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YSM Issue 90.4

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FOCUS<br />

particle physics<br />

IMAGE COURTESY OF BERKELEY LABS<br />

►The color charge acts such all matter must be<br />

locally white, binding quarks into combinations<br />

that preserve this colorlessness and preventing<br />

the sustained existence of free quarks.<br />

IMAGE COURTESY OF GETTY IMAGES<br />

►This image, taken near RHIC at Brookhaven<br />

Laboratory depicts a subset of the STAR<br />

collaboration.<br />

Any angular momentum in the system will<br />

be passed on to the particles it generates,<br />

whose spins are aligned with the whirling<br />

structures from which they came. On average,<br />

those spins will indicate the net angular<br />

momentum created by the system. As<br />

Yale’s Professor Caines, spokesperson for<br />

the collaboration described, “when you collide<br />

them just a little bit edge on edge you<br />

set it spinning, and that’s basically what we<br />

measured, how fast it’s spinning collectively.<br />

We can detect that angular momentum.”<br />

The experiment used two instruments for<br />

this measurement. The first of these was the<br />

Time Project Chamber, which is filled with<br />

gas that surrounds the collision and allows<br />

scientists to track the particles released<br />

from the collision and therefore generated<br />

by the QGP. This detector measures protons<br />

created by the plasma. The second instrument,<br />

the Beam-Beam Counters, measures<br />

deflections in the paths of particles which<br />

whiz by one another and indicates the magnitude<br />

and direction of angular momentum<br />

in each collision. Correlating this measured<br />

angular momentum with aligned direction<br />

of the detected protons, STAR scientists<br />

searched for preference in direction that<br />

will indicate the vorticity of the system.<br />

This measurement indicates that the<br />

QGP is the most vortical fluid known, a<br />

measured value surprising in its magnitude.<br />

The vorticity of the QGP exceeded<br />

all predicted values – whirling faster than<br />

tornados, Jupiter’s red spot, and previous<br />

vorticity record-holder superfluid helium.<br />

This high vorticity is allowed to perpetuate<br />

by the low viscosity of the fluid – since high<br />

resistance to flow would dampen whirls prior<br />

to measurement. Vorticity is a property of<br />

the flow – it’s not intrinsic to the medium,<br />

but results from the medium and its motion.<br />

But since we know the conditions that<br />

produced the flow inside of the collider, it’s<br />

possible to gain useful information about<br />

the fluid properties. Knowing the specifics<br />

of the collision that generated it allows us to<br />

firm up our theories of how the QGP interacts<br />

and responds to forces.<br />

Changes in temperature and pressure induce<br />

phase transitions. Think briefly of ice:<br />

increasing the temperature will turn it to<br />

water, then to vapor. At 4 trillion degrees<br />

Celcius, the quark gluon plasma is very hot,<br />

which is why the strong mutual interactions<br />

of its constituent particles is puzzling. The<br />

QGP behaves more like a fluid than like a<br />

gas. Instead of expanding out evenly in all<br />

directions, it’s preferential in its flow. Is it a<br />

relic of the strong force, which governs interactions<br />

between its constituent parts? Or<br />

perhaps the extreme pressure of the cosmic<br />

soup? In future experiments, the STAR collaboration<br />

hopes to deduce the equation of<br />

state for the quark gluon plasma to resolve<br />

these questions and test theories about the<br />

strong force.<br />

This vorticity measurement will aid in<br />

improving theories of the plasma and how<br />

it affected the properties of the early universe.<br />

Most importantly, spinning charges<br />

produce magnetic fields, making this measurement<br />

an important first step in making<br />

the first measurements of the magnetic<br />

properties of the QGP, an important step<br />

in better understanding the weird physics<br />

surrounding this hot, flowy, whirling<br />

soup. Although the significance of such<br />

fundamental science isn’t always immediately<br />

clear, Yale’s Li Yi, a scientist with the<br />

collaboration sees this as exciting infinite<br />

possibility. “Maybe it sounds like science<br />

fiction, but in all of the modern world most<br />

of the technology is based on QED (quantum<br />

electro dynamics), our theory of the<br />

electromagnetic force. For example, we<br />

transfer the messages and communications<br />

through electromagnetic waves - this is all<br />

through the QED because we really understand<br />

what we can do. QCD we don’t know<br />

exactly how it works - or what we could use<br />

it for.” The STAR Collaboration’s measurements<br />

of the QGP are among the most important<br />

measurements for formulating and<br />

testing this theory.<br />

ABOUT THE AUTHOR<br />

SOPHIA SANCHEZ-MAES<br />

SOPHIA SANCHEZ-MAES is a junior Physics and Astrophysics double major<br />

in Timothy Dwight college. She works with Professor Jun Korenaga on studying<br />

the origin processes of plate tectonics, and topics in complex systems.<br />

THE AUTHOR WOULD LIKE TO THANK Professor Helen Caines and Dr. Li<br />

Yi for their incredible knowledge and willingness to share it.<br />

FURTHER READING<br />

The Star Collaboration. (2017). Global Λ hyperon polarization in nuclear<br />

collisions. Nature. Retrieved October 1, 2017.<br />

14 Yale Scientific Magazine October 2017 www.yalescientific.org

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