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Cryogenic Camera for High Voltage Monitoring in Liquid Xenon Cryogenic Camera for High Voltage Monitoring in Liquid Xenon Amalia Badohu Columbia University REU Program 2021 Email: [email protected] The evidence that has been found for Dark Matter becomes increasingly more prevalent as the years pass and scientific technology becomes more sensitive and advanced. Direct detection of Dark Matter through the use of the XenonnT detector in Gran Sasso is the largest most precise vessel currently constructed. The REU students in the Xenon group were able to construct and test a vessel to house a camera in cryogenic conditions that would be able to record the interactions between Dark Matter and Xenon nuclei. Keywords: Cryogenics; Xenon; Dark Matter; Experimental Analysis; Vessel Construction Received 06 August 2021 1. INTRODUCTION for cosmological use. The free non-reactive properties of dark matter are predicted to be the matter that molded 1.1. Dark Matter the self-interactive clumping of luminous matter in the Early astronomers focused much of their calculations beginnings of the universe[2]. Thus the clustering of and observations of space on the luminous matter that galaxies and stars in the night sky can be attributed to was able to be understood based on the scientific dark matter's observed properties (See Figure 1). Given advancements created by their predecessors. One of the many calculations of the speed and rotational curves the earliest more concrete possible examples of the of stars that have been calculated, scientists are forced existence of Dark Matter in our universe comes from to consider that there is matter fixing these stars in the the astronomer Fritz Zwicky in the 1930s. Zwicky used space of their galaxies rather than flying off into deep the luminosity of galaxies to calculate their velocity. space. Zwicky focused on the Coma Cluster of galaxies and found a huge discrepancy in the values of velocity he 1.2. The Bullet Cluster calculated using luminosity based on his use of the Hubble parameter[1]. This large difference in values Another more prevalent example of direct evidence for allowed him to hypothesize that a large factor of the Dark Matter and its properties is the observation of matter found in these galaxies and ultimately in the the interactions of the Bullet Cluster. The two galaxies universe, is non-luminous matter. crossed paths and were able to carry on unaffected by The evidence of dark matter in the cosmos has been the other. The hot gas clouds surrounding them reacted an integral part of the creation of the standard model with one another and pulled them off of the galaxies FIGURE 1. Galaxy formation over time due to Dark Matter and it's web like properties FIGURE 2. Interactions of baryonic gas between two galaxies. (see Figure 2). This allowed astronomers to recalculate the masses of the galaxies by using gravitational with overtime. We employ these options of detection lensing[3]. Gravitational lensing occurs when large and production in order to gain more knowledge amounts of matter distort light from stars behind of the dark matter, identify individual dark matter them because of the magnitude of their gravitational particles, and observe possible interactions that are field. Researchers were able to witness the gravitational non-gravitational. Direct detection of dark matter properties of the dark matter surrounding the galaxy focuses on the interaction of the dark matter and by the significant increase in the amount of light atoms we have studied and understand. Indirect that was bent by the observed matter. This is great detection focuses on searching for dark matter using evidence for the existence of dark matter because the γ rays, charged cosmic rays, X-rays, microwaves, etc. comparison between previous gravitational lensing and Production experiments focus on trying to create dark this experiment shows how the dark matter around the matter on earth in experiments such as CERN, LHC, galaxy increased the amount of gravitational pull that etc. the matter in that region experienced. Based on what 2. THE XENON EXPERIMENT we know from many observations about dark matter's gravitational abundance, this offers a clear example of This form of detection of dark matter is considered the an increase in gravity that has no other reasonable scattering of atoms. The Xenon experiment uses a very explanation. Similarly, this is great evidence for the large dual-phase time projection chamber(TPC) that low self interactions of dark matter because of the lack records interactions between Xenon nuclei and dark of reactions between the dark matter surrounding each matter particle candidates such as weakly interacting galaxy as they collided. Without the dark matter we mega particles or WIMPs (See Figure 3). would expect to see clear reactions between the atoms in The liquid Xenon atoms in motion excite some of the galaxies, giving us great evidence for the existence the surrounding Xenon atoms and ionize others. The of dark matter in the formation of our galaxies. excited atoms emit photons of light detected by the Photo-multiplier tubes lining the top and bottom of 1.3. Methods for understanding Dark Matter the vessel. We call this light scintillation light and it There are a few different methods for studying and is denoted in this step as the S1 signal output. understanding dark matter that scientists have come up The electrons freed by ionization are then drawn 2 experiment to rule out impossible scattering. 