Abstract
A proper understanding of the mechanics and susceptibility of nanoparticles under the influence of coherent light fields will be a core ingredient throughout this thesis. It will be required for the description of new matter-wave interferometry schemes and of optical methods to manipulate the motion or measure the optical properties of molecules and clusters. This chapter is dedicated to the light–matter interaction in the presence of coherent laser fields, of high-finesse cavity modes and, not least, of a (thermally occupied) radiation field.
More light!—Johann Wolfgang von Goethe’s last words
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsNotes
- 1.
The full mathematical description of Gaussian light fields, as generated by focused laser beams or found in curved-mirror cavities, is a little bit more involved than presented here. I give a detailed formula for symmetric Gaussian mode functions with \(w_{x}=w_{y}=w\) in Appendix A.2. Strictly speaking, the above representations (2.2) and (2.3) are zeroth order approximations of the Gaussian mode fields in the waist parameter \(1/kw\), and additional polarization components must be taken into account for higher orders.
- 2.
Note that the light-atom interaction can also be modeled by a complex linear polarizability provided the light is far detuned from any internal electronic transition and the transition is not strongly driven. In the latter case the atom’s response saturates at sufficiently high field intensities, as described by the Jaynes-Cummings model [4, 5].
- 3.
The vector identities [7],
$$\begin{aligned} \nabla \left( {\varvec{a}}\cdot {\varvec{b}}\right)&={\varvec{a}}\times \left( \nabla \times {\varvec{b}}\right) +{\varvec{b}}\times \left( \nabla \times {\varvec{a}}\right) +\left( {\varvec{b}}\cdot \nabla \right) {\varvec{a}}+\left( {\varvec{a}}\cdot \nabla \right) {\varvec{b}},\\ \left( \nabla \circ {\varvec{b}}\right) {\varvec{a}}&={\varvec{a}}\times \left( \nabla \times {\varvec{b}}\right) +\left( {\varvec{a}}\cdot \nabla \right) {\varvec{b}}, \end{aligned}$$might occasionally be useful here and in the following. The dyadic term \(B=\nabla \circ {\varvec{b}}\) is defined as the matrix \(B_{jk}=\partial b_{k}/\partial x_{j}\).
- 4.
Stochastic differential equations can serve to describe the effective time evolution of open systems in contact with an environment inducing rapid (uncontrollable) state transitions that cannot be examined with the coarse-grained time resolution of observation [9]. The transitions thus show up as random events, or ‘jumps’. Using a Poissonian model we assume single infrequent jumps that can be clearly distinguished.
- 5.
Using a fixed polarization \(\varvec{\epsilon }\left( {\varvec{r}}\right) = \varvec{\epsilon }\) is a good approximation in many practical cases such as Gaussian TEM modes, where position-dependent corrections are negligibly small. A detailed description of modes with a position-dependent polarization vector is more involved and requires a specific physical model of the particle’s response during the absorption process. This is because the orientation of the induced dipole moment then contains information about the position of the particle in the field mode, which is traced out when only the center-of-mass state is monitored.
- 6.
Here I have used the identity \(\left[ {\mathbf {\mathsf{{p}}}} ^{2},f\left( {\mathbf {\mathsf{{r}}}} \right) \right] =-\hbar ^{2}\varDelta f\left( {\mathbf {\mathsf{{r}}}} \right) -2i\hbar \nabla f\left( {\mathbf {\mathsf{{r}}}} \right) \cdot {\mathbf {\mathsf{{p}}}} =\hbar ^{2}\varDelta f\left( {\mathbf {\mathsf{{r}}}} \right) -2i\hbar {\mathbf {\mathsf{{p}}}} \cdot \nabla f\left( {\mathbf {\mathsf{{r}}}} \right) \), as well as the fact that the mode function by construction solves the Helmholtz equation \(\varDelta u=-k^{2}u\).
- 7.
In this approximation, the intensity profile merely limits the interaction time between the field mode and the PPP traversing the cavity volume.
- 8.
