Bragg solitons are optical solitons that can exist in fiber Bragg gratings due to the interplay between nonlinearity and periodic modulation of the refractive index. Fiber Bragg gratings are fabricated by exposing germanium-doped optical fibers to ultraviolet laser irradiation, which produces a periodic refractive index pattern. Bragg solitons have been experimentally observed to propagate in fiber gratings at velocities between 60-80% of the speed of light in the unwritten fiber. Their properties are mathematically modeled using coupled mode equations that take into account the effects of nonlinearity, dispersion, and the periodic grating structure.
Plenary lecture of the XIV SBPMat Meeting, given by Prof. Nader Engheta (University of Pennsylvania) on September 28, 2015, in Rio de Janeiro (Brazil).
Plenary lecture given by Prof. Hajo Freund (Fritz-Haber-Institut der Max-Planck-Gesellschaft, Germany) on September 11, 2017 in Gramado (Brazil) during the XVI B-MRS Meeting.
Plenary lecture of the XIV SBPMat Meeting, given by Prof. Nader Engheta (University of Pennsylvania) on September 28, 2015, in Rio de Janeiro (Brazil).
Plenary lecture given by Prof. Hajo Freund (Fritz-Haber-Institut der Max-Planck-Gesellschaft, Germany) on September 11, 2017 in Gramado (Brazil) during the XVI B-MRS Meeting.
Over five years research and development experience in silicon wafer based solar photovoltaics. Specialized in characterization of silicon wafer and solar cells. Developed and establish methods for the measurement of diffusion length in higher lifetime wafers, front and back surface recombination in silicon solar cell.
Plenary lecture of the XIII SBPMat (Brazilian MRS) meeting, given on September 30th 2014 by Karl Leo, professor of optoelectronics at Dresden University of Technology (Germany) and director of the Solar and Photovoltaic Engineering Research Center at KAUST (Saudi Arabia).
Plenary lecture of the XIII SBPMat (Brazilian MRS) meeting, given on September 30th, 2014, in João Pessoa (Brazil) by Sir Colin Humphreys, Professor at University of Cambridge (U.K.).
Study of highly broadening Photonic band gaps extension in one-dimensional Me...IOSR Journals
In this paper, we show theoretically that the reflectance spectra of one dimensional multilayer metal-organic periodic structure (1D MOPS) can be enhanced due to the addition of the organic constituents. We have used simple transfer matrix method to calculate the absorption, transmittance and reflectance of the 1D MOPS systems. The organic component like N,N’-bis-(1-naphthyl)-N,N’diphenyl-1; 1biphenyl-4; 4diamine (NPB) absorbs the light in ultra-violet, visible and infrared electromagnetic region and the structure with Ag-metal also having the tendency to absorb the light by the plasmaonic action and their refractive can be calculated from Drude equation. The reflectance spectra of multilayer 1D MOPS containing a variable number periodic of Ag/N,N’-bis-(1-naphthyl)-N,N’diphenyl-1; 1biphenyl-4; 4diamine (NPB) structure are calculated taking optical constant of NPB and Ag. The optical band gap and reflectance spectra of 1D MOPS of the considered structure is obtained in the visible and near infrared regions either with the variation of the metal layer thickness or thickness of the organic layer. From the results under investigation through TMM, tunability in the optical band gap was observed either change in thickness of the other layer 1/ or 2 or the angle of the incident. Due to optical absorption of the light in the different region of electromagnetic spectrum due to either N,N’-bis-(1-naphthyl)-N,N’diphenyl-1; 1biphenyl-4; 4diamine (NPB) or silver metal, the optical band gap of 1DMOPS shows the shift of band edges of λL and λR from ultra-violet to visible and the infrared with change the optical constant.
This presentation aims at introducing the concepts of soliton propagation. The solitons are a result of nonlinear optical interaction of light pulses within optical fibers.
Nanometer Bandwidth Soliton Generation and Experimental Transmission within ...University of Malaya (UM)
An optical add-drop filter system is used to generate ultra-short nanometer (nm)
bandwidth soliton pulses to be transmitted along the nano communication nonlinear fiber
optics. In order to reduce the loss during the transmission, ultra-short soliton pulses are
recommended. The theoretical part of this study uses the Z-transform method to present the
characteristic transmission of the optical add-drop filter system. The nonlinear refractive
index of the fiber optic transmission link is 2.6 ×10-20
m
2
/W. The Wavelength Division
Multiplexing (WDM) can be performed to enhance the capacity of the system. This occurs
when the bigger size of the ring resonator is used. Here, soliton pulses with bandwidths of 2.1
and 0.42 nm are generated and transmitted over the fiber optic length, where signals with a
bandwidth of 55 and 200 ps are successfully detected at the end of the transmission link.
A Study on Uniform and Apodized Fiber Bragg GratingsIJSRD
The design, simulation and analysis of an optical Fiber Bragg Grating for maximum reflectivity, minimum side lobe power wastage has been done using MATLAB software. The reflection spectra and side lobes strength were analyzed with different grating lengths, refractive index profiles and pitch values. The simulations are based on coupled mode equations and transfer matrix method that describes the interaction of guided modes.
Multiplex and De-multiplex of Generated Multi Optical Soliton By MRRs Using F...University of Malaya (UM)
A microring resonators (MRRs) system conecting to an ad/drop system is presented
to create ultra-short multi soliton pulses which can be used for optical communication. The
ad/drop system can be used to generate a high capacity of ultra-short soliton pulses. A bright
soliton pulse propagates inside the system, where chaotic noise can be generated. The
obtained multi solution have ful width at half maximum (FWHM) of 16 ps, 20 pm, 140 ps,
40 pm and fre spectrum range, FSR of 50 ps, 0.57 nm, 3.6 ns and 1.45 nm respectively.
