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  1. Book ; Online: Optimized Designs for Very Low Temperature Massive Calorimeters

    Pyle, Matt / Figueroa-Feliciano, Enectali / Sadoulet, Bernard

    2015  

    Abstract: The baseline energy-resolution performance for the current generation of large-mass, low-temperature calorimeters (utilizing TES and NTD sensor technologies) is $>2$ orders of magnitude worse than theoretical predictions. A detailed study of several ... ...

    Abstract The baseline energy-resolution performance for the current generation of large-mass, low-temperature calorimeters (utilizing TES and NTD sensor technologies) is $>2$ orders of magnitude worse than theoretical predictions. A detailed study of several calorimetric detectors suggests that a mismatch between the sensor and signal bandwidths is the primary reason for suppressed sensitivity. With this understanding, we propose a detector design in which a thin-film Au pad is directly deposited onto a massive absorber that is then thermally linked to a separately fabricated TES chip via an Au wirebond, providing large electron-phonon coupling (i.e. high signal bandwidth), ease of fabrication, and cosmogenic background suppression. Interestingly, this design strategy is fully compatible with the use of hygroscopic crystals (NaI) as absorbers. An 80-mm diameter Si light detector based upon these design principles, with potential use in both dark matter and neutrinoless double beta decay, has an estimated baseline energy resolution of 0.35 eV, 20$\times$ better than currently achievable. A 1.75 kg ZnMoO$_{4}$ large-mass calorimeter would have a 3.5 eV baseline resolution, 1000$\times$ better than currently achieved with NTDs with an estimated position dependence $\frac{\Delta E}{E}$ of 6$\times$10$^{-4}$. Such minimal position dependence is made possible by forcing the sensor bandwidth to be much smaller than the signal bandwidth. Further, intrinsic event timing resolution is estimated to be $\sim$170 $\mu$s for 3 MeV recoils in the phonon detector, satisfying the event-rate requirements of large $Q_{\beta \beta}$ next-generation neutrinoless double beta decay experiments. Quiescent bias power for both of these designs is found to be significantly larger than parasitic power loads achieved in the SPICA/SAFARI infrared bolometers.

    Comment: 16 pages, 12 figures
    Keywords Astrophysics - Instrumentation and Methods for Astrophysics ; Physics - Instrumentation and Detectors
    Subject code 621
    Publishing date 2015-03-03
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  2. Book ; Online: Micro-X Sounding Rocket Payload Re-flight Progress

    Adams, J. S. / Bandler, S. R. / Bastidon, N. / Eckart, M. E. / Figueroa-Feliciano, E. / Fuhrman, J. / Goldfinger, D. C. / Hubbard, A. J. F. / Jardin, D. / Kelley, R. L. / Kilbourne, C. A. / Manzagol-Harwood, R. E. / McCammon, D. / Okajima, T. / Porter, F. S. / Reintsema, C. D. / Smith, S. J.

    2021  

    Abstract: Micro-X is an X-ray sounding rocket payload that had its first flight on July 22, 2018. The goals of the first flight were to operate a transition edge sensor (TES) X-ray microcalorimeter array in space and take a high-resolution spectrum of the ... ...

    Abstract Micro-X is an X-ray sounding rocket payload that had its first flight on July 22, 2018. The goals of the first flight were to operate a transition edge sensor (TES) X-ray microcalorimeter array in space and take a high-resolution spectrum of the Cassiopeia A supernova remnant. The first flight was considered a partial success. The array and its time-division multiplexing readout system were successfully operated in space, but due to a failure in the attitude control system, no time on-target was acquired. A re-flight has been scheduled for summer 2022. Since the first flight, modifications have been made to the detector systems to improve noise and reduce the susceptibility to magnetic fields. The three-stage SQUID circuit, NIST MUX06a, has been replaced by a two-stage SQUID circuit, NIST MUX18b. The initial laboratory results for the new detector system will be presented in this paper.