A cavity linewidth of \(1\,\)MHz corresponds to a so-called cavity finesse parameter \(F=\pi c / 2\kappa L \approx 5 \times 10^{-5} \). The latter is related to the reflectivity \(R\) of both mirrors via the relation \(F=\pi \sqrt{R}/\left( 1-R \right) \) in the absence of additional losses in the resonator [28]. The suggested cavity setup requires \(1-R\approx 7\times 10^{-6}\).
- 9.
Since the wavelength of the laser is required to be sufficiently well defined for the present purposes, ultrashort pulses with a broad frequency spectrum are excluded here.
- 10.
To be more concrete, the travelled distance \(v_{z}\tau \) during the interaction period \(\tau \) between the particle and the field must be small compared to the laser wavelength, \(\left| v_{z}\tau \right| \ll \lambda \). Given the reduced one-dimensional quantum state of motion \(\rho _{z}\), the condition should cover its entire velocity distribution \(\langle mv_{z}|\rho |mv_{z}\rangle \).
- 11.
Note that the direction of the grating is commonly referred to as the \(x\)-axis in the interferometry literature, whereas the standing wave is directed along \(z\) in the present notation, which is conventionally used in the description of light scattering at spherical particles. I will resort to the \(x\)-notation in Chap. 3.
- 12.
A realistic description of the molecular beam state involves a broad distribution of velocities \(v\), and the resulting \(\phi _{0}\)-dependent interferogram must be averaged accordingly.
- 13.
Also referred to as OTIMA: optical time-domain ionizing matter-wave interferometer.
- 14.
The ionized particles are in practice removed from the ensemble with the help of a constant electric field applied to the interferometer setup.
- 15.
This is intuitively clear since the absorption of a photon reveals the information that the particle is not located at a node. On the other hand, the photon cannot distinguish two positions \(z\) and \(z'\), which differ by an integer multiple of the wavelength.
- 16.
I made use of the integral representation of the Bessel function \(\int _{0}^{2\pi }\text {d}\varphi \,\exp \left( i\xi \sin \varphi \right) =2\pi J_{0}\left( \xi \right) \), as well as of the integral identity [43]
$$ \int \limits _{0}^{\pi /2}\text {d}\theta \, J_{0}\left( \beta \sin \theta \right) \sin \theta \cos ^{2r+1}\theta =2^{r}\beta ^{-1-r}\varGamma \left( r+1\right) J_{r+1}\left( \beta \right) , $$with \(r=\pm 1/2\) and the Gamma function \(\varGamma \left( 3/2\right) =\sqrt{\pi }/2=2\varGamma \left( 1/2\right) \). The identity leads naturally to spherical Bessel function expressions \(j_{n}\left( \beta \right) =\sqrt{\pi /2\beta }J_{n+1/2}\left( \beta \right) \), where \(j_{0}\left( \beta \right) =\text {sinc}\beta \).
- 17.
The coupling strength between fields of different polarizations through a PPP may vary, most notably if the particle is described by a tensorial polarizability. I omit this additional modulation of the coupling for simplicity.
- 18.
The form is easily obtained by adding the quantized physical fields (2.54) of the modes \( {\mathsf {a}} _{0}\) and \( {\mathsf {b}} \) to an overall electric and magnetic field. When the corresponding field energy density is integrated over the volume in (2.4) the cross terms between both modes yield the above linear coupling Hamiltonian. Terms of the form \( {\mathsf {a}} _{0} {\mathsf {b}} \) and \( {\mathsf {a}} _{0}^{{\dagger }} {\mathsf {b}} \) are omitted in the rotating wave approximation [45], since they oscillate rapidly at twice an optical frequency, \(\omega _{P}+\omega _{0}\), and thus do not affect the actual mode coupling.
- 19.
