This is a talk I am giving the 21 November 2014 at the University of Bristol for the meeting on Functional Materials Far from equilibrium.
It is meant for a broad audience and summarises the result of our paper http://people.bath.ac.uk/maspm/tasepldp-submit.pdf
Detailing Coherent, Minimum Uncertainty States of Gravitons, as Semi Classical Components of Gravity Waves, and How Squeezed States Affect Upper Limits to Graviton Mass /• We present what is relevant to squeezed states of initial space time and how that affects both the composition of relic GW and also gravitons. A side issue to consider is if gravitons can be configured as semi classical “particles”, which is akin to the Pilot particles model of Quantum Mechanics as embedded in a larger non linear “deterministic” background.
First Presented Saturday, September 3, 2011 at the G999 Conference, Philadelphia, PA http://ggg999.org/
Next Presentation : Friday, September 9, SAN MARINO WORKSHOP ON ASTROPHYSICS AND COSMOLOGY
FOR MATTER AND ANTIMATTER
http://www.workshops-hadronic-mechanics.org/
San Marino, N. Italy
Discussion: The Nature of Semi-classical Nature of Gravity Reviewed; And Can We Use a Graviton Entanglement Version of the EPR System to Answer if The Graviton is Classical or Quantum in Origin?
Publisher’s note: Dr. Beckwith: I am honored that you have seen fit to acknowledge me in your presentations of today, September 3, 2011 at the G999 Conference in Philadelphia, and Friday, September 9, at the San Marino Workshop on Astrophysics and Cosmology For Matter and Antimatter, in San Marino, N. Italy.
In my view, these are rather extraordinary postulations, especially the probability of extra-universal black hole gravitational origins, along with expansion beyond Hawking of Quantum Wave theory and the “quantizing” of gravity. The latter may very well lead to a thorough reexamination of our concept of space and time, and that the latter might not be so unidirectional afterall. The potential is breathtaking, as it represents steps forward in proving the existence of subspace, the possibility of concomitant multi-universiality and 5D dimensionality of black holes.
Can time manipulation and Biefeld-Brown suggested electro-gravitics as a spacecraft propulsive methodology be far behind? I think not…
Detailing Coherent, Minimum Uncertainty States of Gravitons, as Semi Classical Components of Gravity Waves, and How Squeezed States Affect Upper Limits to Graviton Mass /• We present what is relevant to squeezed states of initial space time and how that affects both the composition of relic GW and also gravitons. A side issue to consider is if gravitons can be configured as semi classical “particles”, which is akin to the Pilot particles model of Quantum Mechanics as embedded in a larger non linear “deterministic” background.
First Presented Saturday, September 3, 2011 at the G999 Conference, Philadelphia, PA http://ggg999.org/
Next Presentation : Friday, September 9, SAN MARINO WORKSHOP ON ASTROPHYSICS AND COSMOLOGY
FOR MATTER AND ANTIMATTER
http://www.workshops-hadronic-mechanics.org/
San Marino, N. Italy
Discussion: The Nature of Semi-classical Nature of Gravity Reviewed; And Can We Use a Graviton Entanglement Version of the EPR System to Answer if The Graviton is Classical or Quantum in Origin?
Publisher’s note: Dr. Beckwith: I am honored that you have seen fit to acknowledge me in your presentations of today, September 3, 2011 at the G999 Conference in Philadelphia, and Friday, September 9, at the San Marino Workshop on Astrophysics and Cosmology For Matter and Antimatter, in San Marino, N. Italy.
In my view, these are rather extraordinary postulations, especially the probability of extra-universal black hole gravitational origins, along with expansion beyond Hawking of Quantum Wave theory and the “quantizing” of gravity. The latter may very well lead to a thorough reexamination of our concept of space and time, and that the latter might not be so unidirectional afterall. The potential is breathtaking, as it represents steps forward in proving the existence of subspace, the possibility of concomitant multi-universiality and 5D dimensionality of black holes.
Can time manipulation and Biefeld-Brown suggested electro-gravitics as a spacecraft propulsive methodology be far behind? I think not…
Original scientific paper on which September 3&9 presentations by Chongquing University's Dr. Andrew Beckwith is based, and published within the July 2011 edition of the Journal of Modern Physics. (Scientific Research Publishing)
First part of abstract, i.e. part I•
Detailing Coherent, Minimum Uncertainty States of Gravitons, g , y , as Semi Classical Components of Gravity Waves, and How Squeezed States Affect Upper Limits to Graviton Mass /•
“We present what is relevant to squeezed states of initial space time and how that affects both the composition of relic GW and also gravitons. A side ii f li GW, d l i id issue to consider is if gravitons can be configured as semi classical “particles”, which is akin to the Pilot particles model of Quantum Mechanics as embedded in a larger non linear “deterministic” background.” g g -Dr. Andrew Beckwith, Chongquing University, PRC
Links:
G999 Conference, Philadelphia, PA http://ggg999.org/
San Marino Workshop on Astrophysics and Cosmology For Matter and Antimatter, in San Marino, N. Italy.
http://www.workshops-hadronic-mechanics.org/
Slideshare: http://t.co/vEv2ci5
WordPress: http://asimov52.wordpress.com/2011/09/03/dr-andrew-beckwith-%E2%80%9Cdetailing-coherent-minimum-uncertainty-states-of-gravitons-g-y-as-semi-classical-components-of-gravity-waves-and-how-squeezed-states-affect-upper-limits-to-gravito/
Black hole entropy leads to the non-local grid dimensions theory Eran Sinbar
Based on Prof. Bekenstein and Prof. Hawking, the black hole maximal entropy , the maximum amount of information that a black hole can absorb, beyond its event horizon is proportional to the area of its event horizon divided by quantized area units, in the scale of Planck area (the square of Planck length).[1]
This quantization in entropy and information in the quantized units of Planck area leads us to the assumption that space is not “smooth” but rather divided into quantized units (“space cells”). Although the Bekenstein-Hawking entropy equation describes a specific case regarding the quantization of the 2D event horizon, this idea can be generalized to the standard 3 dimension (3D) flat space, outside and far away from the black hole’s event horizon. In this general case we assume that these quantized units of space are 3D quantized space “cells” in the scale of Planck length in each of its 3 dimensions.