    Comment: LTD proceedings, 6 pages, 3 figures, 1 table
    Keywords Astrophysics - Instrumentation and Methods for Astrophysics ; Physics - Instrumentation and Detectors
    Subject code 629
    Publishing date 2021-11-12
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  3. Book ; Online: G4CMP

    Kelsey, M. H. / Agnese, R. / Alam, Y. F. / Langroudy, I. Ataee / Azadbakht, E. / Brandt, D. / Bunker, R. / Cabrera, B. / Chang, Y. -Y. / Coombes, H. / Cormier, R. M. / Diamond, M. D. / Edwards, E. R. / Figueroa-Feliciano, E. / Gao, J. / Harrington, P. M. / Hong, Z. / Hui, M. / Kurinsky, N. A. /
    Lawrence, R. E. / Loer, B. / Masten, M. G. / Michaud, E. / Michielin, E. / Miller, J. / Novati, V. / Oblath, N. S. / Orrell, J. L. / Perry, W. L. / Redl, P. / Reynolds, T. / Saab, T. / Sadoulet, B. / Serniak, K. / Singh, J. / Speaks, Z. / Stanford, C. / Stevens, J. R. / Strube, J. / Toback, D. / Ullom, J. N. / VanDevender, B. A. / Vissers, M. R. / Wilson, M. J. / Wilson, J. S. / Zatschler, B. / Zatschler, S.

    Condensed Matter Physics Simulation Using the Geant4 Toolkit

    2023  

    Abstract: G4CMP simulates phonon and charge transport in cryogenic semiconductor crystals using the Geant4 toolkit. The transport code is capable of simulating the propagation of acoustic phonons as well as electron and hole charge carriers. Processes for ... ...

    Abstract G4CMP simulates phonon and charge transport in cryogenic semiconductor crystals using the Geant4 toolkit. The transport code is capable of simulating the propagation of acoustic phonons as well as electron and hole charge carriers. Processes for anisotropic phonon propagation, oblique charge-carrier propagation, and phonon emission by accelerated charge carriers are included. The simulation reproduces theoretical predictions and experimental observations such as phonon caustics, heat-pulse propagation times, and mean charge-carrier drift velocities. In addition to presenting the physics and features supported by G4CMP, this report outlines example applications from the dark matter and quantum information science communities. These communities are applying G4CMP to model and design devices for which the energy transported by phonons and charge carriers is germane to the performance of superconducting instruments and circuits placed on silicon and germanium substrates. The G4CMP package is available to download from GitHub: github.com/kelseymh/G4CMP.

    Comment: 21 pages, 11 figures, 10 tables
    Keywords High Energy Physics - Experiment ; Quantum Physics
    Subject code 621
    Publishing date 2023-02-12
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  4. Article: Lynx x-ray microcalorimeter.

    Bandler, Simon R / Chervenak, James A / Datesman, Aaron M / Devasia, Archana M / DiPirro, Michael / Sakai, Kazuhiro / Smith, Stephen J / Stevenson, Thomas R / Yoon, Wonsik / Bennett, Douglas / Mates, Benjamin / Swetz, Daniel / Ullom, Joel N / Irwin, Kent D / Eckart, Megan E / Figueroa-Feliciano, Enectali / McCammon, Dan / Ryu, Kevin / Olson, Jeffrey /
    Zeiger, Ben

    Journal of astronomical telescopes, instruments, and systems

    2019  Volume 5, Issue 2, Page(s) 21017

    Abstract: Lynx is an x-ray telescope, one of four large satellite mission concepts currently being studied by NASA to be a flagship mission. One of Lynx's three instruments is an imaging spectrometer called the Lynx x-ray microcalorimeter (LXM), an x-ray ... ...

    Abstract Lynx is an x-ray telescope, one of four large satellite mission concepts currently being studied by NASA to be a flagship mission. One of Lynx's three instruments is an imaging spectrometer called the Lynx x-ray microcalorimeter (LXM), an x-ray microcalorimeter behind an x-ray optic with an angular resolution of 0.5 arc sec and ∼2 m
    Language English
    Publishing date 2019-05-31
    Publishing country United States
    Document type Journal Article
    ISSN 2329-4124
    ISSN 2329-4124
    DOI 10.1117/1.JATIS.5.2.021017
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  5. Article ; Online: First Measurement of the Nuclear-Recoil Ionization Yield in Silicon at 100 eV.