A rotating frame is defined through the unitary state transformation \( {\mathsf {U}} \left( t\right) =\exp \left( i\omega _{P}\sum _{n} {\mathsf {a}} _{n}^{{\dagger }} {\mathsf {a}} _{n}\right) \), with \(\omega _{P}\) the corresponding rotation frequency. Given the quantum state \(\rho \left( t\right) \) of a system of field modes \(\left\{ {\mathsf {a}} _{n}\right\} \) in the Schrödinger picture, the state in the rotating picture reads as \(\rho '= {\mathsf {U}} \left( t\right) \rho \left( t\right) {\mathsf {U}} ^{{\dagger }}\left( t\right) \). Analogously, a displaced frame is defined via the unitary displacement operator, \(\rho '= {\mathsf {D}} ^{{\dagger }}\left( \beta \right) \rho {\mathsf {D}} \left( \beta \right) \). Field observables are displaced as \( {\mathsf {D}} ^{{\dagger }}\left( \beta \right) {\mathsf {b}} {\mathsf {D}} \left( \beta \right) = {\mathsf {b}} + \beta \).
- 20.
Optical frequencies in the environmental mode spectrum are practically unoccupied even at finite temperatures. I thus use the zero-temperature vacuum state here, since the cavity only couples to modes of similar frequencies.
- 21.
Practical implementations of the present cavity dissipation scheme are restricted to non-absorbing particle species. The typically large pump field intensities might otherwise lead to the destruction of the particle.
- 22.
Applying the interaction Hamiltonian to the vacuum state leads to nondiagonal elements of the form \(|1_{n}\rangle \langle \text {vac}|\), with \(|1_{n}\rangle = {\mathsf {a}} _{n}^{{\dagger }}|\text {vac}\rangle \) a single-excitation multimode Fock state. One can easily show that these nondiagonals evolve like \(\exp \left( \mathcal {L} _{C}t\right) |1_{n}\rangle \langle \text {vac}|=\exp \left( -\kappa _{n}t-i\varDelta _{n}t\right) |1_{n}\rangle \langle \text {vac}|\).
- 23.
Running-wave modes do not exhibit a wavelength-scale oscillatory intensity pattern. Their influence on the particle through the optical potential is considerably weaker.
- 24.
Condition (2.83) would be alleviated by a factor \(kw\ll 1\) in the case of a Gaussian profile with waist \(w\).
- 25.
Here I make use of the procedure of integration by parts and of the fact that a well-behaved and normalizable Wigner function should vanish at the infinities.
- 26.
The diffusion matrix generally should be positive semidefinite in order to ensure that the occupied phase-space area increases and that the time evolution produces physical states at all times.
- 27.
This would be a bad approximation if the underlying quantum state would be a delocalized matter-wave state that could be diffracted by the standing-wave structure of the pump mode (see Sect. 2.1.4).
- 28.
Rayleigh scattering can be viewed as absorption and immediate reemission of a pump photon into free space. The absorption is responsible for the radiation pressure force, whereas the reemission does not contribute on average because there is no preferred direction of scattering, \(\left\langle n_{z} \right\rangle =\int \text {d}^{2}n\, R\left( {\varvec{n}}\right) n_{z}=0\).
- 29.
- 30.
This corresponds to the experimental situation when a dilute beam of molecules or nanoparticles crosses the cavity, such that there is on average only one particle inside the cavity at a given time.
- 31.
Laguerre-Gaussian modes can only be used if the mirror system exhibits a cylindrical symmetry. This symmetry may be violated in applications with birefringent mirrors. In this case one must use the rectangular Hermite-Gaussian modes instead [64], which yield similar results as presented here.
- 32.
Second order terms of the form \(z^{2}/d^{2}\), \(1/k^{2}d^{2}\) and \(z/kd^{2}\) are dropped. The inverse tangent is linearized as \(\arctan \left( 2z/d\right) \approx 2z/d\).
- 33.
The average friction rate depends on the size of the averaging area. A larger area covers more space outside the cavity where the friction effect is zero. Nevertheless, the average value is a meaningful quantity to assess the net slowing of particles that are trapped in or passing the chosen region in a given amount of time.
- 34.
