This document provides a brief biography of Albert Einstein. It discusses that he was born in Germany in 1879 and showed an early curiosity about science. He struggled in elementary school but was top of his class. He later studied in Munich and Zurich, publishing several groundbreaking papers in 1905 on topics like the photoelectric effect and special relativity. Einstein had to flee Germany in the 1930s due to Nazi persecution of Jews and immigrated to the United States, where he spent his later career until passing away in 1955 at the age of 76.
NAME
Albert Einstein
PLACE OF BIRTH
March 14 1879
Ulm, Württemberg, Germany
OCCUPATION
Physicist , Scientist
EDUCATION
Luitpold Gymnasium , Eidgenossische Polytechnische Schule (Swiss Federal Polytechnic School)
PLACE OF DEATH
April 18, 1955
Princeton, New Jersey
NAME
Albert Einstein
PLACE OF BIRTH
March 14 1879
Ulm, Württemberg, Germany
OCCUPATION
Physicist , Scientist
EDUCATION
Luitpold Gymnasium , Eidgenossische Polytechnische Schule (Swiss Federal Polytechnic School)
PLACE OF DEATH
April 18, 1955
Princeton, New Jersey
This is a comprehensive endeavour regarding the Early Life & Education, Personal Life, Academic, & Scientific Career, Awards & Honors, and Publications of Albert Einstein
Know about the famous scientist 'Albert Einstein' in the minimal way. Present like an artist.
Presentation made by:- Sarthak Khurana in Google Drive Presentations
Nobel Prize winner Albert Einstein is one of the most influential and well-known physicist in history. Learn more about his life and work in this mini biography.
class XI Book Snapshot
Chapter 4 Albert Einstein At School
N.B : This is for reference only. Students are advised not to copy, but to take ideas and do the work in their own style-it builds your imagination.
A biographical ppt providing a complete account of the life and times of Albert Einstein including his childhood,major achievements and controversies,etc
This is a comprehensive endeavour regarding the Early Life & Education, Personal Life, Academic, & Scientific Career, Awards & Honors, and Publications of Albert Einstein
Know about the famous scientist 'Albert Einstein' in the minimal way. Present like an artist.
Presentation made by:- Sarthak Khurana in Google Drive Presentations
Nobel Prize winner Albert Einstein is one of the most influential and well-known physicist in history. Learn more about his life and work in this mini biography.
class XI Book Snapshot
Chapter 4 Albert Einstein At School
N.B : This is for reference only. Students are advised not to copy, but to take ideas and do the work in their own style-it builds your imagination.
A biographical ppt providing a complete account of the life and times of Albert Einstein including his childhood,major achievements and controversies,etc
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Einstein failed school but was truly a genius who changed the very foundations of physics.
Einstein’s four ground-breaking research papers pertaining to the Photoelectric effect, Brownian motion , special theory of relativity and E=mc2 were published in the Annalen der Physik scientific journal during 1905,the miracle year of his life.
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.
This pdf is about the Schizophrenia.
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The increased availability of biomedical data, particularly in the public domain, offers the opportunity to better understand human health and to develop effective therapeutics for a wide range of unmet medical needs. However, data scientists remain stymied by the fact that data remain hard to find and to productively reuse because data and their metadata i) are wholly inaccessible, ii) are in non-standard or incompatible representations, iii) do not conform to community standards, and iv) have unclear or highly restricted terms and conditions that preclude legitimate reuse. These limitations require a rethink on data can be made machine and AI-ready - the key motivation behind the FAIR Guiding Principles. Concurrently, while recent efforts have explored the use of deep learning to fuse disparate data into predictive models for a wide range of biomedical applications, these models often fail even when the correct answer is already known, and fail to explain individual predictions in terms that data scientists can appreciate. These limitations suggest that new methods to produce practical artificial intelligence are still needed.
In this talk, I will discuss our work in (1) building an integrative knowledge infrastructure to prepare FAIR and "AI-ready" data and services along with (2) neurosymbolic AI methods to improve the quality of predictions and to generate plausible explanations. Attention is given to standards, platforms, and methods to wrangle knowledge into simple, but effective semantic and latent representations, and to make these available into standards-compliant and discoverable interfaces that can be used in model building, validation, and explanation. Our work, and those of others in the field, creates a baseline for building trustworthy and easy to deploy AI models in biomedicine.
Bio
Dr. Michel Dumontier is the Distinguished Professor of Data Science at Maastricht University, founder and executive director of the Institute of Data Science, and co-founder of the FAIR (Findable, Accessible, Interoperable and Reusable) data principles. His research explores socio-technological approaches for responsible discovery science, which includes collaborative multi-modal knowledge graphs, privacy-preserving distributed data mining, and AI methods for drug discovery and personalized medicine. His work is supported through the Dutch National Research Agenda, the Netherlands Organisation for Scientific Research, Horizon Europe, the European Open Science Cloud, the US National Institutes of Health, and a Marie-Curie Innovative Training Network. He is the editor-in-chief for the journal Data Science and is internationally recognized for his contributions in bioinformatics, biomedical informatics, and semantic technologies including ontologies and linked data.
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.