If this is truly the case and the universe fabric of space is quantized to local 3D space cells in the magnitude size of Planck length scale in each dimension, than we assume that there must be extra non-local space dimensions situated in the non-local bordering’s of these 3D space cells since there must be something dividing space into these quantized space cells.
Our assumption is that these bordering’s are extra non local dimensions which we named as the “GRID” (or grid) extra dimensions, since they look like a non-local 3D grid bordering of the local 3D space cells. These non-local grid dimensions are responsible for all unexplained non-local phenomena’s like the well-known non-local entanglement or in the phrase of Albert Einstein “spooky action at a distance” [2].So by proving that space-time is quantized we prove the existence of the non-local grid dimension that divides space-time to these quantized 3D Planck scale cells.
Detailing Coherent, Minimum Uncertainty States of Gravitons, as Semi Classical Components of Gravity Waves, and How Squeezed States Affect Upper Limits to Graviton Mass /• We present what is relevant to squeezed states of initial space time and how that affects both the composition of relic GW and also gravitons. A side issue to consider is if gravitons can be configured as semi classical “particles”, which is akin to the Pilot particles model of Quantum Mechanics as embedded in a larger non linear “deterministic” background.
First Presented Saturday, September 3, 2011 at the G999 Conference, Philadelphia, PA http://ggg999.org/
Next Presentation : Friday, September 9, SAN MARINO WORKSHOP ON ASTROPHYSICS AND COSMOLOGY
FOR MATTER AND ANTIMATTER
http://www.workshops-hadronic-mechanics.org/
San Marino, N. Italy
Discussion: The Nature of Semi-classical Nature of Gravity Reviewed; And Can We Use a Graviton Entanglement Version of the EPR System to Answer if The Graviton is Classical or Quantum in Origin?
Publisher’s note: Dr. Beckwith: I am honored that you have seen fit to acknowledge me in your presentations of today, September 3, 2011 at the G999 Conference in Philadelphia, and Friday, September 9, at the San Marino Workshop on Astrophysics and Cosmology For Matter and Antimatter, in San Marino, N. Italy.
In my view, these are rather extraordinary postulations, especially the probability of extra-universal black hole gravitational origins, along with expansion beyond Hawking of Quantum Wave theory and the “quantizing” of gravity. The latter may very well lead to a thorough reexamination of our concept of space and time, and that the latter might not be so unidirectional afterall. The potential is breathtaking, as it represents steps forward in proving the existence of subspace, the possibility of concomitant multi-universiality and 5D dimensionality of black holes.
Can time manipulation and Biefeld-Brown suggested electro-gravitics as a spacecraft propulsive methodology be far behind? I think not…
Detailing Coherent, Minimum Uncertainty States of Gravitons, as Semi Classical Components of Gravity Waves, and How Squeezed States Affect Upper Limits to Graviton Mass /• We present what is relevant to squeezed states of initial space time and how that affects both the composition of relic GW and also gravitons. A side issue to consider is if gravitons can be configured as semi classical “particles”, which is akin to the Pilot particles model of Quantum Mechanics as embedded in a larger non linear “deterministic” background.
First Presented Saturday, September 3, 2011 at the G999 Conference, Philadelphia, PA http://ggg999.org/
Next Presentation : Friday, September 9, SAN MARINO WORKSHOP ON ASTROPHYSICS AND COSMOLOGY
FOR MATTER AND ANTIMATTER
http://www.workshops-hadronic-mechanics.org/
San Marino, N. Italy
Discussion: The Nature of Semi-classical Nature of Gravity Reviewed; And Can We Use a Graviton Entanglement Version of the EPR System to Answer if The Graviton is Classical or Quantum in Origin?
Publisher’s note: Dr. Beckwith: I am honored that you have seen fit to acknowledge me in your presentations of today, September 3, 2011 at the G999 Conference in Philadelphia, and Friday, September 9, at the San Marino Workshop on Astrophysics and Cosmology For Matter and Antimatter, in San Marino, N. Italy.
In my view, these are rather extraordinary postulations, especially the probability of extra-universal black hole gravitational origins, along with expansion beyond Hawking of Quantum Wave theory and the “quantizing” of gravity. The latter may very well lead to a thorough reexamination of our concept of space and time, and that the latter might not be so unidirectional afterall. The potential is breathtaking, as it represents steps forward in proving the existence of subspace, the possibility of concomitant multi-universiality and 5D dimensionality of black holes.
Can time manipulation and Biefeld-Brown suggested electro-gravitics as a spacecraft propulsive methodology be far behind? I think not…
Original scientific paper on which September 3&9 presentations by Chongquing University's Dr. Andrew Beckwith is based, and published within the July 2011 edition of the Journal of Modern Physics. (Scientific Research Publishing)
First part of abstract, i.e. part I•
Detailing Coherent, Minimum Uncertainty States of Gravitons, g , y , as Semi Classical Components of Gravity Waves, and How Squeezed States Affect Upper Limits to Graviton Mass /•
“We present what is relevant to squeezed states of initial space time and how that affects both the composition of relic GW and also gravitons. A side ii f li GW, d l i id issue to consider is if gravitons can be configured as semi classical “particles”, which is akin to the Pilot particles model of Quantum Mechanics as embedded in a larger non linear “deterministic” background.” g g -Dr. Andrew Beckwith, Chongquing University, PRC
Links:
G999 Conference, Philadelphia, PA http://ggg999.org/
San Marino Workshop on Astrophysics and Cosmology For Matter and Antimatter, in San Marino, N. Italy.
http://www.workshops-hadronic-mechanics.org/
Slideshare: http://t.co/vEv2ci5
WordPress: http://asimov52.wordpress.com/2011/09/03/dr-andrew-beckwith-%E2%80%9Cdetailing-coherent-minimum-uncertainty-states-of-gravitons-g-y-as-semi-classical-components-of-gravity-waves-and-how-squeezed-states-affect-upper-limits-to-gravito/
Black hole entropy leads to the non-local grid dimensions theory Eran Sinbar
Based on Prof. Bekenstein and Prof. Hawking, the black hole maximal entropy , the maximum amount of information that a black hole can absorb, beyond its event horizon is proportional to the area of its event horizon divided by quantized area units, in the scale of Planck area (the square of Planck length).[1]
This quantization in entropy and information in the quantized units of Planck area leads us to the assumption that space is not “smooth” but rather divided into quantized units (“space cells”). Although the Bekenstein-Hawking entropy equation describes a specific case regarding the quantization of the 2D event horizon, this idea can be generalized to the standard 3 dimension (3D) flat space, outside and far away from the black hole’s event horizon. In this general case we assume that these quantized units of space are 3D quantized space “cells” in the scale of Planck length in each of its 3 dimensions.