Nonspherical particles scatter light in different patterns, that is, the multipole composition of the scattered field deviates from the spherical case. The basic consequences of leaving the subwavelength size regime are similar to the spherical case, with the additional complication of coupling to the rotation of the object.
- 35.
I use that the spherical Bessel functions can be approximated by \(j_{\ell }\left( x\right) \approx x^{\ell }/ \left[ 1\cdot 3\cdot \ldots \cdot \left( 2\ell +1\right) \right] \) and \(y_{\ell }\left( x\right) \approx -\left[ 1\cdot 3\cdot \ldots \cdot \left( 2\ell -1\right) \right] / x^{\ell +1}\) to lowest order in \(x\ll 1\), while the spherical Hankel function becomes \(h_{\ell }\left( x\right) \approx iy_{\ell }\left( x\right) \).
- 36.
All the calculations can be done in the vacuum surrounding the sphere, thus avoiding the discussion [72] which form of the Poynting vector to choose inside the medium.
- 37.
This argument holds as long as the sphere is not too far away from the focus of the Gaussian mode. The reason is that the representation of the Gaussian TEM\(_{00}\) mode given in Appendix A.2 ceases to be valid for far-off center coordinates \(\left| {\varvec{r}}_{0}\right| \gg w\). This limit should hardly be of relevance in any practical implementation.
- 38.
Decoherence by absorption becomes relevant, too, but only if the optical depletion effect requires more than one photon to be triggered.
- 39.
The following integral identities for spherical Bessel functions must be used [43]:
$$\begin{aligned} \int \limits _{0}^{X}\text {d}x\, x^2 j_{\ell }\left( x\right) j_{\ell }\left( nx\right)&=\frac{X^{2}}{1-n^{2}}\left[ j_{\ell +1}\left( X\right) j_{\ell }\left( nX\right) -nj_{\ell }\left( X\right) j_{\ell +1}\left( nX\right) \right] \\ \int \limits _{0}^{X}\!\! \text {d}x\left\{ \ell \left( \ell +1\right) j_{\ell }\left( x\right) j_{\ell }\left( nx\right) +\left[ xj_{\ell }\left( x\right) \right] '\left[ xj_{\ell }\left( nx\right) \right] '\right\}&=\frac{n X^{2}}{1-n^{2}}\left[ n j_{\ell +1}\left( X\right) j_{\ell }\left( nX\right) -j_{\ell }\left( X\right) j_{\ell +1}\left( nX\right) \right] \\&+\left( \ell +1\right) Xj_{\ell }\left( X\right) j_{\ell }\left( nX\right) \end{aligned}$$
References
S. Nimmrichter, K. Hammerer, P. Asenbaum, H. Ritsch, M. Arndt, Master equation for the motion of a polarizable particle in a multimode cavity. New J. Phys. 12, 083003 (2010)
H.C. van de Hulst, Light Scattering by Small Particles (Dover, New York, 1981)
C.F. Bohren, D.R. Huffman, Absorption and Scattering of Light by Small Particles (Wiley, New York, 1998)
A.P. Kazantsev, G.I. Surdutovich, V.P. Yakovlev, Mechanical Action of Light on Atoms (World Scientific, Singapore, 1990)
S. Haroche, J.-M. Raimond, Exploring the Quantum: Atoms, Cavities, and Photons (Oxford Graduate Texts) (Oxford University Press, Oxford, 2006)
S.M. Barnett, R. Loudon, On the electromagnetic force on a dielectric medium. J. Phys. B Atomic Mol. Opt. Phys. 39, S671 (2006)
B. Thidé, Electromagnetic Field Theory (Online Version) (Dover, New York, 2011)
J.D. Jackson, Classical Electrodynamics, 3rd edn. (Wiley, New York, 1999)
