Isabella Fritsche’s research while affiliated with University of Innsbruck and other places

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Publications (12)


Dependence of the polaron energy on the impurity concentration
For the FF case, the main steps of measurements and data analysis are illustrated. a, Two exemplary spectroscopy signals (normalized to the initial atom number) taken at X = − 1.41 for different values of the interacting impurity concentration (blue squares C̃=0.17\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tilde{{{{\mathcal{C}}}}}=0.17$$\end{document}, orange diamonds C̃=0.09\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tilde{{{{\mathcal{C}}}}}=0.09$$\end{document}). The solid lines are fits with a Gaussian function on a linear background (the latter being negligibly small in the present data). The error bars represent the standard errors from typically 5-6 measurement repetitions. b, Polaron energy as a function of impurity concentration for X = − 1.41. The blue square and the orange diamond correspond to the exemplary spectra presented in panel a. The black line represents a linear fit to the data with the dashed line showing the extrapolation to zero density. c, Polaron energy as a function of impurity concentration for different values of the interaction parameter X. From center to top (blue to red) increasing repulsion, from center to bottom (green to red) increasing attraction. Statistical uncertainties for b and c are evaluated taking into account fit uncertainties from analyzing the spectra and errors on the Fermi energy.
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Typical RF spectra in the strongly interacting regime and comparison between two fitting functions
Spectroscopy signals for the FB case with X = 0.36 and C̃=0.07\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tilde{{{{\mathcal{C}}}}}=0.07$$\end{document} (a) and X = − 0.34 and C̃=0.07\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tilde{{{{\mathcal{C}}}}}=0.07$$\end{document} (b), and for the FF case with X = 0.47 and C̃=0.03\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tilde{{{{\mathcal{C}}}}}=0.03$$\end{document} (c) and X = − 0.47 and C̃=0.08\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tilde{{{{\mathcal{C}}}}}=0.08$$\end{document} (d) The solid red lines are fits with a Gaussian function on a linear background, the dashed blue lines are fits with a double Gaussian. The error bars represent the standard errors from typically 5-6 measurement repetitions.
Source data
Polaron energy including mediated interactions
The energy of attractive and repulsive polarons is presented as a function of the dimensionless interaction parameter X according to equation (3) using the static limit for the polaron–polaron-mediated interaction defined in equation (2). The results are shown for the limit of a single impurity (that is, C=0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{\mathcal{C}}}}=0$$\end{document}; black dashed lines) and for impurity concentration C=0.5\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${{{\mathcal{C}}}}=0.5$$\end{document} in FB (solid green lines) and FF (solid red lines) K–Li mixtures.
Dependence of polaron energy on the impurity concentration
For the FB case, the main steps of measurements and data analysis are illustrated. a, Two example spectroscopy signals (normalized to the initial atom number) taken at X = 0.98 for different values of the interacting impurity concentration (blue squares, C̃=0.16\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tilde{{{{\mathcal{C}}}}}=0.16$$\end{document}; orange diamonds, C̃=0.04\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\tilde{{{{\mathcal{C}}}}}=0.04$$\end{document}). The solid lines are fits with a Gaussian function on a linear background (the latter being negligibly small in the present data). The error bars represent the standard errors from typically 5–6 measurement repetitions. b, Polaron energy as a function of impurity concentration for X = 0.98. The blue square and the orange diamond correspond to the example spectra presented in a. The black line represents a linear fit to the data, with the dashed line showing the extrapolation to zero density. c, Polaron energy as a function of impurity concentration for different values of interaction parameter X. From centre to top (blue to red), increasing repulsion; from centre to bottom (green to red), increasing attraction. Statistical uncertainties in b and c are evaluated taking into account the fit uncertainties from analysing the spectra and errors on the Fermi energy.
Source data
Polaron energy in the single-impurity limit
The experimental results for ϵ↓0/ϵF\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\epsilon }_{\downarrow }^{0}/{\epsilon }_{{{{\rm{F}}}}}$$\end{document} for the FB (green circles) and FF (red squares) mixtures are compared with the theoretically expected values for a single polaron (green and red solid lines for FB and FF, respectively). In addition, we show the energy of the dressed molecules (green and red dash–dot lines for FB and FF, respectively). Note that the theory lines are almost identical for the FB and FF cases; therefore, they overlap to a large extent. The error bars for ϵ↓0/ϵF\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$${\epsilon }_{\downarrow }^{0}/{\epsilon }_{{{{\rm{F}}}}}$$\end{document} correspond to the uncertainties of the linear fit and the errors on the Fermi energy. The error bars for X, smaller than the symbol size, represent the standard errors for each set of measurements.
Source data

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Mediated interactions between Fermi polarons and the role of impurity quantum statistics
  • Article
  • Full-text available

October 2023

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84 Reads

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44 Citations

Nature Physics

Cosetta Baroni

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Isabella Fritsche

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[...]

