billions-of-rogue-planets-without-a-home/

b) cosmic transfers

Ashley Yeager. Half of the Milky Way comes from other galaxies
Simulations suggest that galactic winds blew the material in from elsewhere. July 26, 2017

https://www.sciencenews.org/article/half-milky-way-comes-other-galaxies

Daniel Angles-Alcazar
Claude-Andre Faucher-Giguere
et al. The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations. Mon Not R Astron Soc (2017) 470 (4): 4698-4719. doi: 10.1093/mnras/stx1517
Publ. June 20, 2017

https://academic.oup.com/mnras/article-abstract/doi/10.1093/mnras/stx1517/3871367/The-Cosmic-Baryon-Cycle-and-Galaxy-Mass-Assembly

c) cosmic impacts

Jenny Wells. Evidence of impacts that structured the Milky Way galaxy. July 18, 2017

https://m.phys.org/news/2017-07-evidence-impacts-milky-galaxy.html

Deborah Ferguson, Susan Gardner, Brian Yanny. Milky Way Tomography with K and M Dwarf Stars: The Vertical Structure of the Galactic Disk. The American Astronomical Society. The Astrophysical Journal, Volume 843, Number 2 . Publ. July 14, 2017.

http://iopscience.iop.org/article/10.3847/1538-4357/aa77fd/meta

giovedì 7 marzo 2019

# gst astro: approaches to hack a black hole (to distinguish scrambled information from noise)

paper.1

Adam Mann. Physicists May Have Found a Way to 'Untangle' Information Trapped in a Black Hole. Mar 6, 2019

https://www.livescience.com/64935-black-hole-information-paradox.html

K. A. Landsman, C. Figgatt, et al. Verified quantum information scrambling. Nature. volume 567, pages 61–65 (2019) Mar 6,  2019.

https://www.nature.com/articles/s41586-019-0952-6

paper.2

Mike McRae. Physicists Want to Use Quantum Particles to Find Out What Happens Inside a Black Hole. Mar 6, 2019.

https://www.sciencealert.com/entangled-particles-could-help-reveal-the-hidden-workings-of-black-holes

Beni Yoshida, Norman Y. Yao. Disentangling Scrambling and Decoherence via Quantum Teleportation. Phys. Rev. X 9, 011006. Jan 9, 2019

https://journals.aps.org/prx/abstract/10.1103/PhysRevX.9.011006

martedì 9 agosto 2016

# s-astro: and come out the other side

<< One  of  the  biggest  problems  when  studying  black  holes  is  that  the  laws  of  physics  as  we  know them  cease  to  apply  in  their  deepest  regions.  Large  quantities  of  matter  and  energy  concentrate in  an  infinitely  small  space,  the  gravitational  singularity,  where  space-time  curves  towards  infinity and  all  matter  is  destroyed.  Or  is  it?  A  recent  study  (..)  suggests  that  matter  might  in  fact  survive  its  foray  into these  space  objects  and  come  out  the  other  side. >>

Do  black  holes  have  a  back  door?  R&I World. 9 Aug 2016.

http://ruvid.org/ri-world/black-holes-might-have-a-back-door/

Gonzalo  J  Olmo ,  D  Rubiera-Garcia   and  A  Sanchez-Puente. Impact  of  curvature  divergences  on  physical observers  in  a  wormhole  space–time  with  horizons.  Classical  and  Quantum  Gravity,  Volume  33,  Number  11. Published  28  April  2016.

http://dx.doi.org/10.1088/0264-9381/33/11/115007

lunedì 17 ottobre 2022

# life: a proposito di bizzarri scenari, qui un ipotetico scenario22 dipinto dal reale ...

img: Congo Square, New Orleans, Louisiana (wikipedia.org)

In definitiva qui si configurerebbe un - intrigante assai - scenario che, grosso modo, si potrebbe sinteticamente 'dipingere' in questi termini: 

(i) entità tre palle destrogire, animate aciclicamente da interazioni attrattive- repulsive a causa di già a suo tempo disvelate pulsioni neuro cognitive arcaiche, riconducibili a visioni neuro predatorie CTZ estreme, perciò ipoteticamente (si fa per dire) a-priori ad esiti immediati e in prospettiva drammaticamente lesivi- autolesivi; 

(ii) entità tre palle levogire, animate da analoghe pulsività, purtuttavia in.forme  tenui, in modalità sottotraccia, frenate da feed-back a modalità allosterica, ombreggiate, stemperate, diluite, discrete, timidamente celate, talvolta fantasmatiche perfino, quasi ma non del tutto mai silenti, perciò anch'esse a tutti gli effetti operative, sebbene a dinamiche più fluide, lente, meno dirompenti rispetto alle destrogire; 

(iii) entrambe l'Entità destrogire e levogire animat(t)rici,  generat(t)rici di dinamiche bi-multi-forcate, transeunti, con picchi di improvvisi aciclici burst ad effetti RAG-time diretti e inversi;

(iv) lo scenario al contorno e forse anche all'interno, nei vari specifici contesti, riconducibile grosso modo alla formazione aciclica di ipotetici buchi neri non inerti, caratterizzati da aciclicità in compressione e dilatazione - come fossero fisarmoniche - animati (in perpetuo?) da multi vortici in ingresso e in uscita;

Non so se basti compulsare un manuale delle funzioni speciali per formalizzare in qualche adatto topo-modo questo pulsatile multi scenario, purtuttavia assolutamente intrigante ... 

Qui una AI operativa nella formalizzazione di analogie potrebbe modellizzare, forse ... (e.g. https://flashontrack.blogspot.com/2021/08/aibot-mechanism-of-analogy-could-be.html )

Quello che appare evidente è la complessità d'insieme, un bizzarro dipinto, uno scenario dinamico che, al confronto, le storiche danze in Congo Square potrebbero sembrare semplici, ordinate coreografie ... queste, rispetto a quelle, delle topo-forme  'primitive', per dire ed anzicheforse.

In sintesi, i riferimenti (ovviamente generici) del bizzarro scenario: 

(:) buco nero con vortici 

(:) scenari generati da 3 palle 
(a)
(b)

(:) effetti RAG-time (RAG: Ralph, Al, George) 
(a) (quasi-stochastic poetry)
(b)

(:) pulsioni predatorie supportate / giustificate da visioni neuro- post- CTZ nelle modalità arcaiche oppure friendly 

(:) Congo Square, jazz 
(a)
(b)
(c) (quasi-stochastic poetry)

(:) approccio Bertalanffy 

(:) un bizzarro tracciatore 

Anche

"Amico, qualunque cosa suonerai ... "
(a) (quasi-stochastic poetry)
(b)

Keywords: life, gst, Congo Square, jazz, Jelly Roll, transition, three-body, RAG, CTZ, black hole, bizarre tracker