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High-resolution Interferometric Diagnostics for Ultrashort Pulses

High-resolution Interferometric Diagnostics for Ultrashort Pulses

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2. BACKGROUNDments [31, 32] led to the deliberate introduction of dispersive elements into the cavity leading togreater pulse compression [33, 34], eventually down to 27 fs [35, 36].While ultrashort dye lasers were enjoying their zenith in the 1980s, investigations into solidstatematerials revealed the potential <strong>for</strong> even greater bandwidths, potentially supporting pulsesas short as 1 fs [37]. From a number of different technologies and pulse generation mechanisms,the Ti:Sapph oscillator emerged as a leading contender. By 1993, pulse durations down to about10 fs [38–41] were being produced. However, in this regime of pulse duration, the enormous bandwidthspossess a chirp which cannot be accurately characterised by a simple linear dependenceof arrival time on wavelength. Instead, several orders of a Taylor polynomial expansion must beconsidered <strong>for</strong> good characterisation and compensation [42]. The combination of the spectrumwith the simple nonlinear autocorrelations, as used previously, did not determine these higher orderterms. This motivated the development of complete characterisation methods, capable of retrievingall in<strong>for</strong>mation about the pulse up to a few well understood, and hopefully insignificant,ambiguities. These measurements guided improvements to the designs. More sensitive autocorrelationmethods [43] guided the introduction of specially-designed chirped mirrors to compensate<strong>for</strong> intra-cavity dispersion [44] with corresponding pulse durations of 8 fs. However, the first completecharacterisation methods such as frequency-resolved optical gating (FROG) [45] and spectralphase interferometry <strong>for</strong> direct electric-field reconstruction (SPIDER) [46], returned the chirp toall orders [47, 48, 48–50], assisting with design improvements which pushed pulse durations downto around 5 fs [51, 52].2.1.2.2 Metrology and the manipulation of ultrashort pulsesBesides the drive towards shorter pulses, another development in ultrafast science is the ability toamplify, compress and shape ultrashort pulses. Metrology also plays a crucial role in these areas.Pulse amplification systems are often limited by the peak intensity, which causes nonlineardistortions of the pulse or induces damage to the materials. Chirped pulse amplification [53, 54]circumvents this by stretching the pulse to reduce its peak intensity, then per<strong>for</strong>ming the amplification,then compressing the pulse by undoing the chirp. The stretching and compression steps10

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