Professional air quality monitoring systems provide immediate, on-site data for analysis, compliance, and decision-making.
Monitor common gases, weather parameters, particulates.
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.
Cancer cell metabolism: special Reference to Lactate PathwayAADYARAJPANDEY1
Normal Cell Metabolism:
Cellular respiration describes the series of steps that cells use to break down sugar and other chemicals to get the energy we need to function.
Energy is stored in the bonds of glucose and when glucose is broken down, much of that energy is released.
Cell utilize energy in the form of ATP.
The first step of respiration is called glycolysis. In a series of steps, glycolysis breaks glucose into two smaller molecules - a chemical called pyruvate. A small amount of ATP is formed during this process.
Most healthy cells continue the breakdown in a second process, called the Kreb's cycle. The Kreb's cycle allows cells to “burn” the pyruvates made in glycolysis to get more ATP.
The last step in the breakdown of glucose is called oxidative phosphorylation (Ox-Phos).
It takes place in specialized cell structures called mitochondria. This process produces a large amount of ATP. Importantly, cells need oxygen to complete oxidative phosphorylation.
If a cell completes only glycolysis, only 2 molecules of ATP are made per glucose. However, if the cell completes the entire respiration process (glycolysis - Kreb's - oxidative phosphorylation), about 36 molecules of ATP are created, giving it much more energy to use.
IN CANCER CELL:
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
Unlike healthy cells that "burn" the entire molecule of sugar to capture a large amount of energy as ATP, cancer cells are wasteful.
Cancer cells only partially break down sugar molecules. They overuse the first step of respiration, glycolysis. They frequently do not complete the second step, oxidative phosphorylation.
This results in only 2 molecules of ATP per each glucose molecule instead of the 36 or so ATPs healthy cells gain. As a result, cancer cells need to use a lot more sugar molecules to get enough energy to survive.
introduction to WARBERG PHENOMENA:
WARBURG EFFECT Usually, cancer cells are highly glycolytic (glucose addiction) and take up more glucose than do normal cells from outside.
Otto Heinrich Warburg (; 8 October 1883 – 1 August 1970) In 1931 was awarded the Nobel Prize in Physiology for his "discovery of the nature and mode of action of the respiratory enzyme.
WARNBURG EFFECT : cancer cells under aerobic (well-oxygenated) conditions to metabolize glucose to lactate (aerobic glycolysis) is known as the Warburg effect. Warburg made the observation that tumor slices consume glucose and secrete lactate at a higher rate than normal tissues.
1. Daffodil International University
Presentation of Physics
With RespectfulTeacher
Shalauddin Submitted By
Senior Lecturer in Physics
Departmentof NaturalSciences Md: Samiul Islam
Daffodil InternationalUniversity Id:141-15-3294
2. Albert
Einstein"Any intelligent fool can make things bigger, more
complex, and more violent. It takes a touch of genius --
and a lot of courage -- to move in the opposite direction."
3. EARLY AGE
Albert was born on March 14, 1879 in Ulm, in the
Germans Empire.
Albert was a typical boy in elementary school with difficulties
in his speech, yet he was the top student.
His curiosity began when his father showed him a pocket
compass and thought “There must be something in there
that causes the needle to spin besides the “empty space”.”
Einstein built models and mechanical devices just for fun
which showed his mathematical skills.
4. When his fathers company failed in 1894, his family
moved to different places.
He then decided to stay in Munich to finish his studies.
His father intended for him to pursue in
electrical engineering.
When Einstein joined his family in Pavia, he wrote his
first scientific work The Investigation of the State of
Aether in Magnetic fields.”
Einstein finished secondary school at age 17.
5. Marriages and
Children
Einstein met Mileva Marić the same year he enrolled at the
Polytechnic.
Over the years their friendship developed into romance.
In early 1902, They had a daughter named
Lieserl. A year later, Einstein and Mileva
married.
They then had two sons names Hans Albert and Eduard.
After 16 years of marriage Einstein and Marić divorced for the
reason that they had been living their lives apart for 5 years.
Einstein remarried a couple months later with Elsa Lowenthal.
They both immigrated to the United States. She then died in
1936.
6. Academic
Career
After completing his thesis with Alfred Kleiner, Albert was awarded
a PhD by the University of Zurich.
Annus_Mirabilis
That same year, in 1905 Albert published 4 “Annus Mirabilis”
papers which were on the photoelectric effect, Brownian
motion, special relativity, and the equivalence of matter and
energy. These papers introduced him to his academic career.
Three years later, he was recognized as a leading scientist and
became a professor.
7. Emigration to the United
States
Einstein was forced to leave Germany and enter the U.S
due to the new Chancellor, Adolf Hitler.
Albert had never felt so Jewish in his life.
Other scientists emigrated to the United
States.
8. Deat
hOn April 17, 1955 Albert suffered from internal bleeding
caused by the rupture of an abdominal aortic
aneurysm.
Albert did not want surgery and said “I want to go when I
want. It is tasteless to prolong life artificially. I have
done my share, it is time to go. I will do it elegantly.”
Einstein died at the age of 76. He was having to work
until the last day of hislife.