    Albakry, M F / Alkhatib, I / Alonso, D / Amaral, D W P / Aralis, T / Aramaki, T / Arnquist, I J / Ataee Langroudy, I / Azadbakht, E / Banik, S / Bathurst, C / Bhattacharyya, R / Brink, P L / Bunker, R / Cabrera, B / Calkins, R / Cameron, R A / Cartaro, C / Cerdeño, D G /
    Chang, Y-Y / Chaudhuri, M / Chen, R / Chott, N / Cooley, J / Coombes, H / Corbett, J / Cushman, P / Das, S / De Brienne, F / Rios, M / Dharani, S / di Vacri, M L / Diamond, M D / Elwan, M / Fascione, E / Figueroa-Feliciano, E / Fink, C W / Fouts, K / Fritts, M / Gerbier, G / Germond, R / Ghaith, M / Golwala, S R / Hall, J / Harms, S A S / Hassan, N / Hines, B A / Hong, Z / Hoppe, E W / Hsu, L / Huber, M E / Iyer, V / Kashyap, V K S / Kelsey, M H / Kubik, A / Kurinsky, N A / Lee, M / Litke, M / Liu, J / Liu, Y / Loer, B / Lopez Asamar, E / Lukens, P / MacFarlane, D B / Mahapatra, R / Mast, N / Mayer, A J / Meyer Zu Theenhausen, H / Michaud, É / Michielin, E / Mirabolfathi, N / Mohanty, B / Nebolsky, B / Nelson, J / Neog, H / Novati, V / Orrell, J L / Osborne, M D / Oser, S M / Page, W A / Pandey, L / Pandey, S / Partridge, R / Pedreros, D S / Perna, L / Podviianiuk, R / Ponce, F / Poudel, S / Pradeep, A / Pyle, M / Rau, W / Reid, E / Ren, R / Reynolds, T / Tanner, E / Roberts, A / Robinson, A E / Saab, T / Sadek, D / Sadoulet, B / Sahoo, S P / Saikia, I / Sander, J / Sattari, A / Schmidt, B / Schnee, R W / Scorza, S / Serfass, B / Poudel, S S / Sincavage, D J / Sinervo, P / Speaks, Z / Street, J / Sun, H / Terry, G D / Thasrawala, F K / Toback, D / Underwood, R / Verma, S / Villano, A N / von Krosigk, B / Watkins, S L / Wen, O / Williams, Z / Wilson, M J / Winchell, J / Wykoff, K / Yellin, S / Young, B A / Yu, T C / Zatschler, B / Zatschler, S / Zaytsev, A / Zeolla, A / Zhang, E / Zheng, L / Zheng, Y / Zuniga, A / An, P / Barbeau, P S / Hedges, S C / Li, L / Runge, J

    Physical review letters

    2023  Volume 131, Issue 9, Page(s) 91801

    Abstract: We measured the nuclear-recoil ionization yield in silicon with a cryogenic phonon-sensitive gram-scale detector. Neutrons from a monoenergetic beam scatter off of the silicon nuclei at angles corresponding to energy depositions from 4 keV down to 100 eV, ...

    Abstract We measured the nuclear-recoil ionization yield in silicon with a cryogenic phonon-sensitive gram-scale detector. Neutrons from a monoenergetic beam scatter off of the silicon nuclei at angles corresponding to energy depositions from 4 keV down to 100 eV, the lowest energy probed so far. The results show no sign of an ionization production threshold above 100 eV. These results call for further investigation of the ionization yield theory and a comprehensive determination of the detector response function at energies below the keV scale.
    Language English
    Publishing date 2023-09-18
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.131.091801
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  6. Book ; Online: Comparison of CDMS [100] and [111] oriented germanium detectors

    Leman, S. W. / Hertel, S. A. / Kim, P. / Cabrera, B. / Silva, E. Do Couto E / Figueroa-Feliciano, E. / McCarthy, K. A. / Resch, R. / Sadoulet, B. / Sundqvist, K. M.

