SUSY in d=3, N=2

•

0 likes•172 views

Flip Tanedo

Presented at the Cornell Graduate Student BSM Journal Club, 28 January 2012.

Science

Viewers also liked

U.E.F "Andres F. Cordova"

San Zambrano

Martin brittany 4.4 final project

musiclover123

Steve Pharoah November Online Version 2015

Steve Pharoah

Presentation1

SHereen Salah

Matthew Taylor PPP Project

MatthewATaylor

cvresume

Claire Henry, M.Ed.,CDP

바둑이게임ょ※SDS119。COM☆め실전게임바둑이사이트dd2

임 상호

Trabajos de los informes de word

stalingeo

QNT 351 Final Exam Answers 1) The main purpose of descriptive statistics is to A. summarize data in a useful and informative manner B. make inferences about a population C. determine if the data adequately represents the population D. gather or collect data 2) The general process of gathering, organizing, summarizing, analyzing, and interpreting data is called A. statistics B. descriptive statistics C. inferential statistics D. levels of measurement 3) The performance of personal and business investments is measured as a percentage, return on investment. What type of variable is return on investment? A. Qualitative B. Continuous C. Attribute D. Discrete 4) What type of variable is the number of robberies reported in your city? A. Attribute B. Continuous C. Discrete D. Qualitative 5) What level of measurement is the number of auto accidents reported in a given month? A. Nominal B. Ordinal C. Interval D. Ratio 6) The names of

QNT 351 Final Exam Answers 2015 version

mahallbethena

Qué es un blog

Xtaby Rosas

Correcting Students

Belén Correa

온라인경마사이트に※SDS119。COM☆づ경마맞떼기ww8

임 상호

인터넷경마ば※SDS119。COM☆な라이브경마cc8

임 상호

JohnA.Roderesume

John Rode

clement cc proceedings APS 2015

Albert Einstein College of Medicine

온라인바둑이や※SDS119。COM☆ぽ인터넷바둑이사이트ee8

임 상호

Viewers also liked (16)

U.E.F "Andres F. Cordova"

Martin brittany 4.4 final project

Steve Pharoah November Online Version 2015

Presentation1

Matthew Taylor PPP Project

cvresume

바둑이게임ょ※SDS119。COM☆め실전게임바둑이사이트dd2

Trabajos de los informes de word

QNT 351 Final Exam Answers 2015 version

Qué es un blog

Correcting Students

온라인경마사이트に※SDS119。COM☆づ경마맞떼기ww8

인터넷경마ば※SDS119。COM☆な라이브경마cc8

JohnA.Roderesume

clement cc proceedings APS 2015

온라인바둑이や※SDS119。COM☆ぽ인터넷바둑이사이트ee8

More from Flip Tanedo

A preponderance of scientific evidence over the last hundred years tells us that our galaxy is filled with an unknown substance called dark matter. In fact, there is five times as much dark matter in the universe than there is ordinary matter: we are swimming in an ocean of dark matter and we have no firm idea what it is. We suspect that dark matter is composed of undiscovered elementary particles whose properties may, in turn, unlock some of the most pressing open questions in fundamental physics. So why haven't we figured out how to study dark matter in the lab, and why should we be optimistic that we may make progress in the coming decades?

Why Haven't We Discovered Dark Matter?

Flip Tanedo

Communicating Science Effectively

Flip Tanedo

Sustainable HEP

Flip Tanedo

Presented at the 2022 APS April Meeting, session Z05.00009 Abstract: We present a novel approach for student assessment in large physics lecture courses on student-recorded videos. Students record 5-minute videos teaching how to solve a problem to other students and are partially graded based on peer reviews from other students. After piloting this method during COVID-19 remote teaching over the last year and a half, we have found encouraging indications that it (1) promotes student self-efficacy and metacognition, (2) builds in a deeper engagement with the material, (3) encourages student creativity, (4) develops technical and critical communication ability, and (5) avoids long-standing issues with digital plagiarism. Though the method was developed during pandemic teaching, we propose that aspects can be readily applied to in-person teaching and scales with class size. We comment on the potential to support diverse student retention in physics and outline potential pedagogical trade-offs of this method.

