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On the Time-Dependent Harmonic Oscillator

Salusti

Published Jan 1, 2007• 0 citations
OpenAlex

Abstract

In recent years, some interes t has been raised by the problem of the quan tum harmonic-osci l la tor wi th a coupling cons tant K(t), which is a funct ion of t ime (1.2). The impor tance of this p roblem has been stressed by the analysis of the mot ion of a charged part ic le in the presence of a magnet ic field H~(t), which has a fixed direct ion bu t changes i ts in tens i ty wi th t ime (1). The reason of this note is tha t , among these recent studies, the most na tura l approach is surprisingly absent. We will describe i t here, and we will analyse some easily solvable potent ials . W e say t h a t i t is a ve ry na tura l approach, because i t consists in a ve ry na ive general ization of Dirae 's method. I n order to in t roduce it, we remark tha t the Dirae creat ion opera tor (in the t imeindependen t case) could be considered as the opera tor t ha t gives a solution once applied to another solution (for ins tance the vacuum). So we in t roduce an opera tor A ( x , ~ /~x , t) with the p rope r ty tha t , once appl ied to a solut ion of the SehrSdinger equat ion , i t gives another solution. The expl ici t form of this opera tor A is obta ined by means of a simple differential equat ion wi th one and only one solution. W e then find an explici t solution of the t ime-dependen t SchrSdinger equat ion , as a simple general izat ion of the vacuum wave function. App ly ing i tc ra t ive ly the A opera to r we obta in an explici t form for a set of solutions. Noth ing can be said, however , abou t the general case.

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In recent years, some interes t has been raised by the problem of the quan tum harmonic-osci l la tor wi th a coupling cons tant K(t), which is a funct ion of t ime (1.2). The impor tance of this p roblem has been stressed by the analysis of the mot ion of a charged part ic le in the presence of a magnet ic field H~(t), which has a fixed direct ion bu t changes i ts in tens i ty wi th t ime (1). The reason of this note is tha t , among these recent studies, the most na tura l approach is surprisingly absent. We will describe i t here, and we will analyse some easily solvable potent ials . W e say t h a t i t is a ve ry na tura l approach, because i t consists in a ve ry na ive general ization of Dirae 's method. I n order to in t roduce it, we remark tha t the Dirae creat ion opera tor (in the t imeindependen t case) could be considered as the opera tor t ha t gives a solution once applied to another solution (for ins tance the vacuum). So we in t roduce an opera tor A ( x , ~ /~x , t) with the p rope r ty tha t , once appl ied to a solut ion of the SehrSdinger equat ion , i t gives another solution. The expl ici t form of this opera tor A is obta ined by means of a simple differential equat ion wi th one and only one solution. W e then find an explici t solution of the t ime-dependen t SchrSdinger equat ion , as a simple general izat ion of the vacuum wave function. App ly ing i tc ra t ive ly the A opera to r we obta in an explici t form for a set of solutions. Noth ing can be said, however , abou t the general case.
mu1 t i p l i e d bya f u n c t i o n o f x', z and T . Here we have de f ined -r = (tr't r ) / n f o r l a t e r convenience. He then c a r r i e r s o u t c a l c u l a t i o n s as T + O ( o r n +a). H i s method has r e c e n t l y been a p p l i e d f o r e v a l u a t i n g t h e propag a t o r o f t ime-dependent fo rced harmonic occ i 1 l a t o r 5 . J n the p resen t work the sane method has been genera l i zed f u r t h e r t o c a l c u l a t e t h e propaga to r o f time-dependent harmonic o s c i l l a t o r w i t h cons tan t damping. I n Sec t ion 2, we a r e a b l e t o t rans fo rm o u r p a t h i n t e g r a l i n t o a f u n c t i o n o f x', x and T. t h e Gaussian i n t e g r a l (1.2) mul t i p l i e d by
I n order to find out new exper iments useful to t es t q u a n t u m predic t ions for the polar izat ion correlat ion of the decay p roduc t s of a composi te sys tem, we have recent ly (1,~) proposed a new m e a s u r e m e n t us ing the th ree annih i la t ion pho tons of t r iplet P , in S-state . The proposed expe r imen t was concerned wi th the m u t u a l polar izat ion of a pa i r of pho tons ana lysed b y ideal p la tes in two typ ica l a symmet r i ca l cases shown in fig. 1, where the pos i t ron ium a t o m is supposed to decay into two pho tons wi th the same m o m e n t u m , while the th i rd one is de te rmined b y the e n e r g y m o m e n t u m conservat ion. I n bo th si tuations the joint p robab i l i t y of detect ing pho tons To . 1 and To . 2 polarized along definite directions was der ived according to the hypo theses which are now briefly recalled: the first hypothes is was following the convent ional lines of q u a n t u m theo ry b y assuming t h a t the initial po lar iza t ion corre lat ion of the emi t t ed pho tons is indefinitely ma in t aned , so t h a t i t r emains
The origin of the wave-part ic le dual ism of quantum theory can be t raced back to Einstein 's analysis of the fluctuations of b lack-body radia t ion in 1909 (1-3). Based on this invest igat ion EINSTEIlq proposed the in te rpre ta t ion tha t the electromagnetic field in thermal equil ibrium has as well par t ic le as wave propert ies . In his analysis concerning the ideal quantum gas of 1925 he came to the conclusion tha t this dualist ic in te rpre ta t ion applies to the par t ic les of the gas as well (a). Recent ly we have shown tha t the fluctuations of b lack-body radia t ion can be explained from the assumption of s ta t i s t ica l ly dependent indist inguishable part icles (5). Moreover, i t tu rned out tha t the so-called wave contr ibut ions to the var iance are ent i re ly due to the s ta t is t ical dependence of these part icles. F rom this viewpoint Einstein 's dualist ic in te rpre ta t ion is incomprehensible. I t is the aim of this note to explain a weak point in Einstein 's analysis in detai l and to show tha t wave proper t ies emerge in the classical l imi t only. Planck 's formula gives the mean value of the energy densi ty g* (with respect to dco) of b lack-body rad ia t ion :