Here, the single temporal soliton pulse having FWHM of 75 fs, 84 fs could be generated. The
ultra-short multi soliton pulses with wavelengths range from λ=150 to λ=1560 can be
multiplexed, transmited along an optical fiber optics with a length of 50 km and finaly be
de-multiplexed and detected by the users at he end of the optical transmision link.
Over five years research and development experience in silicon wafer based solar photovoltaics. Specialized in characterization of silicon wafer and solar cells. Developed and establish methods for the measurement of diffusion length in higher lifetime wafers, front and back surface recombination in silicon solar cell.
Plenary lecture of the XIII SBPMat (Brazilian MRS) meeting, given on September 30th 2014 by Karl Leo, professor of optoelectronics at Dresden University of Technology (Germany) and director of the Solar and Photovoltaic Engineering Research Center at KAUST (Saudi Arabia).
Plenary lecture of the XIII SBPMat (Brazilian MRS) meeting, given on September 30th, 2014, in João Pessoa (Brazil) by Sir Colin Humphreys, Professor at University of Cambridge (U.K.).
Study of highly broadening Photonic band gaps extension in one-dimensional Me...IOSR Journals
In this paper, we show theoretically that the reflectance spectra of one dimensional multilayer metal-organic periodic structure (1D MOPS) can be enhanced due to the addition of the organic constituents. We have used simple transfer matrix method to calculate the absorption, transmittance and reflectance of the 1D MOPS systems. The organic component like N,N’-bis-(1-naphthyl)-N,N’diphenyl-1; 1biphenyl-4; 4diamine (NPB) absorbs the light in ultra-violet, visible and infrared electromagnetic region and the structure with Ag-metal also having the tendency to absorb the light by the plasmaonic action and their refractive can be calculated from Drude equation. The reflectance spectra of multilayer 1D MOPS containing a variable number periodic of Ag/N,N’-bis-(1-naphthyl)-N,N’diphenyl-1; 1biphenyl-4; 4diamine (NPB) structure are calculated taking optical constant of NPB and Ag. The optical band gap and reflectance spectra of 1D MOPS of the considered structure is obtained in the visible and near infrared regions either with the variation of the metal layer thickness or thickness of the organic layer. From the results under investigation through TMM, tunability in the optical band gap was observed either change in thickness of the other layer 1/ or 2 or the angle of the incident. Due to optical absorption of the light in the different region of electromagnetic spectrum due to either N,N’-bis-(1-naphthyl)-N,N’diphenyl-1; 1biphenyl-4; 4diamine (NPB) or silver metal, the optical band gap of 1DMOPS shows the shift of band edges of λL and λR from ultra-violet to visible and the infrared with change the optical constant.
This presentation aims at introducing the concepts of soliton propagation. The solitons are a result of nonlinear optical interaction of light pulses within optical fibers.
Nanometer Bandwidth Soliton Generation and Experimental Transmission within ...University of Malaya (UM)
An optical add-drop filter system is used to generate ultra-short nanometer (nm)
bandwidth soliton pulses to be transmitted along the nano communication nonlinear fiber
optics. In order to reduce the loss during the transmission, ultra-short soliton pulses are
recommended. The theoretical part of this study uses the Z-transform method to present the
characteristic transmission of the optical add-drop filter system. The nonlinear refractive
index of the fiber optic transmission link is 2.6 ×10-20
m
2
/W. The Wavelength Division
Multiplexing (WDM) can be performed to enhance the capacity of the system. This occurs
when the bigger size of the ring resonator is used. Here, soliton pulses with bandwidths of 2.1
and 0.42 nm are generated and transmitted over the fiber optic length, where signals with a
bandwidth of 55 and 200 ps are successfully detected at the end of the transmission link.
A Study on Uniform and Apodized Fiber Bragg GratingsIJSRD
The design, simulation and analysis of an optical Fiber Bragg Grating for maximum reflectivity, minimum side lobe power wastage has been done using MATLAB software. The reflection spectra and side lobes strength were analyzed with different grating lengths, refractive index profiles and pitch values. The simulations are based on coupled mode equations and transfer matrix method that describes the interaction of guided modes.
Multiplex and De-multiplex of Generated Multi Optical Soliton By MRRs Using F...University of Malaya (UM)
A microring resonators (MRRs) system conecting to an ad/drop system is presented
to create ultra-short multi soliton pulses which can be used for optical communication. The
ad/drop system can be used to generate a high capacity of ultra-short soliton pulses. A bright
soliton pulse propagates inside the system, where chaotic noise can be generated. The
obtained multi solution have ful width at half maximum (FWHM) of 16 ps, 20 pm, 140 ps,
40 pm and fre spectrum range, FSR of 50 ps, 0.57 nm, 3.6 ns and 1.45 nm respectively.
Here, the single temporal soliton pulse having FWHM of 75 fs, 84 fs could be generated. The
ultra-short multi soliton pulses with wavelengths range from λ=150 to λ=1560 can be
multiplexed, transmited along an optical fiber optics with a length of 50 km and finaly be
de-multiplexed and detected by the users at he end of the optical transmision link.
A Flexible and Stretchable Tactile Sensor utilizing Static Electricity
The tactile sensor is required for various robots.
In humanoid robots, flexibility of the sensor is an important
feature for preventing physical damage and for interacting
with the human. Moreover, stretchability of the sensor has
advantages that the sensor is nonbreakable and that the sensor can be easily mounted on curved surfaces or deformable parts such as joints. This paper proposes a novel tactile sensor made of flexible and stretchable silicone rubber.