If this is truly the case and the universe fabric of space is quantized to local 3D space cells in the magnitude size of Planck length scale in each dimension, than we assume that there must be extra non-local space dimensions situated in the non-local bordering’s of these 3D space cells since there must be something dividing space into these quantized space cells.
Our assumption is that these bordering’s are extra non local dimensions which we named as the “GRID” (or grid) extra dimensions, since they look like a non-local 3D grid bordering of the local 3D space cells. These non-local grid dimensions are responsible for all unexplained non-local phenomena’s like the well-known non-local entanglement or in the phrase of Albert Einstein “spooky action at a distance” [2].So by proving that space-time is quantized we prove the existence of the non-local grid dimension that divides space-time to these quantized 3D Planck scale cells.
These are the slide that I will be presenting next week in Darmstadt for teh Winter School on Spatial Models in Statistical Mechanics.
Basically, gives the main info on how to do my PhD.
PSOk-NN: A Particle Swarm Optimization Approach to Optimize k-Nearest Neighbo...Aboul Ella Hassanien
This talk presented at Bio-inspiring and evolutionary computation: Trends, applications and open issues workshop, 7 Nov. 2015 Faculty of Computers and Information, Cairo University
(If visualization is slow, please try downloading the file.)
Part 2 of a tutorial given in the Brazilian Physical Society meeting, ENFMC. Abstract: Density-functional theory (DFT) was developed 50 years ago, connecting fundamental quantum methods from early days of quantum mechanics to our days of computer-powered science. Today DFT is the most widely used method in electronic structure calculations. It helps moving forward materials sciences from a single atom to nanoclusters and biomolecules, connecting solid-state, quantum chemistry, atomic and molecular physics, biophysics and beyond. In this tutorial, I will try to clarify this pathway under a historical view, presenting the DFT pillars and its building blocks, namely, the Hohenberg-Kohn theorem, the Kohn-Sham scheme, the local density approximation (LDA) and generalized gradient approximation (GGA). I would like to open the black box misconception of the method, and present a more pedagogical and solid perspective on DFT.
First-order cosmological perturbations produced by point-like masses: all sca...Maxim Eingorn
This presentation based on the paper http://arxiv.org/abs/1509.03835 was made at Institute of Cosmology, Tufts University, on November 12, 2015. The abstract follows:
In the framework of the concordance cosmological model the first-order scalar and vector perturbations of the homogeneous background are derived without any supplementary approximations in addition to the weak gravitational field limit. The sources of these perturbations (inhomogeneities) are presented in the discrete form of a system of separate point-like gravitating masses. The obtained expressions for the metric corrections are valid at all (sub-horizon and super-horizon) scales and converge in all points except the locations of the sources, and their average values are zero (thus, first-order backreaction effects are absent). Both the Minkowski background limit and the Newtonian cosmological approximation are reached under certain well-defined conditions. An important feature of the velocity-independent part of the scalar perturbation is revealed: up to an additive constant it represents a sum of Yukawa potentials produced by inhomogeneities with the same finite time-dependent Yukawa interaction range. The suggesting itself connection between this range and the homogeneity scale is briefly discussed along with other possible physical implications.
ALL-SCALE cosmological perturbations and SCREENING OF GRAVITY in inhomogeneou...Maxim Eingorn
M. Eingorn, First-order cosmological perturbations engendered by point-like masses, ApJ 825 (2016) 84: http://iopscience.iop.org/article/10.3847/0004-637X/825/2/84
In the framework of the concordance cosmological model, the first-order scalar and vector perturbations of the homogeneous background are derived in the weak gravitational field limit without any supplementary approximations. The sources of these perturbations (inhomogeneities) are presented in the discrete form of a system of separate point-like gravitating masses. The expressions found for the metric corrections are valid at all (sub-horizon and super-horizon) scales and converge at all points except at the locations of the sources. The average values of these metric corrections are zero (thus, first-order backreaction effects are absent). Both the Minkowski background limit and the Newtonian cosmological approximation are reached under certain well-defined conditions. An important feature of the velocity-independent part of the scalar perturbation is revealed: up to an additive constant, this part represents a sum of Yukawa potentials produced by inhomogeneities with the same finite time-dependent Yukawa interaction range. The suggested connection between this range and the homogeneity scale is briefly discussed along with other possible physical implications.
We give an elementary exposition of a method to obtain the infinitesimal point symmetries of Lagrangians.Besides, we exhibit the Lanczos approach to Noether’s theorem to construct the first integral associated with each symmetry.
MSC 2010:49S05, 58E30, 70H25, 70H33
These are the slide that I will be presenting next week in Darmstadt for teh Winter School on Spatial Models in Statistical Mechanics.
Basically, gives the main info on how to do my PhD.
PSOk-NN: A Particle Swarm Optimization Approach to Optimize k-Nearest Neighbo...Aboul Ella Hassanien
This talk presented at Bio-inspiring and evolutionary computation: Trends, applications and open issues workshop, 7 Nov. 2015 Faculty of Computers and Information, Cairo University
(If visualization is slow, please try downloading the file.)