    2011  

    Abstract: The Cryogenic Dark Matter Search (CDMS) utilizes large mass, 3" diameter $\times$ 1" thick target masses as particle detectors. The target is instrumented with both phonon and ionization sensors and comparison of energy in each channel provides event-by- ... ...

    Abstract The Cryogenic Dark Matter Search (CDMS) utilizes large mass, 3" diameter $\times$ 1" thick target masses as particle detectors. The target is instrumented with both phonon and ionization sensors and comparison of energy in each channel provides event-by-event classification of electron and nuclear recoils. Fiducial volume is determined by the ability to obtain good phonon and ionization signal at a particular location. Due to electronic band structure in germanium, electron mass is described by an anisotropic tensor with heavy mass aligned along the symmetry axis defined by the [111] Miller index (L valley), resulting in large lateral component to the transport. The spatial distribution of electrons varies significantly for detectors which have their longitudinal axis orientations described by either the [100] or [111] Miller indices. Electric fields with large fringing component at high detector radius also affect the spatial distribution of electrons and holes. Both effects are studied in a 3 dimensional Monte Carlo and the impact on fiducial volume is discussed.

    Comment: Low Temperature Detector 14 conference proceedings to be published in the Journal of Low Temperature Physics
    Keywords Physics - Instrumentation and Detectors ; Astrophysics - Instrumentation and Methods for Astrophysics ; Condensed Matter - Materials Science ; High Energy Physics - Experiment
    Subject code 541
    Publishing date 2011-08-31
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  7. Book ; Online: Phonon Quasidiffusion in Cryogenic Dark Matter Search Large Germanium Detectors

    Leman, S. W. / Cabrera, B. / McCarthy, K. A. / Pyle, M. / Resch, R. / Sadoulet, B. / Sundqvist, K. M. / Brink, P. L. / Cherry, M. / Silva, E. Do Couto E / Figueroa-Feliciano, E. / Mirabolfathi, N. / Serfass, B. / Tomada, A.

    2011  

    Abstract: We present results on quasidiffusion studies in large, 3 inch diameter, 1 inch thick [100] high purity germanium crystals, cooled to 50 mK in the vacuum of a dilution refrigerator, and exposed with 59.5 keV gamma-rays from an Am-241 calibration source. ... ...

    Abstract We present results on quasidiffusion studies in large, 3 inch diameter, 1 inch thick [100] high purity germanium crystals, cooled to 50 mK in the vacuum of a dilution refrigerator, and exposed with 59.5 keV gamma-rays from an Am-241 calibration source. We compare data obtained in two different detector types, with different phonon sensor area coverage, with results from a Monte Carlo. The Monte Carlo includes phonon quasidiffusion and the generation of phonons created by charge carriers as they are drifted across the detector by ionization readout channels.

    Comment: 13 pages, 12 figures, PHONONS201 conference proceedings; http://psroc.phys.ntu.edu.tw/cjp/download.php?d=4&pid=2718
    Keywords Physics - Instrumentation and Detectors ; Condensed Matter - Materials Science ; High Energy Physics - Experiment
    Publishing date 2011-07-18
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  8. Book ; Online: Monte Carlo Comparisons to a Cryogenic Dark Matter Search Detector with low Transition-Edge-Sensor Transition Temperature

    Leman, S. W. / McCarthy, K. A. / Brink, P. L. / Cabrera, B. / Cherry, M. / Silva, E. Do Couto E / Figueroa-Feliciano, E. / Kim, P. / Mirabolfathi, N. / Pyle, M. / Resch, R. / Sadoulet, B. / Serfass, B. / Sundqvist, K. M. / Tomada, A. / Young, B. A.

    2011  

    Abstract: We present results on phonon quasidiffusion and Transition Edge Sensor (TES) studies in a large, 3 inch diameter, 1 inch thick [100] high purity germanium crystal, cooled to 50 mK in the vacuum of a dilution refrigerator, and exposed with 59.5 keV gamma- ... ...