A structure of the sensor is similar to the capacitive tactile sensors. However, the proposed sensor utilizes a different principle from existing sensors. The sensor utilizes static electricity and electrostatic induction phenomenon, and can detect some touch conditions.
This paper reports the principle and characteristics of the
proposed sensor. Experiments show that the sensor output
depends on touch area, touch velocity, and material of touch
objects. However, the sensor does not depend on touch weight.
Moreover, the experiment shows that even if the proposed
sensor is stretched, it performs as the tactile sensor.
Thunderbolt technology is a transformational I/O innovation that provides a leap
in performance over current I/O technologies with 10 Gbps of full-duplex bandwidth
per channel. It significantly simplifies the end-user experience by concurrently supporting
data (PCI Express) and display (DisplayPort) connections over a single cable.
Thunderbolt products may be connected using electrical or optical cables. Thunderbolt
technology enables flexible and innovative system designs by allowing multiple, highperformance,
PCI Express and DisplayPort devices to attach to a computer through a
single physical connector.
We present an ab-initio real-time based computational approach to nonlinear optical properties in Condensed Matter systems. The equation of mot ions, and in particular the coupling of the electrons with the external electric field, are derived from the Berry phase formulation of the dynamical polarization. The zero-field Hamiltonian includes crystal local field effects, the renormalization of the independent particle energy levels by correlation and excitonic effects within the screened Hartree- Fock self-energy operator. The approach is validated by calculating the second-harmonic generation of SiC and AlAs bulk semiconductors : an excellent agreement is obtained with existing ab-initio calculations from response theory in frequency domain . We finally show applications to the second-harmonic generation of CdTe the third-harmonic generation of Si.
Reference :
Real-time approach to the optical properties of solids and nanostructures : Time-dependent Bethe-alpeter equation Phys. Rev. B 84, 245110 (2011)
Nonlinear optics from ab-initio by means of the dynamical Berry-phase
C. Attaccalite and M. Gruning Phys. Rev. B 88 (23), 235113 (2013)
37 Latest results from GRAAL collaboration - Chinese Physics C (HEP & NP), De...Cristian Randieri PhD
Latest results from GRAAL collaboration - Chinese Physics C (HEP & NP), December 2009, Vol. 33, N. 12, pp. 1249-1253, ISSN: 1674-1137, doi: 10.1088/1674-1137/33/12/032
di V. Vegna, V. Bellini, J. P. Bouquet, L. Casano, A. D'Angelo, J. P. Didelez, R. Di Salvo, A. Fantini, D. Franco, G. Gervino, F. Ghio, G. Giardina, B. Girolami, A. Giusa, M. Guidal, E. Hourany, A. S. Ignatov, R. Kunnel, A. Lapik, A. Lleres, P. Levi Sandri, F. Mammoliti, G. Mandaglio, M. Manganaro, M. Moricciani, A.N. Mushkarenkov, V. G. Nedorezov, C. Randieri, D. Rebreyend, N. V. Rudnev, G. Russo, C. Schaerf, M. L. Sperduto, M. C. Sutera, A. Turinge (2009)
Abstract
The GRAAL experimental set-up consists of a polarized and tagged photon beam that covers an energy range from a minimum of 600 MeV up to a maximum of 1500 MeV, of a liquid Hydrogen or Deuterium target and of the 4π Lagrange detector optimized for photon detection. It allows the study of pseudo-scalar and vector meson photoproduction on the nucleon in the energy range corresponding to the second and the third resonance regions. In the following, the σ beam asymmetries in η and π0 photoproduction on quasi-free nucleon are shown. Also single and double polarization observables in K+Λ photoproduction on free proton are shown; they are important to confirm the role of new or poorly known resonances in the 1900 MeV mass region.
The broad lined_type_ic_sn_2012_ap_and_the_nature_of_relatvistic_supernovae_l...Sérgio Sacani
Artigo mostra como os astrônomos deduziram que a supernova SN 2012ap, é o elo perdido que faltava para a construção completa da árvore genealógica das supernovas.