H.-P. Breuer, F. Petruccione, The Theory of Open Quantum Systems (Oxford University Press, Oxford, 2002)
H.M. Wiseman, G.J. Milburn, Quantum Measurement and Control (Cambridge University Press, Cambridge, 2010)
M. Gallis, G. Fleming, Environmental and spontaneous localization. Phys. Rev. A 42, 38 (1990)
S. Nimmrichter, K. Hornberger, H. Ulbricht, M. Arndt, Absolute absorption spectroscopy based on molecule interferometry. Phys. Rev. A 78, 063607 (2008)
H. Du, R.-C.A. Fuh, J. Li, L.A. Corkan, J.S. Lindsey, PhotochemCAD: a computer-aided design and research tool in photochemistry. Photochem. Photobiol. 68, 141 (1998)
J.M. Dixon, M. Taniguchi, J.S. Lindsey, PhotochemCAD 2: a refined program with accompanying spectral databases for photochemical calculations. Photochem. Photobiol. 81, 212 (2007)
K. Hornberger, J.E. Sipe, M. Arndt, Theory of decoherence in a matter mave Talbot-Lau interferometer. Phys. Rev. A 70, 53608 (2004)
K. Hansen, E. Campbell, Thermal radiation from small particles. Phys. Rev. E 58, 5477 (1998)
K. Hornberger, S. Gerlich, P. Haslinger, S. Nimmrichter, M. Arndt, Colloquium: quantum interference of clusters and molecules. Rev. Mod. Phys. 84, 157 (2012)
P. Horak, G. Hechenblaikner, K. Gheri, H. Stecher, H. Ritsch, Cavity-induced atom cooling in the strong coupling regime. Phys. Rev. Lett. 79, 4974 (1997)
M. Gangl, H. Ritsch, Collective dynamical cooling of neutral particles in a high-Q optical cavity. Phys. Rev. A 61, 011402 (1999)
V. Vuletić, S. Chu, Laser cooling of atoms. Ions Mol. Coherent Scattering Phys. Rev. Lett. 84, 3787 (2000)
H. Chan, A. Black, V. Vuletić, Observation of collective-emission-induced cooling of atoms in an optical cavity. Phys. Rev. Lett. 90, 063003 (2003)
P. Maunz, T. Puppe, I. Schuster, N. Syassen, P.W.H. Pinkse, G. Rempe, Cavity cooling of a single atom. Nature 428, 50 (2004)
S. Nußmann, K. Murr, M. Hijlkema, B. Weber, A. Kuhn, G. Rempe, Vacuum-stimulated cooling of single atoms in three dimensions. Nat. Phys. 1, 122 (2005)
M. Wolke, J. Klinner, H. Keßler, A. Hemmerich, Cavity cooling below the recoil limit. Science 337, 75 (2012)
B. Lev, A. Vukics, E. Hudson, B. Sawyer, P. Domokos, H. Ritsch, J. Ye, Prospects for the cavity-assisted laser cooling of molecules. Phys. Rev. A 77, 023402 (2008)
C. Gardiner, P. Zoller, Quantum Noise: A Handbook of Markovian and Non-Markovian Quantum Stochastic Methods with Applications to Quantum Optics (Springer Series in Synergetics) (Springer, Berlin, 2010)
P. Asenbaum, Private Communication (University of Vienna, Austria, 2012)
B.E.A. Saleh, M.C. Teich, Fundamentals of Photonics 2nd edn. (Wiley, New York, 2007)
E.D. Palik, G. Ghosh, Handbook of Optical Constants of Solids (Academic Press, New York, 1985)
M.L. Gorodetsky, A.D. Pryamikov, V.S. Ilchenko, Rayleigh scattering in high-Q microspheres. J. Opt. Soc. Am. B 17, 1051 (2000)
U. Kreibig, M. Vollmer, Optical Properties of Metal Clusters (Springer Series in Materials Science) (Springer, Berlin, 1995)
M.S. Dresselhaus, G. Dresselhaus, P.C. Eklund, Science of Fullerenes and Carbon Nanotubes: Their Properties and Applications (Academic Press, New York, 1996)
G. Lach, B. Jeziorski, K. Szalewicz, Radiative corrections to the polarizability of helium. Phys. Rev. Lett. 92, 233001 (2004)