Explainer Videos

Flip Tanedo

Invited talk at the American Physical Society April Meeting, 9 April 2022. Like many physical systems, the challenge to make physics more equitable is multiscale. The way in which one perceives and is able to change inequities changes over the early phase of an academic career. These changes reflect the scope of one's academic community, the evolving set of career incentives, and a growing ability to directly influence institutional norms. In this talk we provide a framework for how we engage with equity as early career academics. From this framework, we highlight the ways in which early career academics are uniquely qualified to affect change, and the ways institutions can ensure that these academics continue to be agents for positive change as mid-career scientists.

Equity as an Early Career Academic

Flip Tanedo

Diversity, Equity, and Inclusion: Perspectives and Unsolicited Opinions

Flip Tanedo

Snowmass: Theory and the Cosmic Frontier

Flip Tanedo

Popular Book Discussions: a platform for equity in physics

Flip Tanedo

Little Particles in a Big Universe

Flip Tanedo

Non-Traditional Assessment and Inclusivity in Physics Teaching

Flip Tanedo

How to hep-ph

Flip Tanedo

Attending to Diversity in the Physics Classroom

Flip Tanedo

The Invisible Universe and You

Flip Tanedo

Whatever happened to the WIMP of tomorrow?

Flip Tanedo

the ñ in my name

Flip Tanedo

Figuring It Out

Flip Tanedo

P39: the secret syllabus

Flip Tanedo

P39: How to Fail as a Physics Major

Flip Tanedo

P39: How To F Up Your Academic Career

Flip Tanedo

P39: I have no idea

Flip Tanedo

More from Flip Tanedo (20)

Why Haven't We Discovered Dark Matter?

Communicating Science Effectively

Sustainable HEP

Explainer Videos

Equity as an Early Career Academic

Diversity, Equity, and Inclusion: Perspectives and Unsolicited Opinions

Snowmass: Theory and the Cosmic Frontier

Popular Book Discussions: a platform for equity in physics

Little Particles in a Big Universe

Non-Traditional Assessment and Inclusivity in Physics Teaching

How to hep-ph

Attending to Diversity in the Physics Classroom

The Invisible Universe and You

Whatever happened to the WIMP of tomorrow?

the ñ in my name

Figuring It Out

P39: the secret syllabus

P39: How to Fail as a Physics Major

P39: How To F Up Your Academic Career

P39: I have no idea

Recently uploaded

Context. WASP-76 b has been a recurrent subject of study since the detection of a signature in high-resolution transit spectroscopy data indicating an asymmetry between the two limbs of the planet. The existence of this asymmetric signature has been confirmed by multiple studies, but its physical origin is still under debate. In addition, it contrasts with the absence of asymmetry reported in the infrared (IR) phase curve. Aims. We provide a more comprehensive dataset of WASP-76 b with the goal of drawing a complete view of the physical processes at work in this atmosphere. In particular, we attempt to reconcile visible high-resolution transit spectroscopy data and IR broadband phase curves. Methods. We gathered 3 phase curves, 20 occultations, and 6 transits for WASP-76 b in the visible with the CHEOPS space telescope. We also report the analysis of three unpublished sectors observed by the TESS space telescope (also in the visible), which represents 34 phase curves. Results. WASP-76 b displays an occultation of 260±11 and 152±10 ppm in TESS and CHEOPS bandpasses respectively. Depending on the composition assumed for the atmosphere and the data reduction used for the IR data, we derived geometric albedo estimates that range from 0.05 ± 0.023 to 0.146 ± 0.013 and from <0.13 to 0.189 ± 0.017 in the CHEOPS and TESS bandpasses, respectively. As expected from the IR phase curves, a low-order model of the phase curves does not yield any detectable asymmetry in the visible either. However, an empirical model allowing for sharper phase curve variations offers a hint of a flux excess before the occultation, with an amplitude of ∼40 ppm, an orbital offset of ∼−30◦ , and a width of ∼20◦ . We also constrained the orbital eccentricity of WASP-76 b to a value lower than 0.0067, with a 99.7% confidence level. This result contradicts earlier proposed scenarios aimed at explaining the asymmetry observed in high-resolution transit spectroscopy. Conclusions. In light of these findings, we hypothesise that WASP-76 b could have night-side clouds that extend predominantly towards its eastern limb. At this limb, the clouds would be associated with spherical droplets or spherically shaped aerosols of an unknown species, which would be responsible for a glory effect in the visible phase curves.

Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b

Sérgio Sacani

STS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATION

rouseeyyy

PSYCHOSOCIAL NEEDS. in nursing II sem pptx

Suji236384

Clean In Place(CIP).pptx .

Poonam Aher Patil

Seismic Method Estimate velocity from seismic data.pptx

AlMamun560346

Chemical Tests; flame test, positive and negative ions test Edexcel Internati...

ssuser79fe74

Understanding circumstellar disks is of prime importance in astrophysics, however, their birth process remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, often wrapped into a sub-grid model, play a crucial role in disk formation and evolution. This calls for a combined approach in which both the protostar and circumstellar disk are studied in concert. Aims. We aim to elucidate the small scale physics and constrain sub-grid parameters commonly chosen in the literature by resolving the star-disk interaction. Methods. We carry out a set of very high resolution 3D radiative-hydrodynamics simulations that self-consistently describe the collapse of a turbulent dense molecular cloud core to stellar densities. We study the birth of the protostar, the circumstellar disk, and its early evolution (< 6 yr after protostellar formation). Results. Following the second gravitational collapse, the nascent protostar quickly reaches breakup velocity and sheds its surface material, thus forming a hot (∼ 103 K), dense, and highly flared circumstellar disk. The protostar is embedded within the disk, such that material can flow without crossing any shock fronts. The circumstellar disk mass quickly exceeds that of the protostar, and its kinematics are dominated by self-gravity. Accretion onto the disk is highly anisotropic, and accretion onto the protostar mainly occurs through material that slides on the disk surface. The polar mass flux is negligible in comparison. The radiative behavior also displays a strong anisotropy, as the polar accretion shock is shown to be supercritical whereas its equatorial counterpart is subcritical. We also f ind a remarkable convergence of our results with respect to initial conditions. Conclusions. These results reveal the structure and kinematics in the smallest spatial scales relevant to protostellar and circumstellar disk evolution. They can be used to describe accretion onto regions commonly described by sub-grid models in simulations studying larger scale physics.

Formation of low mass protostars and their circumstellar disks

Sérgio Sacani

Mustard, as a crop, is susceptible to a variety of pests that can affect its growth and yield. Here’s a rundown of some common pests that target mustard plants: Aphids: These small, sap-sucking insects can cause significant damage by feeding on the leaves and stems. Aphids also excrete a sticky substance known as honeydew, which can lead to the growth of sooty mold on the plants. Flea Beetles: These tiny beetles jump like fleas when disturbed and chew small holes in the leaves. They are particularly damaging in the early growth stages of the plant. Cabbage Loopers: The larvae of a type of moth, these caterpillars are known for their distinctive looping movement. They chew large holes in the leaves and can defoliate plants if present in large numbers. Diamondback Moth Larvae: Another caterpillar pest, these larvae chew small holes in the leaves and can cause extensive damage, especially when infestations are heavy. Whiteflies: These are tiny, winged insects that feed on plant sap and can quickly become a problem in greenhouse or close planting conditions. Like aphids, they also secrete honeydew. Cutworms: These are the larvae of certain types of moths and are known for cutting young plants at the stem base at ground level. They are most destructive during the night. Root Maggots: The larvae of root maggot flies, these pests attack the roots of mustard plants, causing wilting and potentially killing young plants. Harlequin Bugs: These are colorful stink bugs that suck the sap from mustard plant stems and leaves, causing the leaves to become stippled, wilt, and eventually die if the infestation is severe. Mustard Sawfly: The larvae of the mustard sawfly can cause considerable defoliation, as they feed voraciously on the leaves. Clubroot: Caused by a fungus-like organism, clubroot affects the roots, causing them to swell and distort. While technically a disease, it is often associated with pest management because controlling it involves similar preventative strategies. Control Measures: Managing pests in mustard involves a combination of cultural, biological, and chemical methods. Crop rotation, resistant varieties, timely sowing, maintaining plant health, and using natural predators like ladybugs and parasitic wasps can help keep pest populations under control. Chemical pesticides should be used as a last resort due to their potential impact on the environment and non-target species.