Part 2 of a tutorial given in the Brazilian Physical Society meeting, ENFMC. Abstract: Density-functional theory (DFT) was developed 50 years ago, connecting fundamental quantum methods from early days of quantum mechanics to our days of computer-powered science. Today DFT is the most widely used method in electronic structure calculations. It helps moving forward materials sciences from a single atom to nanoclusters and biomolecules, connecting solid-state, quantum chemistry, atomic and molecular physics, biophysics and beyond. In this tutorial, I will try to clarify this pathway under a historical view, presenting the DFT pillars and its building blocks, namely, the Hohenberg-Kohn theorem, the Kohn-Sham scheme, the local density approximation (LDA) and generalized gradient approximation (GGA). I would like to open the black box misconception of the method, and present a more pedagogical and solid perspective on DFT.
First-order cosmological perturbations produced by point-like masses: all sca...Maxim Eingorn
This presentation based on the paper http://arxiv.org/abs/1509.03835 was made at Institute of Cosmology, Tufts University, on November 12, 2015. The abstract follows:
In the framework of the concordance cosmological model the first-order scalar and vector perturbations of the homogeneous background are derived without any supplementary approximations in addition to the weak gravitational field limit. The sources of these perturbations (inhomogeneities) are presented in the discrete form of a system of separate point-like gravitating masses. The obtained expressions for the metric corrections are valid at all (sub-horizon and super-horizon) scales and converge in all points except the locations of the sources, and their average values are zero (thus, first-order backreaction effects are absent). Both the Minkowski background limit and the Newtonian cosmological approximation are reached under certain well-defined conditions. An important feature of the velocity-independent part of the scalar perturbation is revealed: up to an additive constant it represents a sum of Yukawa potentials produced by inhomogeneities with the same finite time-dependent Yukawa interaction range. The suggesting itself connection between this range and the homogeneity scale is briefly discussed along with other possible physical implications.
ALL-SCALE cosmological perturbations and SCREENING OF GRAVITY in inhomogeneou...Maxim Eingorn
M. Eingorn, First-order cosmological perturbations engendered by point-like masses, ApJ 825 (2016) 84: http://iopscience.iop.org/article/10.3847/0004-637X/825/2/84
In the framework of the concordance cosmological model, the first-order scalar and vector perturbations of the homogeneous background are derived in the weak gravitational field limit without any supplementary approximations. The sources of these perturbations (inhomogeneities) are presented in the discrete form of a system of separate point-like gravitating masses. The expressions found for the metric corrections are valid at all (sub-horizon and super-horizon) scales and converge at all points except at the locations of the sources. The average values of these metric corrections are zero (thus, first-order backreaction effects are absent). Both the Minkowski background limit and the Newtonian cosmological approximation are reached under certain well-defined conditions. An important feature of the velocity-independent part of the scalar perturbation is revealed: up to an additive constant, this part represents a sum of Yukawa potentials produced by inhomogeneities with the same finite time-dependent Yukawa interaction range. The suggested connection between this range and the homogeneity scale is briefly discussed along with other possible physical implications.
We give an elementary exposition of a method to obtain the infinitesimal point symmetries of Lagrangians.Besides, we exhibit the Lanczos approach to Noether’s theorem to construct the first integral associated with each symmetry.
MSC 2010:49S05, 58E30, 70H25, 70H33
Freezing of energy of a soliton in an external potentialAlberto Maspero
We study the dynamics of a soliton in the generalized NLS with a small external potential. We prove that there exists an effective mechanical system describing the dynamics of the soliton and that, for any positive integer r, the energy of such a mechanical system is almost conserved up to times of order ϵ^{−r}. In the rotational invariant case we deduce that the true orbit of the soliton remains close to the mechanical one up to times of order ϵ^{−r}.
The world is ever changing. As a result, many of the systems and phenomena we are interested in evolve over time resulting in time evolving datasets. Timeseries often display any interesting properties and levels of correlation. In this tutorial we will introduce the students to the use of Recurrent Neural Networks and LSTMs to model and forecast different kinds of timeseries.
GitHub: https://github.com/DataForScience/RNN
I am Bing Jr. I am a Signal Processing Assignment Expert at matlabassignmentexperts.com. I hold a Master's in Matlab Deakin University, Australia. I have been helping students with their assignments for the past 9 years. I solve assignments related to Signal Processing.
Visit matlabassignmentexperts.com or email info@matlabassignmentexperts.com. You can also call on +1 678 648 4277 for any assistance with Signal Processing Assignments.
A Fast Hadamard Transform for Signals with Sub-linear SparsityRobin Scheibler
The Hadamard transform is a popular orthogonal transform with a low-complexity algorithm with O(N log N) complexity. In this presentation, we describe a new sub-linear complexity algorithm to compute the Hadamard transform of signals whose Hadamard transform coefficients are sparse - that is very few are non-zero.
1. Where distributions comes from?
2. Interpret and compare distributions.
3. Why normal, chi-square, t and F distributions?
4. Distributions for survivals.
On Generalized Classical Fréchet Derivatives in the Real Banach SpaceBRNSS Publication Hub
In this work, we reviewed the Fréchet derivatives beginning with the basic definitions and touching most of the important basic results. These results include among others the chain rule, mean value theorem, and Taylor’s formula for differentiation. Obviously, having clarified that the Fréchet differential operators exist in the real Banach domain and that the operators are clearly continuous, we then in the last section for main results developed generalized results for the Fréchet derivatives of the chain rule, mean value theorem, and Taylor’s formula among others which become highly useful in the analysis of generalized Banach space problems and their solutions in Rn.
This is a talk I gave as part of the PSS the 5 February 2015 at the University of Bath. It is based on a paper by Mauro Mariani on a large deviation approach to Gamma convergence.
This is an introduction to Analytic Combinatorics. I gave this talk as part of the PSS the 9 October 2014 at the University of Bath... needless to say I threw in a couple of hipster jokes.
This is a talk that I gave as part of the PSS in the University of Bath. It is originally a Prezi presentation, the link is here:
http://prezi.com/gpbduz0tm2l2/?utm_campaign=share&utm_medium=copy
But I just discovered it can be downloaded as a pdf.