A. Miffre, M. Jacquey, M. Büchner, G. Trénec, J. Vigué, Measurement of the electric polarizability of lithium by atom interferometry. Phys. Rev. A 73, 011603 (2006)
R.J. Glauber, High-energy collision theory. in Lectures in Theoretical Physics: Lectures Delivered at the Summer Institute for Theoretical Physics (University of Colorado, Boulder, Wiley, 1959), p. 315
S. Nimmrichter, Matter Wave Talbot-Lau Interferometry Beyond the Eikonal Approximation (Diploma thesis, Technische Universität München, 2007)
S. Nimmrichter, K. Hornberger, Theory of near-field matter-wave interference beyond the eikonal approximation. Phys. Rev. A 78, 023612 (2008)
P.R. Berman, Atom Interferometry (Academic Press, San Diego, 1996)
A.D. Cronin, D.E. Pritchard, Optics and interferometry with atoms and molecules. Rev. Mod. Phys. 81, 1051 (2009)
K. Hornberger, S. Gerlich, H. Ulbricht, L. Hackermüller, S. Nimmrichter, I.V. Goldt, O. Boltalina, M. Arndt, Theory and experimental verification of Kapitza-Dirac-Talbot-Lau interferometry. New J. Phys. 11, 43032 (2009)
S. Nimmrichter, P. Haslinger, K. Hornberger, M. Arndt, Concept of an ionizing time-domain matter-wave interferometer. New J. Phys. 13, 075002 (2011)
A. Turlapov, A. Tonyushkin, T. Sleator, Talbot-Lau effect for atomic de Broglie waves manipulated with light. Phys. Rev. A 71, 043612 (2005)
I.S. Gradshteyn, I.M. Ryzhik, A. Jeffrey, D. Zwillinger, Table of Integrals, Series, and Products (Academic Press, New York, 2007)
S.M. Dutra, Cavity Quantum Electrodynamics: The Strange Theory of Light in a Box (Wiley, New York, 2005)
R.J. Glauber, Quantum Theory of Optical Coherence (Wiley, New York, 2006)
D. Walls, G.J. Milburn, Quantum Optics 2nd edn. (Springer, Berlin, 2007)
G.J. Milburn, Lorentz invariant intrinsic decoherence. New J. Phys. 8, 96 (2006)
G. Hechenblaikner, M. Gangl, P. Horak, H. Ritsch, Cooling an atom in a weakly driven high-Q cavity. Phys. Rev. A 58, 3030 (1998)
M. Poot, H.S. van der Zant, Mechanical systems in the quantum regime. Phys. Rep. 511, 273 (2012)
F. Marquardt, A. Clerk, S. Girvin, Quantum theory of optomechanical cooling. J. Mod. Opt. 55, 3329 (2008)
S. Gröblacher, K. Hammerer, M.R. Vanner, M. Aspelmeyer, Observation of strong coupling between a micromechanical resonator and an optical cavity field. Nature 460, 724 (2009)
M. Aspelmeyer, S. Gröblacher, K. Hammerer, N. Kiesel, Quantum optomechanics-throwing a glance. J. Opt. Soc. Am. B 27, A189 (2010)
P. Domokos, H. Ritsch, Mechanical effects of light in optical resonators. J. Opt. Soc. Am. B 20, 1098 (2003)
S. Stenholm, The semiclassical theory of laser cooling. Rev. Mod. Phys. 58, 699 (1986)
J. Cirac, R. Blatt, P. Zoller, W. Phillips, Laser cooling of trapped ions in a standing wave. Phys. Rev. A 46, 2668 (1992)
K. Jaehne, K. Hammerer, M. Wallquist, Ground-state cooling of a nanomechanical resonator via a Cooper-pair box qubit. New J. Phys. 10, 095019 (2008)
P. Domokos, P. Horak, H. Ritsch, Semiclassical theory of cavity-assisted atom cooling. J. Phys. B At. Mol. Opt. Phys. 34, 187 (2001)
H. Risken, T. Frank, The Fokker-Planck Equation: Methods of Solution and Applications (Springer Series in Synergetics) (Springer, Berlin, 2008)