Pests of mustard_Identification_Management_Dr.UPR.pdf

PirithiRaju

GBSN - Microbiology (Unit 3)

Areesha Ahmad

Theoretical predictions and observational data indicate a class of sub-Neptune exoplanets may have water-rich interiors covered by hydrogen-dominated atmospheres. Provided suitable climate conditions, such planets could host surface liquid oceans. Motivated by recent JWST observations of K2-18 b, we self-consistently model the photochemistry and potential detectability of biogenic sulfur gases in the atmospheres of temperate sub-Neptune waterworlds for the first time. On Earth today, organic sulfur compounds produced by marine biota are rapidly destroyed by photochemical processes before they can accumulate to significant levels. Domagal-Goldman et al. suggest that detectable biogenic sulfur signatures could emerge in Archean-like atmospheres with higher biological production or low UV flux. In this study, we explore biogenic sulfur across a wide range of biological fluxes and stellar UV environments. Critically, the main photochemical sinks are absent on the nightside of tidally locked planets. To address this, we further perform experiments with a 3D general circulation model and a 2D photochemical model (VULCAN 2D) to simulate the global distribution of biogenic gases to investigate their terminator concentrations as seen via transmission spectroscopy. Our models indicate that biogenic sulfur gases can rise to potentially detectable levels on hydrogen-rich water worlds, but only for enhanced global biosulfur flux (20 times modern Earth’s flux). We find that it is challenging to identify DMS at 3.4 μm where it strongly overlaps with CH4, whereas it is more plausible to detect DMS and companion byproducts, ethylene (C2H4) and ethane (C2H6), in the mid-infrared between 9 and 13 μm. Unified Astronomy Thesaurus concepts: Exoplanet atmospheres (487); Exoplanet

Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds

Sérgio Sacani

GBSN - Biochemistry (Unit 1)

Areesha Ahmad

Vip CALL GIRL IN Lonavala 9748763073❤CALL GIRLS IN ESCORT SERVICE❤CALL GIRL IN We are Providing :- ● – Private independent collage Going girls . ● – independent Models . ● – House Wife’s . ● – Private Independent House Wife’s ● – Corporate M.N.C Working Profiles . ● – Call Center Girls . ● – Live Band Girls . ●- Foreigners & Many More . Service type: 1.In call 2.out call 3. full Lip to Lip kiss 4.69 5.b-job without Condom 6. Hard Core sex & Much More. 7 Body to Body Touch 8 Kissing 9 Sucking Boobs and More 10 Enjoy by Hand 11 Relax By Oral 12 Sex with Happy Ending • In Call and Out Call Service • 3* 5* 7* Hotels Service • 24 Hours Available • Indian, Russian, Punjabi, Kashmiri Escorts • Real Models, College Girls, House Wife, Also Available • Short Time and Full Time Service Available • Hygienic Full AC Neat and Clean Rooms Avail. In Hotel 24 hours • Daily Escorts Staff Available • Minimum to Maximum Range Available.c

Vip profile Call Girls In Lonavala 9748763073 For Genuine Sex Service At Just...