    Abstract We present results on phonon quasidiffusion and Transition Edge Sensor (TES) studies in a large, 3 inch diameter, 1 inch thick [100] high purity germanium crystal, cooled to 50 mK in the vacuum of a dilution refrigerator, and exposed with 59.5 keV gamma-rays from an Am-241 calibration source. We compare calibration data with results from a Monte Carlo which includes phonon quasidiffusion and the generation of phonons created by charge carriers as they are drifted across the detector by ionization readout channels. The phonon energy is then parsed into TES based phonon readout channels and input into a TES simulator.
    Keywords Physics - Instrumentation and Detectors ; Astrophysics - Instrumentation and Methods for Astrophysics ; Condensed Matter - Materials Science
    Publishing date 2011-09-06
    Publishing country us
    Document type Book ; Online
    Database BASE - Bielefeld Academic Search Engine (life sciences selection)

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  9. Article ; Online: Constraints on Lightly Ionizing Particles from CDMSlite.

    Alkhatib, I / Amaral, D W P / Aralis, T / Aramaki, T / Arnquist, I J / Ataee Langroudy, I / Azadbakht, E / Banik, S / Barker, D / Bathurst, C / Bauer, D A / Bezerra, L V S / Bhattacharyya, R / Bowles, M A / Brink, P L / Bunker, R / Cabrera, B / Calkins, R / Cameron, R A /
    Cartaro, C / Cerdeño, D G / Chang, Y-Y / Chaudhuri, M / Chen, R / Chott, N / Cooley, J / Coombes, H / Corbett, J / Cushman, P / De Brienne, F / di Vacri, M L / Diamond, M D / Fascione, E / Figueroa-Feliciano, E / Fink, C W / Fouts, K / Fritts, M / Gerbier, G / Germond, R / Ghaith, M / Golwala, S R / Harris, H R / Hines, B A / Hollister, M I / Hong, Z / Hoppe, E W / Hsu, L / Huber, M E / Iyer, V / Jardin, D / Jastram, A / Kashyap, V K S / Kelsey, M H / Kubik, A / Kurinsky, N A / Lawrence, R E / Li, A / Loer, B / Lopez Asamar, E / Lukens, P / MacFarlane, D B / Mahapatra, R / Mandic, V / Mast, N / Mayer, A J / Meyer Zu Theenhausen, H / Michaud, É M / Michielin, E / Mirabolfathi, N / Mohanty, B / Morales Mendoza, J D / Nagorny, S / Nelson, J / Neog, H / Novati, V / Orrell, J L / Oser, S M / Page, W A / Partridge, R / Podviianiuk, R / Ponce, F / Poudel, S / Pradeep, A / Pyle, M / Rau, W / Reid, E / Ren, R / Reynolds, T / Roberts, A / Robinson, A E / Saab, T / Sadoulet, B / Sander, J / Sattari, A / Schnee, R W / Scorza, S / Serfass, B / Sincavage, D J / Stanford, C / Street, J / Toback, D / Underwood, R / Verma, S / Villano, A N / von Krosigk, B / Watkins, S L / Wilson, J S / Wilson, M J / Winchell, J / Wright, D H / Yellin, S / Young, B A / Yu, T C / Zhang, E / Zhang, H G / Zhao, X / Zheng, L

    Physical review letters

    2021  Volume 127, Issue 8, Page(s) 81802

    Abstract: The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to lightly ionizing particles (LIPs) in a previously unexplored ... ...

    Abstract The Cryogenic Dark Matter Search low ionization threshold experiment (CDMSlite) achieved efficient detection of very small recoil energies in its germanium target, resulting in sensitivity to lightly ionizing particles (LIPs) in a previously unexplored region of charge, mass, and velocity parameter space. We report first direct-detection limits calculated using the optimum interval method on the vertical intensity of cosmogenically produced LIPs with an electric charge smaller than e/(3×10^{5}), as well as the strongest limits for charge ≤e/160, with a minimum vertical intensity of 1.36×10^{-7}  cm^{-2} s^{-1} sr^{-1} at charge e/160. These results apply over a wide range of LIP masses (5  MeV/c^{2} to 100  TeV/c^{2}) and cover a wide range of βγ values (0.1-10^{6}), thus excluding nonrelativistic LIPs with βγ as small as 0.1 for the first time.
    Language English
    Publishing date 2021-09-03
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.127.081802
    Database MEDical Literature Analysis and Retrieval System OnLINE

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  10. Article ; Online: Light Dark Matter Search with a High-Resolution Athermal Phonon Detector Operated above Ground.