A glimpse into mathematical finance? The realm of option pricing modelsHoracio González Duhart
This talk was given by Istvan Redl on the 8 October 2013 as part of the PSS at the University of Bath.
http://people.bath.ac.uk/hgd20/pss.html
Abstract: After introducing one of the most important concepts of mathematical finance, the fundamental theorem of asset pricing (FTAP) and the related no arbitrage pricing theory (NAPT), I will briefly discuss the main techniques and tools extensively used in option pricing, namely Monte Carlo, Fourier Transform and PDE methods. In order to give a fairly well-structured overview of a great chunk of currently preferred models, through a simple example the hierarchy of the mathematical models will be demonstrated by going from the basic Black-Scholes to some more advanced models, e.g. Stochastic Volatility with jumps. (Even those people, who are familiar with these concepts, might find the main focus, i.e. structured overview, of this talk beneficial).
This is for a 10 minutes talk for the Meeting of Minds to be given on the 6 of June of 2013... don't know how many people will be there, but they are cataloged as "general public".
I'm pretty sure I also used it for the Symposium of Mexicans and Mexican Studies in the UK in Sheffield in 2013 (although I don't remember the exact date) or a very similar version.
Esta presentación la hice para enseñarle a una amiga unas dudas que tenía de Excel, ahorita me la volví a encontrar y soy super fan. Espero les sirva.
Además acabo de encontrar los datos que usé para los ejercicios, aquí están:
https://docs.google.com/spreadsheet/ccc?key=0Ahhuytu9wOaMdGdXWHlPYjBBRGNWWWZTM1hYUWx5SXc&usp=sharing
Esta plática la di a los alumnos de último año en la preparatoria donde estudié con el objetivo de promover el estudio de las matemáticas como carrera profesional está pensada como para 30 a 40 minutos. Ahora no encimé tanto las animaciones para que se pueda ver toda la información más fácilmente.
No tengo idea de cuando hice esta presentación... pero años después Magda me regaló esta versión del problema hecha de madera... aprovecho para subir una solución.
Estas diapositivas las presente para una platica de como 30 minutos en el ITAM durante la semana de Matematicas Aplicadas.
Introduce los modelos estructurales y habla un poco sobre lo que haciamos con estos modelos en la empresa donde laboraba en aquel entonces. No recuerdo la fecha exacta.
This is a talk I gave the 8 Nov 2011 for the postgraduate seminar at the University of Bath.
The talk was roughly half an hour long and it's a small introduction to my MSc dissertation.
These slides were used for a talk to primary school students during the masterclasses at the University of Bath at the beginning of 2012.
I really liked this one! :P
The ability to recreate computational results with minimal effort and actionable metrics provides a solid foundation for scientific research and software development. When people can replicate an analysis at the touch of a button using open-source software, open data, and methods to assess and compare proposals, it significantly eases verification of results, engagement with a diverse range of contributors, and progress. However, we have yet to fully achieve this; there are still many sociotechnical frictions.
Inspired by David Donoho's vision, this talk aims to revisit the three crucial pillars of frictionless reproducibility (data sharing, code sharing, and competitive challenges) with the perspective of deep software variability.
Our observation is that multiple layers — hardware, operating systems, third-party libraries, software versions, input data, compile-time options, and parameters — are subject to variability that exacerbates frictions but is also essential for achieving robust, generalizable results and fostering innovation. I will first review the literature, providing evidence of how the complex variability interactions across these layers affect qualitative and quantitative software properties, thereby complicating the reproduction and replication of scientific studies in various fields.
I will then present some software engineering and AI techniques that can support the strategic exploration of variability spaces. These include the use of abstractions and models (e.g., feature models), sampling strategies (e.g., uniform, random), cost-effective measurements (e.g., incremental build of software configurations), and dimensionality reduction methods (e.g., transfer learning, feature selection, software debloating).
I will finally argue that deep variability is both the problem and solution of frictionless reproducibility, calling the software science community to develop new methods and tools to manage variability and foster reproducibility in software systems.
Exposé invité Journées Nationales du GDR GPL 2024
Seminar of U.V. Spectroscopy by SAMIR PANDASAMIR PANDA
Spectroscopy is a branch of science dealing the study of interaction of electromagnetic radiation with matter.
Ultraviolet-visible spectroscopy refers to absorption spectroscopy or reflect spectroscopy in the UV-VIS spectral region.
Ultraviolet-visible spectroscopy is an analytical method that can measure the amount of light received by the analyte.
Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic ...Sérgio Sacani
We characterize the earliest galaxy population in the JADES Origins Field (JOF), the deepest
imaging field observed with JWST. We make use of the ancillary Hubble optical images (5 filters
spanning 0.4−0.9µm) and novel JWST images with 14 filters spanning 0.8−5µm, including 7 mediumband filters, and reaching total exposure times of up to 46 hours per filter. We combine all our data
at > 2.3µm to construct an ultradeep image, reaching as deep as ≈ 31.4 AB mag in the stack and
30.3-31.0 AB mag (5σ, r = 0.1” circular aperture) in individual filters. We measure photometric
redshifts and use robust selection criteria to identify a sample of eight galaxy candidates at redshifts
z = 11.5 − 15. These objects show compact half-light radii of R1/2 ∼ 50 − 200pc, stellar masses of
M⋆ ∼ 107−108M⊙, and star-formation rates of SFR ∼ 0.1−1 M⊙ yr−1
. Our search finds no candidates
at 15 < z < 20, placing upper limits at these redshifts. We develop a forward modeling approach to
infer the properties of the evolving luminosity function without binning in redshift or luminosity that
marginalizes over the photometric redshift uncertainty of our candidate galaxies and incorporates the
impact of non-detections. We find a z = 12 luminosity function in good agreement with prior results,
and that the luminosity function normalization and UV luminosity density decline by a factor of ∼ 2.5
from z = 12 to z = 14. We discuss the possible implications of our results in the context of theoretical
models for evolution of the dark matter halo mass function.
Salas, V. (2024) "John of St. Thomas (Poinsot) on the Science of Sacred Theol...Studia Poinsotiana
I Introduction
II Subalternation and Theology
III Theology and Dogmatic Declarations
IV The Mixed Principles of Theology
V Virtual Revelation: The Unity of Theology
VI Theology as a Natural Science
VII Theology’s Certitude
VIII Conclusion
Notes
Bibliography
All the contents are fully attributable to the author, Doctor Victor Salas. Should you wish to get this text republished, get in touch with the author or the editorial committee of the Studia Poinsotiana. Insofar as possible, we will be happy to broker your contact.