EXTINCTION AND THE DIMMING OF KIC 8462852Sérgio Sacani
To test alternative hypotheses for the behavior of KIC 8462852, we obtained measurements of the star
over a wide wavelength range from the UV to the mid-infrared from October 2015 through December
2016, using Swift, Spitzer and at AstroLAB IRIS. The star faded in a manner similar to the longterm
fading seen in Kepler data about 1400 days previously. The dimming rate for the entire period
reported is 22.1 ± 9.7 milli-mag yr−1
in the Swift wavebands, with amounts of 21.0 ± 4.5 mmag in
the groundbased B measurements, 14.0 ± 4.5 mmag in V , and 13.0 ± 4.5 in R, and a rate of 5.0 ± 1.2
mmag yr−1 averaged over the two warm Spitzer bands. Although the dimming is small, it is seen at
& 3 σ by three different observatories operating from the UV to the IR. The presence of long-term
secular dimming means that previous SED models of the star based on photometric measurements
taken years apart may not be accurate. We find that stellar models with Tef f = 7000 - 7100 K and
AV ∼ 0.73 best fit the Swift data from UV to optical. These models also show no excess in the
near-simultaneous Spitzer photometry at 3.6 and 4.5 µm, although a longer wavelength excess from
a substantial debris disk is still possible (e.g., as around Fomalhaut). The wavelength dependence of
the fading favors a relatively neutral color (i.e., RV & 5, but not flat across all the bands) compared
with the extinction law for the general ISM (RV = 3.1), suggesting that the dimming arises from
circumstellar material
36 Measurement of Σ beam asymmetry in π0 photoproduction off the neutron in t...Cristian Randieri PhD
Measurement of Σ beam asymmetry in π0 photoproduction off the neutron in the second and third resonances region - The European Physical Journal A, Hadrons and Nuclei, November 2009, Vol. 42, N. 2, pp. 151-157, ISSN: 1434-6001, doi: 10.1140/epja/i2009-10870-x
di R. Di Salvo, A. Fantini, G. Mandaglio, F. Mammoliti, O. Bartalini, V. Bellini, J. P. Bocquet, L. Casano, A. D’angelo, J. P. Didelez, D. Franco, G. Gervino, F. Ghio, G. Giardina, B. Girolami, A. Giusa, M. Guidal, E. Hourany, R. Kunne, A. Lapik, P. Levi Sandri, A. Lleres, M. Manganaro, D. Moricciani, A. N. Mushkarenkov, V. Nedorezov, C. Randieri, D. Rebreyend, N. Rudnev, G. Russo, C. Schaerf, M. L. Sperduto, M. C. Sutera, A. Turinge, V. Vegna, A. Fix, S. S. Kamalov, L. Tiator (2009)
Abstract
The Σ beam asymmetry in the photoproduction of neutral pions from quasi-free nucleons in a deuteron target was measured for the first time between 0.60 and 1.50GeV, with the GRAAL polarized and tagged photon beam. The asymmetry values from the quasi-free proton were found equal to the ones extracted from a pure proton target. The asymmetries from quasi-free proton and quasi-free neutron were found equal up to 0.82GeV and substantially different at higher energies. The results are compared with recent partial-wave analyses.
Spitzer Observations of the Predicted Eddington Flare from Blazar OJ 287Sérgio Sacani
Binary black hole (BH) central engine description for the unique blazar OJ 287 predicted that the
next secondary BH impact-induced bremsstrahlung flare should peak on 2019 July 31. This prediction
was based on detailed general relativistic modeling of the secondary BH trajectory around the primary
BH and its accretion disk. The expected flare was termed the Eddington flare to commemorate the
centennial celebrations of now-famous solar eclipse observations to test general relativity by Sir Arthur
Corresponding author: Lankeswar Dey
lankeswar.dey@tifr.res.in
arXiv:2004.13392v1 [astro-ph.HE] 28 Apr 2020
2 Laine et al.
Eddington. We analyze the multi-epoch Spitzer observations of the expected flare between 2019 July
31 and 2019 September 6, as well as baseline observations during 2019 February–March. Observed
Spitzer flux density variations during the predicted outburst time display a strong similarity with
the observed optical pericenter flare from OJ 287 during 2007 September. The predicted flare appears
comparable to the 2007 flare after subtracting the expected higher base-level Spitzer flux densities at
3.55 and 4.49 µm compared to the optical R-band. Comparing the 2019 and 2007 outburst lightcurves
and the previously calculated predictions, we find that the Eddington flare arrived within 4 hours of
the predicted time. Our Spitzer observations are well consistent with the presence of a nano-Hertz
gravitational wave emitting spinning massive binary BH that inspirals along a general relativistic
eccentric orbit in OJ 287. These multi-epoch Spitzer observations provide a parametric constraint
on the celebrated BH no-hair theorem.
Confirmation of the_planetary_microlensing_signal_and_star_and_planet_mass_de...Sérgio Sacani
O Telescópio Espacial Hubble e o Observatório W. M. Keck, no Havaí, fizeram confirmações independentes de um exoplaneta orbitando sua estrela central de uma distância bem grande. O planeta foi descoberto através de uma técnica chamada de microlente gravitacional.
Essa descoberta traz uma nova peça para o processo de caçada de exoplanetas: para descobrir planetas longe de suas estrelas, como Júpiter e Saturno estão do Sol. Os resultados obtidos pelo Hubble e pelo Keck apareceram em dois artigos da edição de 30 de Julho de 2015 do The Astrophysical Journal.
A grande maioria dos exoplanetas catalogados são aqueles localizados bem perto de suas estrelas, isso acontece porque as técnicas atuais de se caçar exoplanetas favorecem a descoberta de planetas com curtos períodos orbitais. Mas esse não é o caso da técnica de microlente gravitacional, que pode encontrar planetas mais frios e mais distantes com órbitas de longo período que outros métodos não são capazes de detectar.
Matter ejections behind the highs and lows of the transitional millisecond pu...Sérgio Sacani
Transitional millisecond pulsars are an emerging class of sources linking low-mass X-ray binaries to millisecond radio pulsars in
binary systems. These pulsars alternate between a radio pulsar state and an active low-luminosity X-ray disc state. During the active
state, these sources exhibit two distinct emission modes (high and low) that alternate unpredictably, abruptly, and incessantly. X-ray
to optical pulsations are observed only during the high mode. Knowledge of the root reason for this puzzling behaviour remains
elusive. This paper presents the results of the most extensive multi-wavelength campaign ever conducted on the transitional pulsar
prototype, PSR J1023+0038, covering from radio to X-rays. The campaign was carried out over two nights in June 2021, and involved
12 different telescopes and instruments including XMM-Newton, HST, VLT/FORS2 (in polarimetric mode), ALMA, VLA and FAST.