Monika Rani

Unit5-Cloud.pptx for lpu course cse121 o

ManavSingh202607

biology HL practice questions IB BIOLOGY

1301aanya

module for grade 9 for distance learning

levieagacer

Module for Grade 9 for Asynchronous/Distance learning

levieagacer

Kochi CALL GIRL 84099*07087 ❤CALL GIRLS IN Kochi ESCORT SERVICE❤CALL GIRL IN We are Providing :- ● – Private independent collage Going girls . ● – independent Models . ● – House Wife’s . ● – Private Independent House Wife’s ● – Corporate M.N.C Working Profiles . ● – Call Center Girls . ● – Live Band Girls . ●- Foreigners & Many More . Service type: 1.In call 2.out call 3. full Lip to Lip kiss 4.69 5.b-job without Condom 6. Hard Core sex & Much More. 7 Body to Body Touch 8 Kissing 9 Sucking Boobs and More 10 Enjoy by Hand 11 Relax By Oral 12 Sex with Happy Ending • In Call and Out Call Service • 3* 5* 7* Hotels Service • 24 Hours Available • Indian, Russian, Punjabi, Kashmiri Escorts • Real Models, College Girls, House Wife, Also Available • Short Time and Full Time Service Available • Hygienic Full AC Neat and Clean Rooms Avail. In Hotel 24 hours • Daily Escorts Staff Available • Minimum to Maximum Range Available.

Kochi ❤CALL GIRL 84099*07087 ❤CALL GIRLS IN Kochi ESCORT SERVICE❤CALL GIRL

kantirani197

Zoology 5th semester notes( Sumit_yadav).pdf

Sumit Kumar yadav

low price Call me 7857803690 100%genuine sexy VIP call girl safe service WhatsApp chat. 785780369 Normal call kijiye 7857803690 100% genuine young college girl and housewife Full enjoy open minded girl provide 24hour full cooperative model and full satisfactions☎️*78578//03690*⭐Escorts service █▬█⓿▀█▀ call girls and bhabhi available for room Sex and video call service A-1 HIGH CLASS CALL GIRLS TOP MODEL 24X7 HOME/HOTEL Call Girls Safe & Secure High Class Sm Affordable Rate 100% Satisfaction, Unlimited Enjoyment. Any Time for Model/Escort in High class luxury and premium

SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICE

ayushi9330

IDENTIFICATION OF THE LIVING- forensic medicine

sherlingomez2

Recently uploaded (20)

Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b

STS-UNIT 4 CLIMATE CHANGE POWERPOINT PRESENTATION

PSYCHOSOCIAL NEEDS. in nursing II sem pptx

Clean In Place(CIP).pptx .

Seismic Method Estimate velocity from seismic data.pptx

Chemical Tests; flame test, positive and negative ions test Edexcel Internati...

Formation of low mass protostars and their circumstellar disks

Pests of mustard_Identification_Management_Dr.UPR.pdf

GBSN - Microbiology (Unit 3)

Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds

GBSN - Biochemistry (Unit 1)

Vip profile Call Girls In Lonavala 9748763073 For Genuine Sex Service At Just...

Unit5-Cloud.pptx for lpu course cse121 o

biology HL practice questions IB BIOLOGY

module for grade 9 for distance learning

Module for Grade 9 for Asynchronous/Distance learning

Kochi ❤CALL GIRL 84099*07087 ❤CALL GIRLS IN Kochi ESCORT SERVICE❤CALL GIRL

Zoology 5th semester notes( Sumit_yadav).pdf

SAMASTIPUR CALL GIRL 7857803690 LOW PRICE ESCORT SERVICE

IDENTIFICATION OF THE LIVING- forensic medicine

SUSY in d=3, N=2

Recommended

Recommended

More Related Content

Viewers also liked

Viewers also liked (16)

More from Flip Tanedo

More from Flip Tanedo (20)

Recently uploaded

Recently uploaded (20)