Phenomics assisted breeding in crop improvementIshaGoswami9
As the population is increasing and will reach about 9 billion upto 2050. Also due to climate change, it is difficult to meet the food requirement of such a large population. Facing the challenges presented by resource shortages, climate
change, and increasing global population, crop yield and quality need to be improved in a sustainable way over the coming decades. Genetic improvement by breeding is the best way to increase crop productivity. With the rapid progression of functional
genomics, an increasing number of crop genomes have been sequenced and dozens of genes influencing key agronomic traits have been identified. However, current genome sequence information has not been adequately exploited for understanding
the complex characteristics of multiple gene, owing to a lack of crop phenotypic data. Efficient, automatic, and accurate technologies and platforms that can capture phenotypic data that can
be linked to genomics information for crop improvement at all growth stages have become as important as genotyping. Thus,
high-throughput phenotyping has become the major bottleneck restricting crop breeding. Plant phenomics has been defined as the high-throughput, accurate acquisition and analysis of multi-dimensional phenotypes
during crop growing stages at the organism level, including the cell, tissue, organ, individual plant, plot, and field levels. With the rapid development of novel sensors, imaging technology,
and analysis methods, numerous infrastructure platforms have been developed for phenotyping.
DERIVATION OF MODIFIED BERNOULLI EQUATION WITH VISCOUS EFFECTS AND TERMINAL V...Wasswaderrick3
In this book, we use conservation of energy techniques on a fluid element to derive the Modified Bernoulli equation of flow with viscous or friction effects. We derive the general equation of flow/ velocity and then from this we derive the Pouiselle flow equation, the transition flow equation and the turbulent flow equation. In the situations where there are no viscous effects , the equation reduces to the Bernoulli equation. From experimental results, we are able to include other terms in the Bernoulli equation. We also look at cases where pressure gradients exist. We use the Modified Bernoulli equation to derive equations of flow rate for pipes of different cross sectional areas connected together. We also extend our techniques of energy conservation to a sphere falling in a viscous medium under the effect of gravity. We demonstrate Stokes equation of terminal velocity and turbulent flow equation. We look at a way of calculating the time taken for a body to fall in a viscous medium. We also look at the general equation of terminal velocity.
Nutraceutical market, scope and growth: Herbal drug technologyLokesh Patil
As consumer awareness of health and wellness rises, the nutraceutical market—which includes goods like functional meals, drinks, and dietary supplements that provide health advantages beyond basic nutrition—is growing significantly. As healthcare expenses rise, the population ages, and people want natural and preventative health solutions more and more, this industry is increasing quickly. Further driving market expansion are product formulation innovations and the use of cutting-edge technology for customized nutrition. With its worldwide reach, the nutraceutical industry is expected to keep growing and provide significant chances for research and investment in a number of categories, including vitamins, minerals, probiotics, and herbal supplements.
What is greenhouse gasses and how many gasses are there to affect the Earth.moosaasad1975
What are greenhouse gasses how they affect the earth and its environment what is the future of the environment and earth how the weather and the climate effects.
Remote Sensing and Computational, Evolutionary, Supercomputing, and Intellige...University of Maribor
Slides from talk:
Aleš Zamuda: Remote Sensing and Computational, Evolutionary, Supercomputing, and Intelligent Systems.
11th International Conference on Electrical, Electronics and Computer Engineering (IcETRAN), Niš, 3-6 June 2024
Inter-Society Networking Panel GRSS/MTT-S/CIS Panel Session: Promoting Connection and Cooperation
https://www.etran.rs/2024/en/home-english/
2. nite TASEP: Large Deviations via
Matrix Products
H. G. Duhart, P. Morters, J. Zimmer
University of Bath
21 November 2014
3. The TASEP
The totally asymmetric simple exclusion process is one of the
simplest interacting particle systems. It was introduced by Liggett
in 1975.
Horacio Gonzalez Duhart TASEP: LDP via MPA
4. The TASEP
The totally asymmetric simple exclusion process is one of the
simplest interacting particle systems. It was introduced by Liggett
in 1975.
Create particles in site 1 at rate 2 (0; 1).
Horacio Gonzalez Duhart TASEP: LDP via MPA
5. The TASEP
The totally asymmetric simple exclusion process is one of the
simplest interacting particle systems. It was introduced by Liggett
in 1975.
Create particles in site 1 at rate 2 (0; 1).
Particles jump to the right with rate 1.
Horacio Gonzalez Duhart TASEP: LDP via MPA
6. The TASEP
The totally asymmetric simple exclusion process is one of the
simplest interacting particle systems. It was introduced by Liggett
in 1975.
Create particles in site 1 at rate 2 (0; 1).
Particles jump to the right with rate 1.
At most one particle per site.
Horacio Gonzalez Duhart TASEP: LDP via MPA
7. The TASEP
The totally asymmetric simple exclusion process is one of the
simplest interacting particle systems. It was introduced by Liggett
in 1975.
Create particles in site 1 at rate 2 (0; 1).
Particles jump to the right with rate 1.
At most one particle per site.
1
. . .
Horacio Gonzalez Duhart TASEP: LDP via MPA
8. The TASEP
Formally, the state space is f0; 1gN and its generator:
Gf () = (1 1)
f (1) f ()
+
X
k2N
k(1 k+1)
f (k;k+1) f ()
Horacio Gonzalez Duhart TASEP: LDP via MPA
9. The TASEP
Theorem (Liggett 1975)
Let be a product measure on f0; 1gN for which
:= lim
k!1
f : k = 1g exists. Then there exist probability
measures %
de
10. ned if either 1
2 and % 1 , or 1
2 and
12
% 1, which are asymptotically product with density %, such
that
if
1
2
then lim
t!1
S(t) =
(
if 1
if 1 ;
and if
1
2
then lim
t!1
S(t) =
8
:
1=2 if
1
2
if
1
2
.