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Georg M. Bruun

The notion of quasi-particles is essential for understanding the behaviour of complex many-body systems. A prototypical example of a quasi-particle is a polaron, formed by an impurity strongly interacting with a surrounding medium. Fermi polarons, created in a Fermi sea, provide a paradigmatic realization of this concept. Importantly, such quasi-particles interact with each other via the modulation of the medium. However, although quantum simulation experiments with ultracold atoms have substantially improved our understanding of individual polarons, the detection of their interactions has so far remained elusive. Here we report the observation of mediated interactions between Fermi polarons consisting of K impurities embedded in a Fermi sea of Li atoms. Our results confirm two predictions of Landau’s Fermi-liquid theory: the shift in polaron energy due to mediated interactions, which is linear in the concentration of impurities; and its sign inversion with impurity quantum statistics. For weak-to-moderate interactions between the impurities and the medium, our results agree with the static predictions of Fermi-liquid theory. For stronger impurity–medium interactions, we show that the observed behaviour at negative energies can be explained by a more refined many-body treatment including retardation and dressed molecule formation.

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Fig. 2 Dependence of the polaron energy on the impurity concentration. For the FB case, the main steps of measurements and data analysis are illustrated. a, Two exemplary spectroscopy signals (normalized to the initial atom number) taken at X = 0.98 for different values of the interacting impurity concentration (blue squares˜Csquares˜ squares˜C = 0.16, orange diamonds˜Cdiamonds˜ diamonds˜C = 0.04). The solid lines are fits with a Gaussian function on a linear background (the latter being negligibly small in the present data). The error bars represent the standard errors from typical 5-6 measurement repetitions. b, Polaron energy as a function of impurity concentration for X = 0.98, the blue squares and the orange diamonds correspond to the exemplary spectra presented in panel a. The black line represents a linear fit to the data with the dashed line showing the extrapolation to zero density. c, Polaron energy as a function of impurity concentration for different values of the interaction parameter X. From center to top (blue to red) increasing repulsion, from center to bottom (green to red) increasing attraction. Statistical uncertainties are evaluated taking into account fit uncertainties from analyzing the spectra and errors on Fermi energy.
Fig. 3 Polaron energy in the single-impurity limit. The experimental results for 0 ↓ // F for the FB (green circles) and the FF (red squares) mixture are compared with the theoretically expected values for a single polaron (green and red solid lines for FB and FF, respectively). In addition we show the energy of the dressed molecules (green and red dashdotted lines for FB and FF, respectively). Note that the theory lines are almost identical for the FB and the FF case, so that they overlap to a large extent. Error bars for 0 ↓ // F correspond to the uncertainties of the linear fit and the errors on the Fermi energy. Error bars for X, smaller than the symbol size, represent the standard errors for each set of measurements.
Fig. 4 Mediated interaction coefficient in the regime of moderate impuritymedium interactions. The experimental results for ¯ f n ↑ // F for FB (green circles) and FF (red squares) are compared with equation (4) with ¯ f given by the static limit of the Fermi liquid theory of equation (3) (green and red solid lines refer to FB and FF cases, respectively) for interaction values |X| 1. Error bars on ¯ f n ↑ // F correspond to the uncertainties of the linear fit and the errors on the Fermi energy. Error bars on X, smaller than the symbol size, represent the standard errors for each set of measurements.
Fig. 5 Mediated interaction coefficient across the resonance. The experimental results for ¯ f n ↑ // F for the FB (green circles) and the FF (red squares) mixture are compared with the static Fermi liquid theory of equation (3) (dashed green and red lines for FB and FF, respectively) and with the corresponding microscopic many-body result (see details in the Supplementary Information), assuming a density of molecules equal to 2.5 times that of the impurities (solid green and red lines for FB and FF, respectively). Error bars on ¯ f n ↑ // F correspond to the uncertainties of the linear fit and the errors on the Fermi energy. Error bars on X, smaller than the symbol size, represent the standard errors for each set of measurements.
Fig. S 1. Effects of the impurity mean energy. a: mean energy of the K impurities as a function of the concentration, obtained by numerically solving equation (S.1) with typical experimental parameters. Circles are obtained using the same value for the trap frequencies as in the experiment, diamonds using four fold increased ones. The color scale represent the effective temperature of the impurities for different concentrations. The orange and the blue lines represent the limit of a classical and an ideal Fermi gas at finite temperature, respectively. E ♦ F K and T ♦ F K are, respectively, the Fermi energy and the Fermi temperature relative to impurities with C = 0.5. The red dashed line represents the high temperature expansion. b: variation of the polaron energy with the concentration, considering only the mediated polaron-polaron interaction (solid blue lines) and the mediated polaron-polaron interaction plus the contribution of the mean energy of the impurities (solid red lines). c: single impurity limit for T = 0 (solid blue lines) and considering the effect of the impurity mean energy for T = 250 nK (solid red lines). The green squares are the experimental data for the FF mixture, as in Fig. 3 of the main text. The quantities in all the panels are normalized by the Fermi energy of the Li Fermi sea
Mediated interactions between Fermi polarons and the role of impurity quantum statistics