2.1. The 2021 REU Project The impacts of COVID-19 are still making lab work and collaboration strained as safety regulations force countries to remain separate and communicate through online channels such as zoom. Despite these complications, the students chosen for the 2020 summer FIGURE 3. Schematic of Xenon interaction dual phase program were offered the chance to participate in the TPC . summer of 2021 despite any changes in eligibility. The students were also allowed to attend the program towards the anode where they will react again with in person if they so chose to. This allowed the the molecules of gaseous Xenon in the second phase 2021 XENON group students to take part in an of the chamber. The strong electric field in the exciting hands-on project of the experimental design gaseous Xenon section of the chamber accelerates these of a cryogenic camera vessel to record the interactions electrons enough to cause a larger flash of light upon between Xenon nuclei and dark matter particles inside collision which we denote as the S2 signal output the XENONnT and future versions. The students The pattern of the S2 signal gives data relevant began with research and reading into the XENON to the transverse position of the interaction of experiments, cryogenic hardware, cryogenic camera molecules inside the chamber, as well as allowing the testing, etc. The students began with basic tasks researcher to separate the interactions classified as Dark to prepare for the construction of the camera vessel. Matter collision events and events of other radioactive Sanitizing flanges, copper gaskets, and the inside of contaminants. While the time between reactions in S1 the vessel itself. Proper sanitization was important and S2 tells researchers the depth of the reaction inside for keeping the conditions of the chamber at expected the chamber. values. We also wanted a pure system to ensure we We house this experiment inside of the Gran Sasso could recycle the Xenon for future use. The students mountain in Italy for many reasons. First, the gained great experience with wire working and electrical experiment is very large so the space needed to house understanding. Students were able to unsolder multipin this experiment needed to be very big in order to safely connectors, solder wiring, prepare wires for connection, complete it. Secondly, the location is important for etc. To prepare the wires, students cut the connector performing scattering experiments on earth because side of the AC wire off, stripped the smaller wires inside, experimenters must ensure that the interactions they and crimped the individual loose wires with ferrules for are witnessing are that of actual dark matter candidates easier and cleaner connection of the PAX-P and PAX-T and not other particles and matter. Housing this deep output controllers (See Figures 5 and 6). inside the mountain ensures that cosmic radiation and The construction of the outer chamber involved rays are not able to make it through the water tank carefully connecting flanges, making sure not to scrape and the many layers of the mountain's rock. We use any metal pieces to ensure the connections would be the Monte Carlo simulations to set a basis for the true with no possible leaks. As well as tightening the types of interactions we expect to encounter during the screws and learning to use torque wrenches to tighten 3 FIGURE 4. Sanitization of the camera housing vessel using ethyl alcohol FIGURE 6. Pressure and Temperature controllers that students made the wires for connection to the vessel (Bottom row) magnitude of 10 (See Figure 7). Students then were able to test the connection of the flanges and other ports by spraying a small amount of Helium gas into the small test ports in all of the connections (See Figure 8). This test is not something many physics students get to see a side of when taking part in experiments because they focused more heavily on data analysis. But this gave the students a great example of how experimental the FIGURE 5. Ferrules crimped on the connector end of and AC power cord for PAX-(P/T) construction of the test chambers are and how much care and testing is needed for the apparati before they're flange connections and stretch screws to the point of given to scientists for their experimental usage.
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