Horacio Gonzalez Duhart TASEP: LDP via MPA
11. Main result
We will assume that our process f(t)gt0 starts with no
particles. That is
P[k(0) = 0 8k 2 N] = 1
Horacio Gonzalez Duhart TASEP: LDP via MPA
12. Main result
We will assume that our process f(t)gt0 starts with no
particles. That is
P[k(0) = 0 8k 2 N] = 1
Working under the reached invariant measure, we will
13. nd a
large deviation principle for the sequence of random variables
fXngn2N of the empirical density of the
14. rst n sites.
Xn =
1
n
Xn
k=1
k
Horacio Gonzalez Duhart TASEP: LDP via MPA
16. nite TASEP with
injection rate 2 (0; 1) starting with an empty lattice. Then,
under the invariant probability measure given by Theorem 1,
fXngn2N satis
17. es a large deviation principle with convex rate
function I : [0; 1] ! [0;1] given as follows:
(a) If
1
2
, then I (x) = x log
x
+ (1 x) log
1 x
1
.
(b) If
1
2
, then
I (x) =
8
:
x log
x
+ (1 x) log
1 x
1
+ log (4(1 )) if 0 x 1 ;
2 [x log x + (1 x) log(1 x) + log 2] if 1 x
1
2
;
x log x + (1 x) log(1 x) + log 2 if
1
2
x 1:
Horacio Gonzalez Duhart TASEP: LDP via MPA
19. The MPA
Grokinsky (2004), based on the work of Derrida et. al. (1993),
found a way to completely characterise the measure of Theorem 1
via a matrix representation.
Theorem (Grokinsky)
Suppose there exist (possibly in
24. The MPA
The invariant measure given by Liggett is the same as the one
given by Grokinsky.
Horacio Gonzalez Duhart TASEP: LDP via MPA
25. The MPA
The invariant measure given by Liggett is the same as the one
given by Grokinsky.
We will focus on the case when we start with an empty lattice.
Horacio Gonzalez Duhart TASEP: LDP via MPA
26. The MPA
12
The invariant measure given by Liggett is the same as the one
given by Grokinsky.
We will focus on the case when we start with an empty lattice.
When , sites behave like iid Bernoulli random variables
with parameter .
Horacio Gonzalez Duhart TASEP: LDP via MPA
27. The MPA
12
The invariant measure given by Liggett is the same as the one
given by Grokinsky.
We will focus on the case when we start with an empty lattice.
When , sites behave like iid Bernoulli random variables
with parameter .
We can
28. nd explicit solutions for the matrices and vectors in
the case 1
2 .
Horacio Gonzalez Duhart TASEP: LDP via MPA
29. The MPA
12
The invariant measure given by Liggett is the same as the one
given by Grokinsky.
We will focus on the case when we start with an empty lattice.
When , sites behave like iid Bernoulli random variables
with parameter .
We can
30. nd explicit solutions for the matrices and vectors in
the case 1
2 .
D =
0
1 1 0 0
0 1 1 0
0 0 1 1
0 0 0 1
BBBBBB@
. . .
...
...
...
...
. . .
1
CCCCCCA
; E =
0
1 0 0 0
1 1 0 0
0 1 1 0
0 0 1 1
BBBBBB@
. . .
...
...
...
...
. . .
1
CCCCCCA
; v =
0
BBB@
1
2
3
...
1
CCCA
;
and wT =
1;
1
1;
1
1
2
;
Horacio Gonzalez Duhart TASEP: LDP via MPA
37. nition (Large deviation principle)
Let X be a Polish space. Let fPngn2N be a sequence of probability
of measures on X. We say fPngn2N satis
38. es a large deviation
principle with rate function I if the following three conditions meet:
i) I is a rate function (non-negative and lsc).
ii) lim sup
n!1
1
n
log Pn[F] inf
x2F
I (x) 8F X closed
iii) lim inf
n!1
1
n
log Pn[G] inf
x2G
I (x) 8G X open:
Horacio Gonzalez Duhart TASEP: LDP via MPA
39. Large deviations
The study of large deviations has been developed since
Varadhan uni
40. ed the theory in 1966.
Horacio Gonzalez Duhart TASEP: LDP via MPA
41. Large deviations
The study of large deviations has been developed since
Varadhan uni
42. ed the theory in 1966.
The result we will use for our proof the Gartner-Ellis Theorem.
Horacio Gonzalez Duhart TASEP: LDP via MPA
43. Large deviations
The study of large deviations has been developed since
Varadhan uni
44. ed the theory in 1966.
The result we will use for our proof the Gartner-Ellis Theorem.
Theorem (Gartner-Ellis)
Let fXngn2N be a sequence of random variables on a probability
space (
;A; P), where
is a nonempty subset of R. If the limit
cumulant generating function : R ! R de
45. ned by
() = lim
n!1
1n
log E[enXn ]
exists and is dierentiable on all R, then fXngn2N satis
46. es a large
deviation principle with rate function I :
! [1;1] de
47. ned by
I (x) = sup
fx ()g:
2R
Horacio Gonzalez Duhart TASEP: LDP via MPA
48. Idea of the proof of the main result
Now the idea is to use the the MPA in calculating the
function in Gartner-Ellis Theorem.
Horacio Gonzalez Duhart TASEP: LDP via MPA
49. Idea of the proof of the main result
Now the idea is to use the the MPA in calculating the
function in Gartner-Ellis Theorem.
() = lim
n!1
1
n
enXn
log E
= lim
n!1
1
n
h
exp
log E
Xn
k=1
k
i
Horacio Gonzalez Duhart TASEP: LDP via MPA
50. Idea of the proof of the main result
Now the idea is to use the the MPA in calculating the
function in Gartner-Ellis Theorem.
() = lim
n!1
1
n
enXn
log E
= lim
n!1
1
n
h
exp
log E
Xn
k=1
k
i
= lim
n!1
1
n
log
X
2f0;1gn
1=4f : k = k for k ng exp
Xn
k=1
k
!
Horacio Gonzalez Duhart TASEP: LDP via MPA
51. Idea of the proof of the main result
Now the idea is to use the the MPA in calculating the
function in Gartner-Ellis Theorem.