May 2023

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58 Reads

The notion of quasi-particles is essential for understanding the behaviour of complex many-body systems. A prototypical example of a quasi-particle, a polaron, is an impurity strongly interacting with a surrounding medium. Fermi polarons, created in a Fermi sea, provide a paradigmatic realization of this concept. As an inherent and important property such quasi-particles interact with each other via modulation of the medium. While quantum simulation experiments with ultracold atoms have significantly improved our understanding of individual polarons, the detection of their interactions has remained elusive in these systems. Here, we report the unambiguous observation of mediated interactions between Fermi polarons consisting of K impurities embedded in a Fermi sea of Li atoms. Our results confirm two landmark predictions of Landau's Fermi-liquid theory: the shift of the polaron energy due to mediated interactions, linear in the concentration of impurities, and its sign inversion with impurity quantum statistics. For weak to moderate interactions between the impurities and the medium, we find excellent agreement with the static (zero-momentum and energy) predictions of Fermi-liquid theory. For stronger impurity-medium interactions, we show that the observed behaviour at negative energies can be explained by a more refined many-body treatment including retardation and molecule formation


Stability and breakdown of Fermi polarons in a strongly interacting Fermi-Bose mixture

May 2021

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30 Reads

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65 Citations

Physical Review A

We investigate the properties of a strongly interacting imbalanced mixture of bosonic K41 impurities immersed in a Fermi sea of ultracold Li6 atoms. This enables us to explore the Fermi polaron scenario for large impurity concentrations including the case where they form a Bose-Einstein condensate. The system is characterized by means of radio-frequency injection spectroscopy and interspecies interactions are widely tunable by means of a well-characterized Feshbach resonance. We find that the energy of the Fermi polarons formed in the thermal fraction of the impurity cloud remains rather insensitive to the impurity concentration, even as we approach equal densities for both species. The apparent insensitivity to high concentration is consistent with a theoretical prediction, based on Landau's quasiparticle theory, of weak effective interaction between the polarons. The condensed fraction of the bosonic K41 gas is much denser than its thermal component, which leads to a break-down of the Fermi polaron description. Instead, we observe a new branch in the radio-frequency spectrum with a small energy shift, which is consistent with the presence of Bose polarons formed by Li6 fermions inside the K41 condensate. A closer investigation of the behavior of the condensate by means of Rabi oscillation measurements supports this observation, indicating that we have realized Fermi and Bose polarons, two fundamentally different quasiparticles, in one cloud.


Stability and breakdown of Fermi polarons in a strongly interacting Fermi-Bose mixture

March 2021

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27 Reads

We investigate the properties of a strongly interacting imbalanced mixture of bosonic 41^{41}K impurities immersed in a Fermi sea of ultracold 6^6Li atoms. This enables us to explore the Fermi polaron for large impurity concentrations including the case where they form a Bose-Einstein condensate. The system is characterized by means of radio-frequency injection spectroscopy for tunable interactions using an interspecies Feshbach resonance. We find that the energy of the Fermi polarons formed in the thermal fraction of the impurity cloud remains rather insensitive to the impurity concentration, even as we approach equal densities for both species. The apparent insensitivity to high concentration is consistent with the theoretical prediction, based on Landau's quasiparticle theory, of a weak effective interaction between the polarons. The condensed fraction of the bosonic 41^{41}K gas is much denser than its thermal component, which leads to a break-down of the Fermi polaron description. Instead, we observe a new branch in the radio-frequency spectrum with a small energy shift, which is consistent with the presence of Bose polarons formed by 6^{6}Li fermions inside the 41^{41}K condensate. A closer investigation of the behavior of the condensate by means of Rabi oscillation measurements support this observation, indicating that we have realized Fermi and Bose polarons, two fundamentally different quasiparticles, in one cloud.


