Page 248 - Organic Electronics in Sensors and Biotechnology
P. 248

An Intr oduction to Or ganic Photodetectors     225

               statistics and consequently applies only when the electrons behave as
               independent particles. Interactions between particles can lead to
               more or less noise than predicted by the shot expression. An impor-
               tant example in inorganic semiconductor devices is the so-called
               flicker noise, which has a spectral energy density that varies as  f α
               where α≤ 1; its precise origin is poorly understood and remains a
               subject of considerable debate.  The effect of flicker noise is to increase
                                         50
               the noise level above the shot limit at frequencies less than a few hun-
               dred hertz, and whenever possible, it is advisable to work at appre-
               ciably higher frequencies. We are aware of no studies investigating
               the existence of flicker noise in organic photodiodes.
               Noise Equivalent Power
               The noise equivalent power (NEP) is a useful means of characterizing
               the sensitivity of a detector. The NEP is the minimum detectable
               power and is formally defined as the incident power required to
               achieve a signal-to-noise ratio of 1. In a system dominated by shot
               and thermal noise, the total noise current per square root of band-
               width is
                                                     4 kT
                                                V +
                                        V + 2
                               σ = 2 eI  ()  eI  ()    B            (6.42)
                              I     dark      ph
                                                      R
               To generate a photocurrent of equal size would require an incident
                           σ
                              λ
               power P()λ =    ()/ S()λ , and hence we obtain for the noise equiva-
                             I
               lent power per square root of hertz

                         NEP =   1   2 eI  ()  eI ()   4 kT         (6.43)
                                                   V +
                                                         B
                                          V + 2
                                 λ
                                S()    dark      ph      R
          6.5 Measuring a Current
               The simplest way to measure a small current is to pass it through a
               large “sense” resistor and measure the associated voltage drop across
               the resistor (Fig. 6.17a). The current can then be determined by simple
               application of Ohm’s law. There are several problems with this
               approach, however. To obtain a reasonably sized voltage from a small
               current, a very large sense resistor is required; e.g., a gigaohm resis-
               tance is required to generate a millivolt from a picoampere. The high
               resistance combines with the high capacitance of the photodiode to
               create a large RC time constant, which results in a sluggish response.
               For instance, a photodiode capacitance of 100 pF coupled to a gigaohm
               sense resistance yields a time constant of 100 ms, making it difficult to
               measure signals above 10 Hz. A faster response can be obtained by
               reducing the sense resistor, but the increased speed comes at the
               expense of reduced gain. The use of a large sense resistor also limits
   243   244   245   246   247   248   249   250   251   252   253