() = lim
n!1
1
n
enXn
log E
= lim
n!1
1
n
h
exp
log E
Xn
k=1
k
i
= lim
n!1
1
n
log
X
2f0;1gn
1=4f : k = k for k ng exp
Xn
k=1
k
!
= lim
n!1
1
n
log
wT (eD + E)nv
wT (D + E)nv
Horacio Gonzalez Duhart TASEP: LDP via MPA
52. Idea of the proof of the main result
Now the idea is to use the the MPA in calculating the
function in Gartner-Ellis Theorem.
() = lim
n!1
1
n
enXn
log E
= lim
n!1
1
n
h
exp
log E
Xn
k=1
k
i
= lim
n!1
1
n
log
X
2f0;1gn
1=4f : k = k for k ng exp
Xn
k=1
k
!
= lim
n!1
1
n
log
wT (eD + E)nv
wT (D + E)nv
= lim
n!1
1
n log wT (eD + E)nv 2 log 2:
Horacio Gonzalez Duhart TASEP: LDP via MPA
53. Idea of the proof of the main result
Having the equation
() = lim
n!1
1nlog wT (eD + E)nv 2 log 2
we would like to simplify it and use Gartner-Ellis Theorem.
Horacio Gonzalez Duhart TASEP: LDP via MPA
54. Idea of the proof of the main result
Having the equation
() = lim
n!1
1nlog wT (eD + E)nv 2 log 2
we would like to simplify it and use Gartner-Ellis Theorem.
However, even when we have a explicit form of D, E, v, and
w, the term wT (eD + E)nv is not easy to handle, and so we
split into a lower bound and an upper bound.
Horacio Gonzalez Duhart TASEP: LDP via MPA
55. Upper bound
2s
The upper bound comes from noticing that (eD + E) is a
Toeplitz operator (constant diagonals in the matrix), and v
and w live on a family of weighted spaces `and its dual,
respectively.
Horacio Gonzalez Duhart TASEP: LDP via MPA
56. Upper bound
2s
The upper bound comes from noticing that (eD + E) is a
Toeplitz operator (constant diagonals in the matrix), and v
and w live on a family of weighted spaces `and its dual,
respectively.
We then use Cauchy-Schwarz inequality and optimise over the
parameter s of permissible weights.
wT (eD + E)nv jwj`2?
s
jj(eD + E)njB(`2s
)jvj`2s
Horacio Gonzalez Duhart TASEP: LDP via MPA
57. Lower bound
The lower bound comes from expanding the term
wT (eD + E)nv =
Xn
p=1
Xp
j=0
f n
p;j ()wTEpjDjv
where f n
p;j () are polynomials on e with non-negative
coecients.
Horacio Gonzalez Duhart TASEP: LDP via MPA
58. Lower bound
The lower bound comes from expanding the term
wT (eD + E)nv =
Xn
p=1
Xp
j=0
f n
p;j ()wTEpjDjv
where f n
p;j () are polynomials on e with non-negative
coecients.
We then
59. nd a lower bound when j = 0:
wT (eD + E)nv
Xn
p=1
f n
p;0()wTEpv:
Horacio Gonzalez Duhart TASEP: LDP via MPA
60. Lower bound
The lower bound comes from expanding the term
wT (eD + E)nv =
Xn
p=1
Xp
j=0
f n
p;j ()wTEpjDjv
where f n
p;j () are polynomials on e with non-negative
coecients.
We then
61. nd a lower bound when j = 0:
wT (eD + E)nv
Xn
p=1
f n
p;0()wTEpv:
And another when j = p:
wT (eD + E)nv
Xn
p=1
f n
p;p()wTDpv:
Horacio Gonzalez Duhart TASEP: LDP via MPA
62. Summarising. . .
TASEP: Create particles at rate . Move them to the right at rate 1.
One particle per site.
Horacio Gonzalez Duhart TASEP: LDP via MPA
63. Summarising. . .
TASEP: Create particles at rate . Move them to the right at rate 1.
One particle per site.
MPA: Find matrices and vectors satisfying certain condition to
64. nd the
invariant measure.
Horacio Gonzalez Duhart TASEP: LDP via MPA
65. Summarising. . .
TASEP: Create particles at rate . Move them to the right at rate 1.
One particle per site.
MPA: Find matrices and vectors satisfying certain condition to
66. nd the
invariant measure.
LDP: Find the exponential rate of convergence to 0 of unlikely events.
Horacio Gonzalez Duhart TASEP: LDP via MPA
67. Summarising. . .
TASEP: Create particles at rate . Move them to the right at rate 1.
One particle per site.
MPA: Find matrices and vectors satisfying certain condition to
68. nd the
invariant measure.
LDP: Find the exponential rate of convergence to 0 of unlikely events.
Our result: Find an LDP of the empirical density of the TASEP via the
MPA.
Horacio Gonzalez Duhart TASEP: LDP via MPA
69. Summarising. . .
TASEP: Create particles at rate . Move them to the right at rate 1.
One particle per site.
MPA: Find matrices and vectors satisfying certain condition to
70. nd the
invariant measure.
LDP: Find the exponential rate of convergence to 0 of unlikely events.
Our result: Find an LDP of the empirical density of the TASEP via the
MPA.
Horacio Gonzalez Duhart TASEP: LDP via MPA
71. References
F. den Hollander. Large Deviations, volume 14 of Fields Institute
Monographs. American Mathematical Society, Providence, RI, 2000.
B. Derrida, M. R. Evans, V. Hakim, and V. Pasquier. Exact solution
of a 1D asymmetric exclusion model using a matrix formulation. J.
Phys. A, 26(7):1493,1993.
S. Grokinsky. Phase transitions in nonequilibrium stochastic
particle systems with local conservation laws. PhD thesis, TU
Munich, 2004.
T. M. Liggett. Ergodic theorems for the asymmetric simple
exclusion process. Trans. Amer. Math. Soc., 213:237-261,1975.
H. G. Duhart, P. Morters, and J. Zimmer. The Semi-In
72. nite
Asymmetric Exclusion Process: Large Deviations via Matrix
Products. ArXiv e-prints, arXiv:1411.3270v1, November 2014.
Horacio Gonzalez Duhart TASEP: LDP via MPA