By modelling the broadband spectral energy distributions in both emission modes, we show that the mode switches are caused by
changes in the innermost region of the accretion disc. These changes trigger the emission of discrete mass ejections, which occur on
top of a compact jet, as testified by the detection of at least one short-duration millimetre flare with A
Complete Photoproduction Experiments - 12th International Conference on Meson-Nucleon Physics and the Structure of the Nucleon, Virginia, USA, 31 May-4 June 2010. AIP Conference Proceedings, October 2011, Vol. 1374, pp. 17-22, ISSN: 0094-243X, doi: 10.1063/1.3647092
di A. D’Angelo, K. Ardashev, C. Bade, O. Bartalini, V. Bellini, M. Blecher, J. P. Bocquet, M. Capogni, A. Caracappa, L. E. Casano, M. Castoldi, R. Di Salvo, A. Fantini, D. Franco, G. Gervino, F. Ghio, G. Giardina, C. Gibson, B. Girolami, A. Giusa, H. Glu, K. Hicks, S. Hoblit, A. Honig, T. Kageya, M. Khandaker, O. C. Kistner, S. Kizilgul, S. Kucuker, A. Lapikf, A. Lehmann, P. Levi Sandri, A. Lleres, M. Lowry, M. Lucas, J. Mahon, F. Mammoliti, G. Mandaglio, M. Manganaro, L. Miceli, D. Moricciani, A. Mushkarenkovf, V. Nedorezovf, B. Norum, M. Papb, B. Preedom, H. Seyfarthb, C. Randieri, D. Rebreyend, N. Rudnevf, G. Russo, A. Sandorfi, C. Schaerf, M. L. Sperduto, H. Stroher, M. C. Sutera, C. E. Thorn, A. Turingef, V. Vegna, C. S. Whisnanth, K. Wang, X. Wei (2011)
Abstract
The extraction of resonance parameters from meson photo-reaction data is a challenging effort, that would greatly benefit from the availability of several polarization observables, measured for each reaction channel on both proton and neutron targets. In the aim of obtaining such complete experiments, polarized photon beams and targets have been developed at facilities, worldwide. We report on the latest results from the LEGS and GRAAL collaborations, providing single and double polarization measurements on pseudo-scalar meson photo-production from the nucleon.
Optical band gap measurement by diffuse reflectance spectroscopy (drs)Sajjad Ullah
Introduction to Optical band gap measurement
by electronic spectroscopy and diffuse reflectance spectroscopy (DRS) with comparison of the results obtained suing different equation and measurement techniques.
The role of scattering in extinction of light as it passes through media is briefly discussed.
I gave 1 hour seminar at ANSTO (Australian Nuclear Science and Technology Organization) to introduce my approach to magnetism. I see myself as an experimental physicist who is studying magnetism by using neutron scattering techniques. Throughout my career, I had learned local structure analysis (PDF), magnetic structural analysis, and inelastic neutron scattering technique to investigate superconductor, multiferroics, antiferromagnets, helimagnets, and frustrated magnets. I was trying to explain my approach to magnetism as an experiment physicist to both professional scientists and novices.
43 Beam asymmetry Σ measurements on the π- Photoproduction off neutrons - Phy...Cristian Randieri PhD
Beam asymmetry Σ measurements on the π- Photoproduction off neutrons - The American Physical Society, Physical Review C, Nuclear Physics, October 2010, Vol. 82, N. 4, pp. 045209-1-045209-7, ISSN: 0556-2813, doi: 10.1103/PhysRevC.82.045209
di G. Mandaglio, F. Mammoliti, M. Manganaro, V. Bellini, J. P. Bocquet, L. Casano, A. D'Angelo, R. Di Salvo, A. Fantini, D. Franco, G. Gervino, F. Ghio, G. Giardina, B. Girolami, A. Giusa, A. Ignatov, A. Lapik, P. Levi Sandri, A. Lleres, D. Moricciani, A. N. Mushkarenkov, V. Nedorezov, C. Randieri, D. Rebreyend, N. V. Rudnev, G. Russo, C. Schaerf, M. L. Sperduto, M. C. Sutera, A. Turinge, V. Vegna, W. J. Briscoe, I. I. Strakovsky (2010)
Abstract
The Σ beam asymmetry in the photoproduction of negative pions from quasi-free neutrons in a deuterium target was measured at Graal in the energy interval 700 - 1500 MeV and a wide angular range, using polarized and tagged photons. The results are compared with recent partial wave analyses.
They say casteism is no more. But there is no day when Dalits don't suffer by inhuman deeds with them. Even after 67-68 years of freedom, many many things are faced by dalits, rapes with their ladies is becoming very fascinating now a days. Lot many shameful deeds are still continuing, and importantly ..... no one fights for their rights but millions are fighting to end the reservation.....
Study of Raman Scattering in Carbon nanotubesajay singh
Abstract: Present thesis reports the Raman investigation of the Raman scattering in MWNTs as function of laser power. Raman spectra of MWNT were taken at laser parameters (514.5nm, 0.1- 0.6 w). The mathematical analysis of graphitic Raman peaks was done based on Einstein model. Earlier we chose Gaussian and Lorentzian weighting function to investigate Raman graphitic peaks. Earlier we discussed about size dependent Raman scattering in CNTs. When the laser power is increased from a minimum value, it causes the increase in induced temperature in the sample. In this section we have discussed Temperature dependence on Raman spectra. The temperature dependence of linewidth has been interpreted as due to decay of optical phonon into two LA phonons at half optical frequency. Temperature rise in the sample was calculated theoretically as well as experimentally.
Study of size dependence of Raman scattering in Carbon nanotubes.