    Alkhatib, I / Amaral, D W P / Aralis, T / Aramaki, T / Arnquist, I J / Ataee Langroudy, I / Azadbakht, E / Banik, S / Barker, D / Bathurst, C / Bauer, D A / Bezerra, L V S / Bhattacharyya, R / Binder, T / Bowles, M A / Brink, P L / Bunker, R / Cabrera, B / Calkins, R /
    Cameron, R A / Cartaro, C / Cerdeño, D G / Chang, Y-Y / Chaudhuri, M / Chen, R / Chott, N / Cooley, J / Coombes, H / Corbett, J / Cushman, P / De Brienne, F / di Vacri, M L / Diamond, M D / Fascione, E / Figueroa-Feliciano, E / Fink, C W / Fouts, K / Fritts, M / Gerbier, G / Germond, R / Ghaith, M / Golwala, S R / Harris, H R / Herbert, N / Hines, B A / Hollister, M I / Hong, Z / Hoppe, E W / Hsu, L / Huber, M E / Iyer, V / Jardin, D / Jastram, A / Kashyap, V K S / Kelsey, M H / Kubik, A / Kurinsky, N A / Lawrence, R E / Li, A / Loer, B / Lopez Asamar, E / Lukens, P / MacDonell, D / MacFarlane, D B / Mahapatra, R / Mandic, V / Mast, N / Mayer, A J / Meyer Zu Theenhausen, H / Michaud, É M / Michielin, E / Mirabolfathi, N / Mohanty, B / Morales Mendoza, J D / Nagorny, S / Nelson, J / Neog, H / Novati, V / Orrell, J L / Oser, S M / Page, W A / Pakarha, P / Partridge, R / Podviianiuk, R / Ponce, F / Poudel, S / Pyle, M / Rau, W / Reid, E / Ren, R / Reynolds, T / Roberts, A / Robinson, A E / Saab, T / Sadoulet, B / Sander, J / Sattari, A / Schnee, R W / Scorza, S / Serfass, B / Sincavage, D J / Stanford, C / Street, J / Toback, D / Underwood, R / Verma, S / Villano, A N / von Krosigk, B / Watkins, S L / Wills, L / Wilson, J S / Wilson, M J / Winchell, J / Wright, D H / Yellin, S / Young, B A / Yu, T C / Zhang, E / Zhang, H G / Zhao, X / Zheng, L / Camilleri, J / Kolomensky, Yu G / Zuber, S

    Physical review letters

    2021  Volume 127, Issue 6, Page(s) 61801

    Abstract: We present limits on spin-independent dark matter-nucleon interactions using a 10.6 g Si athermal phonon detector with a baseline energy resolution of σ_{E}=3.86±0.04(stat)_{-0.00}^{+0.19}(syst)  eV. This exclusion analysis sets the most stringent dark ... ...

    Abstract We present limits on spin-independent dark matter-nucleon interactions using a 10.6 g Si athermal phonon detector with a baseline energy resolution of σ_{E}=3.86±0.04(stat)_{-0.00}^{+0.19}(syst)  eV. This exclusion analysis sets the most stringent dark matter-nucleon scattering cross-section limits achieved by a cryogenic detector for dark matter particle masses from 93 to 140  MeV/c^{2}, with a raw exposure of 9.9 g d acquired at an above-ground facility. This work illustrates the scientific potential of detectors with athermal phonon sensors with eV-scale energy resolution for future dark matter searches.
    Language English
    Publishing date 2021-08-21
    Publishing country United States
    Document type Journal Article
    ZDB-ID 208853-8
    ISSN 1079-7114 ; 0031-9007
    ISSN (online) 1079-7114
    ISSN 0031-9007
    DOI 10.1103/PhysRevLett.127.061801
    Database MEDical Literature Analysis and Retrieval System OnLINE

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