W.P. Schleich, Quantum Optics in Phase Space (Wiley, Berlin, 2001)
S. Barnett, S. Stenholm, Hazards of reservoir memory. Phys. Rev. A 64, 033808 (2001)
J. Salo, S.M. Barnett, S. Stenholm, Non-Markovian thermalisation of a two-level atom. Opt. Commun. 259, 772 (2006)
J. Piilo, K. Härkönen, S. Maniscalco, K.-A. Suominen, Open system dynamics with non-Markovian quantum jumps. Phys. Rev. A 79, 062112 (2009)
G.D. Boyd, J.P. Gordon, Confocal multimode resonator for millimeter through optical wavelength masers. Bell Syst. Tech. J 40, 489 (1961)
N. Hodgson, H. Weber, Optical Resonators: Fundamentals, Advanced Concepts, Applications (Springer Series in Optical Sciences) (Springer, New York, 2005)
P. Asenbaum, Towards Cavity Cooling of a Molecular Beam (Diploma thesis, Universität Wien, 2009)
P. Domokos, H. Ritsch, Collective cooling and self-organization of atoms in a cavity. Phys. Rev. Lett. 89, 253003 (2002)
A. Black, H. Chan, V. Vuletić, Observation of collective friction forces due to spatial self-organization of atoms: from rayleigh to bragg scattering. Phys. Rev. Lett. 91, 203001 (2003)
A. Pflanzer, O. Romero-Isart, J.I. Cirac, Master-equation approach to optomechanics with arbitrary dielectrics. Phys. Rev. A 86, 013802 (2012)
O. Romero-isart, M.L. Juan, R. Quidant, J.I. Cirac, Toward quantum superposition of living organisms. New J. Phys. 12, 33015 (2010)
D.E. Chang, C.A. Regal, S.B. Papp, D.J. Wilson, J. Ye, O. Painter, H.J. Kimble, P. Zoller, Cavity opto-mechanics using an optically levitated nanosphere. Proc. Nat. Acad. Sci. 107, 1005 (2010)
B. Dalton, E. Guerra, P. Knight, Field quantization in dielectric media and the generalized multipolar Hamiltonian. Phys. Rev. A 54, 2292 (1996)
S.M. Barnett, R. Loudon, The enigma of optical momentum in a medium. Philos. Trans. A 368, 927 (2010)
L.D. Landau, L.P. Pitaevskii, E. Lifshitz, Electrodynamics of Continuous Media (Course of Theoretical Physics), 2nd edn, vol. 8 (Butterworth-Heinemann, 1984)
L. Tsang, J.A. Kong, K.-H. Ding, Scattering of Electromagnetic Waves: Theories and Applications (Wiley, New York, 2000)
J.A. Stratton, Electromagnetic Theory (Wiley, New York, 2007)
S. Nimmrichter, K. Hornberger, P. Haslinger, M. Arndt, Testing spontaneous localization theories with matter-wave interferometry. Phys. Rev. A 83, 43621 (2011)
O. Romero-Isart, A.C. Pflanzer, F. Blaser, R. Kaltenbaek, N. Kiesel, M. Aspelmeyer, J.I. Cirac, Large Quantum Superpositions and Interference of Massive Nanometer-Sized Objects. Phys. Rev. Lett. 107, 20405 (2011)
D.M. Pozar, Microwave Engineering 4th edn. (Wiley, New York, 2011)
Author information
Authors and Affiliations
Corresponding author
Rights and permissions
Copyright information
© 2014 Springer International Publishing Switzerland
About this chapter
Cite this chapter
Nimmrichter, S. (2014). Interaction of Polarizable Particles with Light. In: Macroscopic Matter Wave Interferometry. Springer Theses. Springer, Cham. https://doi.org/10.1007/978-3-319-07097-1_2
Download citation
DOI: https://doi.org/10.1007/978-3-319-07097-1_2
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-319-07096-4
Online ISBN: 978-3-319-07097-1
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)