To Study Temperature dependence of Raman spectra
To Study spatial distribution of temperature during laser processing
To Study Temperature rise in CNTs as a function of laser power
Theoretically calculated Vs Experimental Raman temperature
2024.06.01 Introducing a competency framework for languag learning materials ...Sandy Millin
http://sandymillin.wordpress.com/iateflwebinar2024
Published classroom materials form the basis of syllabuses, drive teacher professional development, and have a potentially huge influence on learners, teachers and education systems. All teachers also create their own materials, whether a few sentences on a blackboard, a highly-structured fully-realised online course, or anything in between. Despite this, the knowledge and skills needed to create effective language learning materials are rarely part of teacher training, and are mostly learnt by trial and error.
Knowledge and skills frameworks, generally called competency frameworks, for ELT teachers, trainers and managers have existed for a few years now. However, until I created one for my MA dissertation, there wasn’t one drawing together what we need to know and do to be able to effectively produce language learning materials.
This webinar will introduce you to my framework, highlighting the key competencies I identified from my research. It will also show how anybody involved in language teaching (any language, not just English!), teacher training, managing schools or developing language learning materials can benefit from using the framework.
The Roman Empire A Historical Colossus.pdfkaushalkr1407
The Roman Empire, a vast and enduring power, stands as one of history's most remarkable civilizations, leaving an indelible imprint on the world. It emerged from the Roman Republic, transitioning into an imperial powerhouse under the leadership of Augustus Caesar in 27 BCE. This transformation marked the beginning of an era defined by unprecedented territorial expansion, architectural marvels, and profound cultural influence.
The empire's roots lie in the city of Rome, founded, according to legend, by Romulus in 753 BCE. Over centuries, Rome evolved from a small settlement to a formidable republic, characterized by a complex political system with elected officials and checks on power. However, internal strife, class conflicts, and military ambitions paved the way for the end of the Republic. Julius Caesar’s dictatorship and subsequent assassination in 44 BCE created a power vacuum, leading to a civil war. Octavian, later Augustus, emerged victorious, heralding the Roman Empire’s birth.
Under Augustus, the empire experienced the Pax Romana, a 200-year period of relative peace and stability. Augustus reformed the military, established efficient administrative systems, and initiated grand construction projects. The empire's borders expanded, encompassing territories from Britain to Egypt and from Spain to the Euphrates. Roman legions, renowned for their discipline and engineering prowess, secured and maintained these vast territories, building roads, fortifications, and cities that facilitated control and integration.
The Roman Empire’s society was hierarchical, with a rigid class system. At the top were the patricians, wealthy elites who held significant political power. Below them were the plebeians, free citizens with limited political influence, and the vast numbers of slaves who formed the backbone of the economy. The family unit was central, governed by the paterfamilias, the male head who held absolute authority.
Culturally, the Romans were eclectic, absorbing and adapting elements from the civilizations they encountered, particularly the Greeks. Roman art, literature, and philosophy reflected this synthesis, creating a rich cultural tapestry. Latin, the Roman language, became the lingua franca of the Western world, influencing numerous modern languages.
Roman architecture and engineering achievements were monumental. They perfected the arch, vault, and dome, constructing enduring structures like the Colosseum, Pantheon, and aqueducts. These engineering marvels not only showcased Roman ingenuity but also served practical purposes, from public entertainment to water supply.
Introduction to AI for Nonprofits with Tapp NetworkTechSoup
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1. Bragg Solitons
Research Scholar
Center for Nanoscience and Engineering
Indian Institute of Science, Bangalore
Course presentation: Nonlinear Photonics
Ajay Singh
2. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Fiber Brag Grating
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
3. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Fiber Brag Grating
How to write:
Irradiation from UV
Irradiate germanium doped
fiber with argon laser
Holographic technique
kg= 2π/Λ
Λ =~o.5 µm for λ=1.55 µm region
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
4. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Fiber Brag Grating Coupled-Mode Equations
How to write:
Irradiation from UV
Irradiate germanium doped
fiber with argon laser
Holographic technique
kg= 2π/Λ
Λ =~o.5 µm for λ=1.55 µm region
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
5. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Fiber Brag Grating Coupled-Mode Equations
How to write:
Irradiation from UV
Irradiate germanium doped
fiber with argon laser
Holographic technique
kg= 2π/Λ
Λ =~o.5 µm for λ=1.55 µm region
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
6. Coupled-Mode Equations and Nonlinear Propagation Equations
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
7. Coupled-Mode Equations and Nonlinear Propagation Equations
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
8. Coupled-Mode Equations and Nonlinear Propagation Equations
Anomalous
GVD
Normal
GVD
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
Link
10. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Effective NLS Equation
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal”
cademic PressElsevier Science, USA (2003)
Now introduce the speed reduction factor
f:
11. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Effective NLS Equation
Fig.. Intensity (solid
line) and normalized
spatial width (dot-
dashed line) of
fundamental soliton
pulses, [6].
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal”
cademic PressElsevier Science, USA (2003)
Now introduce the speed reduction factor
f:
12. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Effective NLS Equation
Fig.. Intensity (solid
line) and normalized
spatial width (dot-
dashed line) of
fundamental soliton
pulses, [6].
Fig. Evoluation of (a) |Af|2 and (b) |Ab|2 [6].
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal”
cademic PressElsevier Science, USA (2003)
Now introduce the speed reduction factor
f:
13. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Let us consider different cases of Bragg solitons
1-<v<1
Ψ=π/2: Center of the stop band: Combination of two counter-propogating waves VG = v.νg
If equal amplitude: νg= 0 Stationary gap soliton
|v|=1
Bragg soliton ceases to exist since the grating becomes ineffactive
General solution (coupled mode eqn) of shape preserving solitons: Solition exist in normal
Dispersion region also: Dark solitions
Video: Propagation of a
single bragg soliton in a
uniform grating [17]
14. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B [7]
Fig. Schematic of our experimental setup.
15. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B [7]
Fig. Schematic of our experimental setup.
Link
16. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Fig. Schematic of our experimental setup.
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B [7]
Link
818 m-1
3612 m-1
17. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B [7]
18. Link
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B [7]
19. Fig. 16. transmitted pulse for incoming pulse energies of 0.66
µJ Left experimental results; right follow numerical
calculation.(solid curves) The values of the detuning are 876 m-
1 [traces (a) and (b)], 994 m-1 [traces (c) and (d)], 1318 m-1
[traces (e) and (f )], and 1847 m-1 [traces (g) and (h)].
Intensity(a.u.)
Link
Link
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B [7]
Link
20. Mathematical Analysis…..
• All-optical switching [5,8,9],
• Pulse compression [10,11,25],
• Pulse Limiting [12],
• Logic operations [13],
• Promising for the fiber-sensing technology [14],
• Optical communication systems [15,16],
• All optical buffers and storing devices can be based on such fibers [18],
• Pulse source for the soliton transmission system [19,20 ],
• All-optical modulation and demultiplexing systems [23],
• Tunable optical pulse source [24, 26],
• A possible way to trap a zero-velocity soliton is to use an attractive
finite-size or Local defect in BG [22] ,
• THz pulse generation !!!
• Suppercontinuum generation !!!
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Applications of Bragg Solitons…..
21. Solitons Bragg Grating Bragg Solitons Mathematical Analysis Applications
References:
[1] K. O. Hill, Y. Fujii, D. C. Johnson, and B. S. Kawasaki, Appl. Phys. Lett.,Vol. 32, pp. 647, 1978.
[2] E. Yablonovitchand T. J. Gmitter,Phys. Rev. Lett.,Vol. 63, pp. 1950, 1989.
[3] A. A. Sukhorukov, Y. S. Kivshar, H. S. Eisenberg and Y. Silberberg, IEEE J. QuantumElectron, Vol. 39, pp. 31, 2003.
[4] W. Chen and D. L. Mills, Phys. Rev. Lett., Vol. 58, pp. 160, 1987.
[5] S. Larochelle, V. Mizrahi, and G. Stegeman, Electron. Lett., Vol. 26, pp. 1459, 1990.
[6] A. B. Aceves and S. Wabnitz, Phys. Lett. A, Vol. 141, pp. 37, 1989.
[7] B. J. Eggleton,C. M. de, Sterke, and R. E. Slusher, J. Opt. Soc. Am. B, Vol. 16, pp. 587, 1999.
[8] N. G. R. Broderick, D. Taverner, and D. J. Richardson, Opt. Express,Vol. 3, pp. 447, 1998.
[9] Amer Kotb and Kyriakos, Optical Engineering (SPIE),Optical Engineering , Vol. 55(8), pp. 087109 (1-7), 2016.
[10] N. G. R. Broderick, D. Taverner, D. J. Richardson, M. Ibsen and R. I. Laming, Opt. Lett. Vol. 22, pp. 1837, 1997.
[11] N. G. R. Broderick, D. Taverner, D. J. Richardson, M. Ibsen and R. I. Laming, Phys. Rev. Lett.,Vol.79,pp. 4566, 1997.
[12] D. E. Pelinovsky, L. Brzozowski, and E. H. Sargent. Phys. Rev. E, Vol. 62, pp. 4536, 2000.
[13]. L. Brzozowski and E. H. Sargent, IEEE J. QuantumElectron, Vol. 36, pp. 550, 2000.
[14] W. C. K. Mak, B. A. Malomed, and P. L. Chu, J. Opt. Soc. Am. B, Vol. 20, pp. 725, 2003.
[15] R. H. Goodman, R. E. Slusher, and M. I. Weinstein,J. Opt. Soc. Am. B, Vol. 19, pp. 1635, 2002.
[16] G. P. Agrawal, Nonlinear Fiber Optics. (New York: Academic), 1989.
[17]. https://www.youtube.com/watch?v=GxmjYNuaoSE
[18]. Xiaolu Li, Yuesong Jiang, and Lijun Xu, Communicationand Network, Vol. 2, pp. 44, 2010
[19] N. Dogru and M. S. Ozyazici, LFNM. September 2004, pp. 115.
[20]. N. Dogru, 2005, IEEE NUSOD’05, September 2005, pp.89.
[21] C. M. de Sterke, B. J. Eggleton,and P. A. Krug, J. Lightwave Technol,Vol. 15, pp. 1494, 1997.
[22] K. T. Mc-Donald, Am. J. Phys., Vol. 68, pp. 293, 2000.
[23]. J. H. Lee, L. Katsuo, K. S. Berg, A. T. Clausen, D. J. Richardson, and P. Jeppesen, J. Lightwave Technol,Vol. 21, pp. 2518,
2003.
[24]. J. H. Lee, Y. M. Chang, Y. G. Han, S. H. Kim, H. Chung,and S. B. Lee, IEEEPhoton. Technol.Lett., Vol. 17, pp. 34, 2005.
[25]. G. Lenz and B. J. Eggleton,J. Opt. Soc. Am. B, Vol. 15, pp. 2980, 1998.
[26] Norihiko Nishizawa,Yoshimichi Andou, Emiko Omoda, Hiromichi Kataura, and Youichi Sakakibara, Opt. Exp. 23403, Vol.
24, 2016.
24. 1553.2 nm
Q-switching of the laser at a repetition rate of 500 Hz.
train of pulses, each with a duration of approximately 80 ps.