Breathing mode of a Bose-Einstein condensate repulsively interacting with a fermionic reservoir

April 2019

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83 Reads

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42 Citations

Physical Review A

We investigate the fundamental breathing mode of a small-sized elongated Bose-Einstein condensate coupled to a large Fermi sea, which consists of fully spin-polarized atoms in the collisionless regime. Our observations show a dramatic shift of the breathing frequency when the mixture undergoes phase separation at strong interspecies repulsion. We find that the maximum frequency shift in the full phase-separation limit depends essentially on the atom number ratio of the components. We interpret the experimental observations by modeling the complex dynamics of the collisionless fermions within two complementary approaches. One model assumes an adiabatic response of the Fermi sea, while the other one considers single fermion trajectories for a fully phase-separated mixture. Our models capture the observed features over the full range of interest.


Breathing Mode of a BEC Repulsively Interacting with a Fermionic Reservoir

December 2018

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74 Reads

We investigate the fundamental breathing mode of a small-sized elongated Bose-Einstein condensate coupled to a large Fermi sea of atoms. Our observations show a dramatic shift of the breathing frequency when the mixture undergoes phase separation at strong interspecies repulsion. We find that the maximum frequency shift in the full phase-separation limit depends essentially on the atom number ratio of the components. We interpret the experimental observations within a model that assumes an adiabatic response of the Fermi sea, or within another model that considers single fermion trajectories for a fully phase-separated mixture. These two complementary models capture the observed features over the full range of interest.


Probing the Interface of a Phase-Separated State in a Repulsive Bose-Fermi Mixture

February 2018

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44 Reads

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105 Citations

Physical Review Letters

We probe the interface between a phase-separated Bose-Fermi mixture consisting of a small BEC of 41^{41}K residing in a large Fermi sea of 6^6Li. We quantify the residual spatial overlap between the two components by measuring three-body recombination losses for variable strength of the interspecies repulsion. A comparison with a numerical mean-field model highlights the importance of the kinetic energy term for the condensed bosons in maintaining the thin interface far into the phase-separated regime. Our results demonstrate a corresponding smoothing of the phase transition in a system of finite size.


Probing the Interface of a Phase-Separated State in a Repulsive Bose-Fermi Mixture

February 2018

We probe the interface between a phase-separated Bose-Fermi mixture consisting of a small BEC of 41^{41}K residing in a large Fermi sea of 6^6Li. We quantify the residual spatial overlap between the two components by measuring three-body recombination losses for variable strength of the interspecies repulsion. A comparison with a numerical mean-field model highlights the importance of the kinetic energy term for the condensed bosons in maintaining the thin interface far into the phase-separated regime. Our results demonstrate a corresponding smoothing of the phase transition in a system of finite size.


Thermometry of a deeply degenerate Fermi gas with a Bose-Einstein condensate

February 2017

We measure the temperature of a deeply degenerate Fermi gas, by using a weakly interacting sample of heavier bosonic atoms as a probe. This thermometry method relies on the thermalization between the two species and on the determination of the condensate fraction of the bosons. In our experimental implementation, a small sample of 41K atoms serves as the thermometer for a 6Li Fermi sea. We investigate the evaporative cooling of a 6Li spin mixture in a single-beam optical dipole trap and observe how the condensate fraction of the thermometry atoms depends on the final trap depth. From the condensate fraction, the temperature can be readily extracted. We show that the lowest temperature of 6.3(5)% of the Fermi temperature is obtained, when the decreasing trap depth closely approaches the Fermi energy. To understand the systematic effects that may in uence the results, we carefully investigate the role of the number of bosons and the thermalization dynamics between the two species. Our thermometry approach provides a conceptually simple, accurate, and general way to measure the temperature of deeply degenerate Fermi gases. Since the method is independent of the specific interaction conditions within the Fermi gas, it applies to both weakly and strongly interacting Fermi gases.


