Selected Publications

We report a precision measurement of the parity-violating asymmetry A PV in the elastic scattering of longitudinally polarized electrons from Pb 208. We measure A PV= 550±16 (stat)±8 (syst) parts per billion, leading to an extraction of the neutral weak form factor F W (Q 2= 0.00616 GeV 2)= 0.368±0.013. Combined with our previous measurement, the extracted neutron skin thickness is R n− R p= 0.283±0.071 fm. The result also yields the first significant direct measurement of the interior weak density of Pb 208: ρ W 0=− 0.0796±0.0036 (exp)±0.0013 (theo) fm− 3 leading to the interior baryon density ρ b 0= 0.1480±0.0036 (exp)±0.0013 (theo) fm− 3. The measurement accurately constrains the density dependence of the symmetry energy of nuclear matter near saturation density, with implications for the size and composition of neutron stars.
Physics Review Letters

The Qweak experiment has made possible the first determination of the weak charge of the proton QWp by incorporating earlier parity-violating electron scattering (PVES) data at higher Q2 to constrain hadronic corrections. The value of QWp obtained in this way is QWp(PVES)=0.0719±0.0045, which is in good agreement with the standard model prediction of QWp(SM)=0.0710±0.0007.
Nature

The experiment provides a measurement of the parity-violating asymmetry in electron–quark scattering, which yields a determination of $2C_{2u} − C_{2d}$ (where u and d denote up and down quarks, respectively) with a precision increased by a factor of five relative to the earlier result. These results provide evidence with greater than 95 percent confidence that the C2q couplings are non-zero, as predicted by the electroweak theory.
Nature Journal

The Qweak experiment has made possible the first determination of the weak charge of the proton QWp by incorporating earlier parity-violating electron scattering (PVES) data at higher Q2 to constrain hadronic corrections. The value of QWp obtained in this way is QWp(PVES)=0.064±0.012, which is in good agreement with the standard model prediction of QWp(SM)=0.0710±0.0007.
Physics Review Letters

The skin thikness of 208Pb, difference between the radii of the neutron and proton distributions Rn - Rp = 0.33 +0.16 -0.18 fm and provides the first electroweak observation of the neutron skin which is expected in a heavy, neutron-rich nucleus.
Physics Review Letters

Recent Publications

  • Accurate Determination of the Neutron Skin Thickness of through Parity-Violation in Electron Scattering

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  • Precision measurement of the weak charge of the proton

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  • Measurement of parity violation in electron–quark scattering

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  • First Determination of Weak Charge of Proton

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  • Measurement of the Neutron Radius of 208Pb Through Parity-Violation in Electron Scattering

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Recent & Upcoming Talks

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Research

P2 Experiment

The Qweak experiment at Jefferson Lab is making the first direct measurement of the weak charge of the proton, $ Q^p_W$.

For Prospective Students

For Prospective Students

Current Activities

Current Activities

The MOLLER experiment

The MOLLER experiment at Jefferson Lab will measure the weak charge of the electron, $ Q^e_W = 1 - 4 sin^2 \theta_W $

PREX/CREX Experiments

Extract a model independent measurement of the neutron skin thickness of the $ m ^{208}Pb$ and $ m ^{48}Ca$ nuclei

QWEAK Experiment

The Qweak experiment at Jefferson Lab is making the first direct measurement of the weak charge of the proton, $ Q^p_W$.

My Research

Precision measurements of the SM predicted quantities can be used to test the SM and discover new physics interactions beyond the SM.

My Citations

Google Scholar Profile

Deep Learning

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External Project

An example of linking directly to an external project website using external_link.

Outreach

Louisiana Science Olympiad (B & C) Invitational 2019

Louisiana Tech hosted the ONLY Science Olympiad invitational in the state on Saturday, January 26, 2019. I have volunteered to make Astronomy (division C) and Solar system (division B) competition.

Astronomy (division C) invitational Exam

Astronomy (division C) invitational Exam Key

Solar system (division B) invitational Exam

Solar system (division B) invitational Exam Key

Rakitha S. Beminiwattha at Louisiana Science Olympiad (B & C) Invitational 2019 during January 26, 2019

CosmicPi: Building the world’s largest distributed cosmic ray detector

I’m collaborating with a group of people from CERN to build the world’s largest open source distributed cosmic ray telescope. We are using our spare time to build Cosmic Pi, a cosmic ray detector based on a Raspberry Pi. The goal is to crowdsource the world’s largest cosmic ray telescope by getting the devices into the hands of people and organisations around the globe and then collecting data that will help astrophysicists understand more about cosmic rays. CosmicPi detector

The CosmicPi detector aims to fulfill the following features:

  • Detects cosmic muons and shares the events on the internet
  • All contained in a small, pocket sized box.
  • Low-cost at a $350 budget
  • Capable of detecting Muons of cosmic origin, mean energy 2.4 GeV using an organic plastic scintillator.
  • Fitted with a GPS receiver, altitude sensor, accelerometer and magnetometer to locate cosmic rays in time and space with high precision.
  • Accessible over Wi-Fi via a web-interface.
  • Open source in all aspects

More information CosmicPi main page

Volunteering for Hour of Code

It is vital to have a globally competitive STEM workforce in the USA. I’m committed to volunteer at public schools and other outreach programs to teach computer science related subjects for students at all ages. Volunteering for the Hour of Code during December 5-11, 2016 at the Lincoln Preparatory School, Grambling, LA Rakitha S. Beminiwattha at Hour of Code during December 5-11, 2016 at the Lincoln Preparatory School, Grambling, LA

Adopt-A-Physicist

Volunteering my time for Adopt-a-Physicist program organized by Sigma Pi Sigma society at APS. It connects high school students to real physics graduates and PI has been volunteering for this program for three years and will continue to participate. I have been volunteering for four years now. Rakitha S. Beminiwattha certificate of participation for Adopt-a-Physicist 2016

Teaching

Advanced Electronic Laboratory

Material Course
Syllabus Syllabus
Grade Rubric Rubric
Lab 1 Lab 1
Lab 2 Lab 2
Lab 3 Lab 3
Lab 4 Lab 4
Lab 5 Lab 5
Lab 6 Lab 6
Lab 7 Lab 7
Lab 8 Lab 8

Advanced Electromagnetic Laboratory

Material Course
Syllabus Syllabus
Grade Rubric Rubric
Lab 1 Lab 1
Lab 2 Lab 2
Lab 3 Lab 3
Lab 4 Lab 4
Lab 5 Lab 5
Lab 6 Lab 6
Lab 7 Lab 7
Lab 8 Lab 8

Undergraduate Teaching List

Quarter Course
Winter 17 Introduction to Physics I (Algebra based) PHYS 209 - Syllabus
Spring 17 Introduction to Physics II (Algebra based) PHYS 210 - Syllabus
Fall 17 Introduction to Physics II (Algebra based) PHYS 210 - Syllabus
Winter 18 Electronics Lab PHYS 404 - Syllabus
Spring 18 Electromagnetics Lab PHYS 405 - Syllabus
Fall 18 Introduction to Physics I (Algebra based) PHYS 209 - Syllabus
Winter 19 Introduction to Physics I (Algebra based) PHYS 209 - Syllabus
Spring 19 Introduction to Physics I (Algebra based) PHYS 209 - Syllabus

List of resources

PhET Simulation List

Science of NFL

Science of NHL

Science of NASCAR

An Example of Interactive Physics Simulations developed at University of Colarado

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