To avoid thermal effects, an electro-optic pulse selector was used to
select one pulse in each train.
fast photodiode with a response time of 9 ps
The net time resolution, including trigger jitter and oscilloscope
resolution, was approximately 20 ps.
75-mm-long unchirped, apodized fiber grating
Back
25. Schematic illustration of a fiber grating. Dark and light shaded regions
withi n the fiber core show periodic variations of the refractive index.
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
First photo-induced optical fiber Bragg gratings
by Hill and coworkers in 1978 [1]
Photonic band structure” concept: Yablonovitch
in the late 1980’s [2]
Light interaction with nonlinear periodic media
yields a diversity of fascinating phenomenan:
discrete (or lattice) solitons and gap (or Bragg)
solitons [11-12]
Larochelle, Hihino, Mizrahi and Stegeman (in
1990): experimental investigation of the optical
response of nonlinear periodic structures.
investigation of nonlinear pulse propagation in
uniform fiber gratings: the Bragg solitons easily
generated in the laboratory travel at 60–80% of
veocity of light in fiber absence of grating [5]
Fiber Brag Grating
How to write:
Irradiation from UV
Irradiate germanium
doped fiber with argon
laser
Holographic technique
kg= 2π/Λ
Λ =~o.5 µm for λ=1.55 µm
region
Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
26. Optical solitons: From fibers to photonic crystals,“Yuri S. Kivshar and Govind P. Agrawal” cademic PressElsevier Science, USA (2003)
Coupled-Mode Equations
And here dispersion comes into play…..
Figure : Dispersion curves showing variation of 6 with q and the
existence of the photonic bandgap for a fiber grating.
Anomalous
GVD
Normal
GVD
o β2 changes its sign on the
two sides of the stop band
centered at the Bragg
wavelength, whose
location is easily
controlled and can be in
any region of the optical
spectrum.
o β2 is anomalous on the
shorter-wavelength side
of the stop band, unlike
for wavelengths longer
than the zero dispersion
wave-length in the fibers
o The magnitude of β2 >
100ps2/cm
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
o the negative sign appearing in front
of the ∂Ab/∂Z term: because of
backward propagation of Ab and
o the presence of linear coupling
between the counter propagating
waves governed by the parameter k
Back
27. Fig. 13. Comparison
between the estimated
pulse energy in the
fiber and the deduced
value of the peak
intensity. The result,
which is consistent
with the expected
proportionality
between the two
quantities, leads to a
proportionality
constant of 47 GW/cm2
µJ-1.
Fig. 8. Intensity versus
time after propagation
through the grating at a
pulse energy of
approximately 0.66 µJ,
for a detuning close to
the edge of the gap
(solid curve) and far
from the edge of the
gap (dashed curve). The
pulse tuned close to the
edge of the gap is
delayed by
approximately 310 ps,
corresponding to an
average velocity of
approximately 0.50V.
Fig. 7. Intensity versus
time after propagation
through the grating at a
peak input intensity of 11
GW/cm2, for seven
different values of the
detuning (solid curve,
729 m-1; dotted curve,
788 m-1; short-dashed
curve, 847 m-1; long-
dashed curve, 935 m-1;
short-dashed–dotted
curve, 1053 m-1; long-
dashed–dotted curve,
1406 m-1; long–short-
dashed curve, 3612 m-1)
Fig. 6. Delay of the
transmitted pulses
versus detuning at
low intensity.
Experimental
results are
indicated by dots,
numerical results by
the solid curve.
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B
Back
28. Fig. 16. transmitted pulse for incoming pulse energies of 0.66 µJ at 4 different
detunings. Left figures are experimental results; right follow from solving Eq. (1)
numerically and convolving the result with the estimated response of the detection
system (solid curves) and from the NLSE followed by a convolution (dashed curves).
The values of the detuning are 876 m-1 [traces (a) and (b)], 994 m-1 [traces (c) and
(d)], 1318 m-1 [traces (e) and (f )], and 1847 m-1 [traces (g) and (h)].
Fig. 9. FWHM of the
transmitted pulses versus
detuning at an estimated
pulse energy of 0.06 µJ.
Experimental results are
indicated by dots,
numerical results obtained
by solving Eq. (1) are
indicated by the solid
curve, and numerical
obtained by solving
q. (10) are indicated by the
dashed curve; in both sets
of numerical results the
peak intensity of the
incoming pulse is taken to
be 3 GW/cm2.
Fig. 15. Solid curve:
Estimated peak power of the
fundamental soliton versus
detuning with the
parameters from the text.
Dots: Similar results, but
deduced from the
experiments, with the
criterion that the width does
not change upon
propagation.
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B
Back
29. Fig. 5. Full-width at
half-maximum
(FWHM) of the
transmitted pulses
versus detuning at
low intensity.
Experimental
results are
indicated by dots,
numerical results
by the solid curve.
Solitons Bragg Grating Bragg Solitons Mathematical Analysis Experimental Applications
Fig. Schematic of our experimental setup.
B. J. Eggleton, R. E. Slusher (Bell Laboratories, Lucent Technologies, New Jersey 07974) and C.
Martijn de Sterke (University of Sydney): Vol. 16, No. 4/ April 1999/J.Opt. Soc. Am. B [7]
Fig. Intensity versus
time after propagation
through the grating at
low intensity, for seven
different values of the
detuning (solid curve,
818 m-1; dotted curve,
847 m-1; short-dashed
curve, 906 m-1; long-
dashed curve, 965 m-1;
short-dashed– dotted
curve, 1023 m-1; long-
dashed–dotted curve,
1171 m-1; long–short-
dashed curve, 3612 m-
1).
Back