Title Text

 

University of Delaware

Department of Physics and Astronomy

 

federica bianco

she/her

Biden School of Public Policy and Administration

Data  Science Institute

I am trained as an astrophysicst

1/2 million hours of star light with 5 measurements per second

9,000,000,000 data points

220 hours of star light with 30 measurements per second

158,400,000 data points

brightness

(arbitrary units)

star 1

star 2

brightness

(arbitrary units)

star 1

star 2

star 1

star 2

1/2 million hours of star light with 5 measurements per second

9,000,000,000 data points

220 hours of star light with 30 measurements per second

158,400,000 data points

NULL RESULTS ARE KEY SCIENTIFIC RESULTS!

prediction from solar system formation models

Reason to study Supernovae

SN are enable life in the Universe

 

 

SN are natural extreme physics laboratories

 

 

SN trace the evolution of the Universe

we are made of stars

“The nitrogen in our DNA, the calcium in our teeth, the iron in our blood, the carbon in our apple pies were made in the interiors of collapsing stars.

We are made of starstuff.”

Carl Sagan, Cosmos

...a highly visible feminist who never lifted a finger around the house and paid scant attention to the needs of first-wife [Lynne] Margulis, [an evolutionary biologist,] whose career would one day rival his own...

https://www.americanscientist.org/article/carl-sagan-carl-sagan-biographies-echo-an-extraordinary-life

Elements up to iron are forged in star cores.

Iron is so tightly bound that it absorbs energy instead of generating it in fusion : temperature drops instead of rising, gravitational pressure wins

I. we are made of star dust

lives of stars

\mathrm{life}_\mathrm{Sun} = \mathrm{10 ~Billion~ years}

Massive stars

live fast die young

lives of stars

lives of stars

\mathrm{life}_\mathrm{Sun} = \mathrm{10 ~Billion~ years}
\mathrm{life}_\mathrm{Star} = \left(\frac{M_\mathrm{Sun}}{M}\right)^{2.5} {\mathrm{life}_\mathrm{Sun}}

Massive stars

live fast die young

lives of stars

lives of stars

\mathrm{life}_\mathrm{2xSun} = \mathrm{~1.5 ~Billion~ years}
\mathrm{life}_\mathrm{Sun} = \mathrm{10 ~Billion~ years}
\mathrm{life}_\mathrm{Star} = \left(\frac{M_\mathrm{Sun}}{M}\right)^{2.5} {\mathrm{life}_\mathrm{Sun}}

Massive stars

live fast die young

lives of stars

lives of stars

\mathrm{life}_\mathrm{100xSun} = \mathrm{~300,000~ years}
\mathrm{life}_\mathrm{2xSun} = \mathrm{~1.5 ~Billion~ years}
\mathrm{life}_\mathrm{Sun} = \mathrm{10 ~Billion~ years}
\mathrm{life}_\mathrm{Star} = \left(\frac{M_\mathrm{Sun}}{M}\right)^{2.5} {\mathrm{life}_\mathrm{Sun}}

….. live to be old and die peacefully by slowly cooling down

low initial mass

0.1-8 MSun

lives of stars

UNLESS...

low initial mass

0.1-8 MSun

lives of stars

low initial mass but with a sibling 

even a low mass start will explode if its in a binary system and captures mass from the companion

lives of stars

II. understanding extreme physics

largest explosion on earth 10,000,000 erg

typical SN 10,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,000,00 erg

II. understanding extreme physics

largest explosion on earth 10,000,000 erg

typical SN

II. understanding extreme physics

largest explosion on earth 10,000,000 erg

typical SN

White Dwarf: supported by electron degenerate pressure - The Pauli exclusion principle states that no two electrons with the same spin can occupy the same energy state in the same volume.

Maximum mass: Chandrasekhar limit M = 1.44 MSun

Neutron star: supported by neutron degenerate pressure - The Pauli exclusion principle exists for neutrons as well.

 

1 Earth radius

size of manhattan

Black hole

star remnants:

           extreme physics environments

III. they tell us fundamental things about the Universe

Farthest SN

 

10.5 billion years ago

 

3 billion years after the Big Bang

 

redshift 4

 

 

 

who 'sploded??

1 SN / 100 years / galaxy

Building a legacy:

The Vera C. Rubin Observatory LSST

 

what's in a name?

The first ground-based national US observatory named after a woman, Dr. Vera C. Rubin 

The first ground-based national US observatory named after a woman, Dr. Vera C. Rubin

Pioneered the study of Dark Matter

The DOE LSST Camera - 3.2 Gigapixel

3024 science raft amplifier channels

Camera and Cryostat integration completed at SLAC in May 2022,

Shutter and filter auto-changer integrated into camera body

LSSTCam undergoing final stages of testing at SLAC

artist (me) impression of the first image taken by ComCam

it takes a village - many villages - the whole world!

400 hours of 4k HD videos or 1,000,000 typical TikTok videos every night

made with gemini AI

(not sure what is up w the nose or the third arm....)

Dr. Somayeh Khakpash (she/her), postdoc at UD, 

now LSSTC Catalyst Fellow, Rutgers

Can AI replace forward modeling of physical processes?

Many problems in astrophysics require expensive simulations.

Willow Fox Fortino (they/them), UD grad student

solving "who'sploded" with transformer AI

this one was a star 10 times more massive than the sun!

Continuous readout astronomical data for fast evolving transients (now with AI!)

Shar Daniels (they/them)

NSF GRFP Fellow

Multi City Urban Observatory

Director Greg Dobler, Biden School of Public Policy and Administration

REVA KAY WILLIAMS

first Black-American woman to receive a PhD in astrophysics

former professor at UD

Who's left behind

"an ideology that focuses on individual accumulation, capital, and individuality, rather than on redistributing power or reconsidering existing structures."

Focusing on equipping individuals to overcome the barriers to success imposed by the status quo, instead of dismanteling discriminatory structures

22 black women PhD in astro across the USA in 2022

having so little diversity shelters STEM from the reality of racism

Dr. Raven Baxter

The first ground-based national US observatory named after a woman, Dr. Vera C. Rubin 

The first ground-based national US observatory named after a woman, Dr. Vera C. Rubin

Who's left behind

FEMMINIST

Feminist: the person who believes in the social
Political, and economic equality of the sexes

Beyonce'

What has feminism been about? its been about contesting a received idea of what a woman is.

 

we wanted to call into questions these presuppositions that had been taken for granted for too long

 

so we ask the question "what does it mean to be a woman" ?

 

its a question of history, its a question of freedom

 

feminism always left the question open and refused to answer it on principle

 

Judith Butler, author of "Gender Trouble"

You do you

Dont give it for granted

In 1919, Afghan women were granted the right to vote.

In 1920 the first school for girls opened its doors.

 

In the 1970s, the Afghan government raised the marriage age for women from 18 to 21, abolished polygamy and introduced compulsory education.

In the 1970’s, women made up a significant proportion of all teachers and a significant percentage of doctors and civil servants.

 

In 2021, before the Taliban regime, women formed 27% of the Members of Parliament in Afghanistan

© Getty Images

The board of directors of "Jam'iat e nesvan e vatan-khah", a women's rights association in Tehran (1923–1933)

Iranian newspaper clip from 1968 reads:

"A quarter of Iran's Nuclear Energy scientists are women"

thank you!

 

University of Delaware

Department of Physics and Astronomy

 

Biden School of Public Policy and Administration

Data  Science Institute

federica bianco

fbianco@udel.edu

UDinnovateher2025

By federica bianco

UDinnovateher2025

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