Thermometry of a deeply degenerate Fermi gas with a Bose-Einstein condensate

February 2017

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23 Reads

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46 Citations

Physical Review A

We measure the temperature of a deeply degenerate Fermi gas, by using a weakly interacting sample of heavier bosonic atoms as a probe. This thermometry method relies on the thermalization between the two species and on the determination of the condensate fraction of the bosons. In our experimental implementation, a small sample of 41K atoms serves as the thermometer for a 6Li Fermi sea. We investigate the evaporative cooling of a 6Li spin mixture in a single-beam optical dipole trap and observe how the condensate fraction of the thermometry atoms depends on the final trap depth. From the condensate fraction, the temperature can be readily extracted. We show that the lowest temperature of 6.3(5)% of the Fermi temperature is obtained, when the decreasing trap depth closely approaches the Fermi energy. To understand the systematic effects that may in uence the results, we carefully investigate the role of the number of bosons and the thermalization dynamics between the two species. Our thermometry approach provides a conceptually simple, accurate, and general way to measure the temperature of deeply degenerate Fermi gases. Since the method is independent of the specific interaction conditions within the Fermi gas, it applies to both weakly and strongly interacting Fermi gases.


Citations (6)


... The realization of polarons in cold atoms [12][13][14][15][16][17] opens a new and ideal platform to study correlation effects due to the high degree of tunability and clean environment [18][19][20][21]. This achievement has led to the study of the strong impurity-bath coupling regime, i.e., strongly correlated polarons, previously unattainable or uncontrollable in solid-state systems [22][23][24], along with the investigation of the interplay between different particle statistics such as the Bose or Fermi polaron, an impurity immersed in a bosonic or fermionic bath respectively , and multiple impurities where statistics and manybody effects play an important role [46][47][48][49][50][51][52][53][54]. ...

Reference:

Bose–Fermi N -polaron state emergence from correlation-mediated blocking of phase separation
Mediated interactions between Fermi polarons and the role of impurity quantum statistics

Nature Physics

... The realization of polarons in cold atoms [12][13][14][15][16][17] opens a new and ideal platform to study correlation effects due to the high degree of tunability and clean environment [18][19][20][21]. This achievement has led to the study of the strong impurity-bath coupling regime, i.e., strongly correlated polarons, previously unattainable or uncontrollable in solid-state systems [22][23][24], along with the investigation of the interplay between different particle statistics such as the Bose or Fermi polaron, an impurity immersed in a bosonic or fermionic bath respectively , and multiple impurities where statistics and manybody effects play an important role [46][47][48][49][50][51][52][53][54]. ...

Stability and breakdown of Fermi polarons in a strongly interacting Fermi-Bose mixture
  • Citing Article
  • May 2021

Physical Review A

... Another topic of considerable interest is the formation of bound states in Fermi gases with unequal masses, such as mixtures of 6 Li and 40 K near the Feshbach resonance [14,29]. These mass-imbalanced systems introduce additional degrees of freedom and complex interaction landscapes, which are crucial for understanding few-body and many-body physics. ...

Breathing mode of a Bose-Einstein condensate repulsively interacting with a fermionic reservoir
  • Citing Article
  • April 2019

Physical Review A

... Before delving into the analysis of mechanical stability, we present the results for the thermodynamic parameters B , F , 0 obtained by solving the set of Eqs. (15)(16)(17). The results for these quantities have already been presented in [52]. ...

Probing the Interface of a Phase-Separated State in a Repulsive Bose-Fermi Mixture
  • Citing Article
  • February 2018

Physical Review Letters

... Hence, temperature control is an essential tool for the calibration of quantum simulators. In this regard, proposals for measuring the temperature of a fermionic quantum gas with a neutral and charged impurity have already been put forward [20][21][22] as well as by using Bose polarons [23], where sub-nK thermometry has been predicted. Most importantly, those approaches are non-destructive, in contrast to, e.g., time-of-flight measurements, and can be even more precise. ...

Thermometry of a deeply degenerate Fermi gas with a Bose-Einstein condensate
  • Citing Article
  • February 2017

Physical Review A

... Furthermore, different spectroscopy techniques allow for direct measurement of the spectral function, offering insights into elementary excitations in complex quantum systems. For instance, Ramsey interferometry has been used to implement a two-point measurement scheme to determine the work probability distribution of a driven non-equilibrium state [55], granting direct access to both its excitation spectrum and thermodynamic properties. ...

Ultrafast many-body interferometry of impurities coupled to a Fermi sea
  • Citing Article
  • October 2016

Science